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"Response ID","Date Submitted","First Name:Author","Last Name:Author","ORCID iDWhat's This?:Author","Affiliation:Author","Co-Author 1:Given name(s):If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 2:Given name(s):If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 3:Given name(s):If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 4:Given name(s):If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 5:Given name(s):If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 1:Family name(s):If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 2:Family name(s):If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 3:Family name(s):If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 4:Family name(s):If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 5:Family name(s):If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 1:ORCID iD:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 2:ORCID iD:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 3:ORCID iD:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 4:ORCID iD:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 5:ORCID iD:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 1:Email:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 2:Email:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 3:Email:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 4:Email:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 5:Email:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 1:Affiliation:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 2:Affiliation:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 3:Affiliation:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 4:Affiliation:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","Co-Author 5:Affiliation:If you have five or fewer co-authors provide their information here. Please fill in as much information as you have available, and leave unknown or inapplicable cells blank.","1:If you have six or more co-authors please download this form, complete it, and upload here. ","Pick at most two of the following main topics for your white paper.","From your previous selections, pick at most two of the following subcategories for Basic Research.","Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment:From your previous selections, pick at most two of the following subcategories for Basic Research.","Other - Write In:From your previous selections, pick at most two of the following subcategories for Basic Research.","From your previous selections, pick at most two of the following subcategories for Space Weather Applications.","Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment:From your previous selections, pick at most two of the following subcategories for Space Weather Applications.","Other - Write In:From your previous selections, pick at most two of the following subcategories for Space Weather Applications.","From your previous selections, pick at most two of the following subcategories for Infrastructure, Workforce, Other Programmatic.","Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment:From your previous selections, pick at most two of the following subcategories for Infrastructure, Workforce, Other Programmatic.","Other - Write In:From your previous selections, pick at most two of the following subcategories for Infrastructure, Workforce, Other Programmatic.","Does your white paper include a notional concept for a ground- or space-based mission or project? (can choose both)","White Paper Title","Short Description (400 character limit)","1:Upload White Paper "
"2","11 July 2022 5:10:42 am","Andre","Galli","0000-0003-2425-3793","University of Bern, Switzerland","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F208-e25f602a148b553c1f0e4088ffd6de9a_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","Measuring interstellar neutrals in-situ: a critical contribution to heliospheric science","A near-term Interstellar Probe would enable in-situ measurements of the interstellar gas all the way from the Earth to the heliosheath and beyond the reaches of the heliopause. These revolutionary measurements would reveal how the interstellar medium is filtrated and deflected by our heliosphere and the chemical and isotopical composition of the interstellar medium itself.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F241-bc48b8849760632d651c51b37c99ba04_GalliAndre.pdf"
"3","11 July 2022 1:06:35 pm","Liliana","Liliana Rivera","","TECNOLOGICO NACIONAL MARIO MOLINA PASQUEL Y HENRIQUEZ","","","","","","","","","","","","","","","","","","","","","","","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","catalogue solar","catalogue for solar filaments that is available and offers consistent data for future studies of filaments evolution. A sequence of Interactive Data Language (IDL) and Python scripts was developed in order to obtain the catalogue. Our database was compiled for the first two years of the solar cycle 25, respectively, for 2020 and 2021 (January to September). ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-bea4c97a9b5903a5f0dc78ba1f2f26ef_Liliana_Rivera_Asturias_whitepaper.pdf"
"4","21 July 2022 9:39:34 am","Fabrizio","Sassi","0000-0002-9492-7434","Naval Research Laboratory","Manbharat","Jens","Douglas","","","Dhadly","Oberheide","Rowland","","","0000-0003-0731-788X","0000-0001-6721-2540","0000-0003-0948-6257","","","[email protected]","[email protected]","[email protected]","","","Naval Research Laboratory","Clemson University","NASA/GSFC","","","","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","Other Space Weather","","","","","","Space-based","SassiFabrizio1.pdf","This white paper describes how neutral winds are critical to advance our current understanding of the physical processes in the upper atmosphere, underlying the basic foundation of the ionosphere and atmosphere interaction, and how the existing gaps in observations have hampered the efficacy of global space weather research and forecasting capabilities.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-3912faf7c1f955451e48e90ba595664a_SassiFabrizio1.pdf"
"5","20 July 2022 7:43:09 pm","Brian","Walsh","0000-0001-7426-5413","Center for Space Physics, Boston University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-f846043685224d8e0928572293d9e330_WalshBrianM1.xlsx","Basic Research","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","Scientific Priorities for the Solar Wind-Magnetosphere Interaction: A System-of-Systems Perspective","This white paper advocates for a cross-scaled and system approach to studying solar wind-magnetosphere coupling. To make substantive progress in understanding the solar wind-magnetosphere interaction we must understand the cross-scale coupling of physics with focus on meso- (larger than ion-scale, fractions of Earth radii) to macro- (global, over many Earth radii) scale and system response. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-aa1cedd2bbef3c216435e68162e3de99_WalshBrianM1.pdf"
"6","27 July 2022 10:27:52 am","Majd","Mayyasi","0000-0002-5663-602X","Boston University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-d58bf44bff945a457ec98d1a814fbf9e_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Space Weather Applications","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Outer Heliosphere","","","Other Space Weather","","","","","","Space-based","Measuring Neutral Hydrogen Properties in the Interplanetary Medium","This supports development and deployment-to-space of a high-resolution spectrograph to distinguish different populations of H atoms that directly interact at the interface of the heliosheath, the region where the solar wind is subsonic. Resulting science would support Voyagers, IBEX, IMAP, New Horizons, and Interstellar Probe mission observations, and improve characterization of the solar wind.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-eaaa2faa8886260a557e78c2b61f4958_MayyasiMajdA.pdf"
"8","27 July 2022 1:12:35 pm","David","Malaspina","0000-0003-1191-1558","University of Colorado, Boulder","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-689633cab7269086a22c8225023df4db_SSPH_White_Paper_Author_Information_Form_MalaspinaDavidM2.xlsx","Basic Research","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","An Implementation for the PILOT (Plasma Imaging LOcal and Tomographic experiment) Mission Concept","The Plasma Imaging LOcal and Tomographic experiment (PILOT) mission concept provides the transformational multi-scale observations needed to determine the pathways of mass and energy flow through the coupled systems of the terrestrial magnetosphere. This white paper describes a technical implementation of PILOT, including spacecraft bus, instrumentation, orbits, launch, and enabling technology.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F241-a1620e7391aacca56258e4fdae41e94c_MalaspinaDavidM2.pdf"
"9","30 July 2022 5:40:33 pm","Chester","Gardner","https://orcid.org/ 0000-0001-9765-8973","University of Illinois at Urbana-Champaign","Xinzhao","Daniel","John","Scott","Diego","Chu","Marsh","Plane","Bailey","Janches","","","","","","[email protected]","[email protected] < [email protected]>","John Plane < [email protected]>","Bailey, Scott < [email protected]>","Janches, Diego. (GSFC-6750) < [email protected]>","University of Colorado Boulder","National Center for Atmospheric Research","University of Leeds","Virginia Polytechnic Institute and State University","NASA-Goddard","","Basic Research","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","","","","","","","Ground-based;Space-based","Wave-induced Mixing and Transport in the Middle Atmosphere-Lower Thermosphere (MLT)","Although the major effects of wave forcing are known, there are still large uncertainties in the middle atmosphere-lower thermosphere circulation because the global distribution of gravity waves and their dynamical and thermal effects during dissipation and breaking, are poorly constrained by observations and only crudely parameterized in global circulation models. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F189-46bc253f577a66b2efae77b1e09b488b_GardnerChesterS.docx"
"10","3 August 2022 10:44:52 am","David","Hysell","0000-0001-7410-7335","Cornell University","Jorge","Marco","","","","Chau","Milla","","","","0000-0002-2364-8892","0000-0001-9067-863X","","","","[email protected]","[email protected]","","","","AIP Germany","PUCP Peru","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","An Ionospheric Modification Facility for the Magnetic Equator","This is a conceptual proposal for the deployment of an ionospheric modification facility, also called and HF facility or ionospheric heater, near the geomagnetic equator. A heater is a powerful high-frequency (HF), or shortwave, radio transmitter that can be used to induce a number of phenomena of importance to the solar-terrestrial research community.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F227-7bdd71ff7a2e7d06d3904eab357dd9b4_whitepaper_heater.pdf"
"11","4 August 2022 11:01:41 am","Jens","Oberheide","0000-0001-6721-2540","Clemson University","McArthur","Komal","","","","Jones Jr.","Kumari","","","","0000-0002-0569-0093","0000-0002-6192-3584","","","","[email protected]","[email protected]","","","","U.S. Naval Research Laboratory","Arizona State University","","","","","Basic Research","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","Resolving the tidal weather of the thermosphere","We reiterate on the urgent need for global wind measurements in the ~100-250 km region with at least four but preferably six local times per days. This would transform our understanding of how the magnetic control of ion-neutral interactions produces variability in the thermosphere, and how lower atmosphere and solar/geomagnetic forcing work together to produce quiet and storm time space weather. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F160-0767fd6be99581fb300d64de303ea29a_Resolving_the_tidal_weather_of_the_thermosphere_final.pdf"
"15","9 August 2022 12:07:34 pm","Rolando","Garcia","0000-0002-6963-4592","NCAR","Lynn","Erich","Chihoko","","","Harvey","Becker","Cullens","","","0000-0002-7928-0804","0000-0001-7883-3254","0000-0002-9951-9763","","","[email protected]","[email protected]","[email protected]","","","CU/LASP","NWRA","CU/LASP","","","","Basic Research","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","","","","","","","Space-based","Potential Consequences of Breaking of the Diurnal Migrating Tide","Breaking of the migrating diurna tide is a potential mechanism for the generation of ""secondary"" gravity waves that might couple the upper mesosphere with the ionosphere and seed phenomena such as TIDs and plasma bubbles.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-5e86ee70c44608f70d2e4c497c036031_GarciaRolando-DW1breaking.pdf"
"16","9 August 2022 5:21:39 pm","Stefan","Eriksson","0000-0002-5619-1577","University of Colorado Boulder","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-766bd0be61a60dffa7920447c6ae10a9_SSPH_White_Paper_Author_Information_Form_Eriksson.xlsx","Basic Research","Outer Heliosphere","","","","","","","","","Space-based","Magnetic Reconnection Science in the Outer Heliosphere","We propose an investigation on magnetic reconnection and its importance in understanding the dynamics and structure of the boundary regions of the outer heliosphere, where the heliosphere interacts with the local interstellar medium. Now is the time to launch an Interstellar Probe with modern instrumentation to address this objective and many others in the Heliophysics of the outer heliosphere.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F16-f0649ac0821357e3b8a400ec1ccee6c7_ErikssonStefan.pdf"
"17","11 August 2022 3:10:09 pm","Lynn","Wilson","0000-0002-4313-1970","NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD 20771, USA","Katherine","Drew","Ian","Phyllis","Steven","Goodrich","Turner","Cohen","Whittlesey","Schwartz","0000-0002-4288-5084","0000-0002-2425-7818","0000-0002-9163-6009","0000-0002-7287-5098","0000-0003-0682-2753","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","University of West Virginia, Department of Physics and Astronomy, Morgantown, WV, USA","he Johns Hopkins University, Applied Physics Laboratory, Laurel, MD, USA","he Johns Hopkins University, Applied Physics Laboratory, Laurel, MD, USA","Space Sciences Laboratory, University of California, Berkeley, Berkeley, CA, USA","Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Boulder, CO, USA","","Basic Research","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","Space-based","The necessity of accurate measurements of thermal velocity distribution functions in the solar wind","The current state of the art thermal particle measurements in the solar wind are insufficient to address many long standing, fundamental physical processes. The solar wind exhibits multiple particle populations for each particle species. We can resolve the electron populations but only separate the ion species. Thus, we are inherently limited in our understanding of the solar wind kinetics.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-2e3204740952c5a8bccc1914b3f1e56c_white_paper_decadal_2023.pdf"
"18","13 August 2022 8:48:25 am","ROMANA","RATKIEWICZ","0000-0002-0029-5836","Space Research Centre Polish Academy Of Sciences","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F160-4b97a610f8c27d080103abd31565c8da_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Outer Heliosphere;Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","Ground-based","Creating a new paradigm by modeling the interaction of the solar wind with the interstellar medium using a hybrid-kinetic model","The White Paper consists: The present state of knowledge. Where are the gaps and how to fill them? So what to do in the future? and answer: Develop the hybrid -kinetic model of the heliosphere. The role of Logistics in promoting the Space Research","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F93-74f8b7691a24b160c865eaf8f1d485c6_RatkiewiczRomanaE..pdf"
"19","13 August 2022 3:12:14 pm","Jia","Yue","0000-0003-0577-5289","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F246-833e0e9ffcbe755f4250462755e36b45_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Space-based","Characterization and understanding of the lower thermosphere circulation —the new frontier in the ionosphere thermosphere mesosphere system","In this paper we lay out the suggested modeling, observations, and scientific questions for the decadal survey to fill the knowledge gap in our understanding of this lower thermosphere circulation and the dynamics in this region as a whole due primarily to lack of observations. We propose here that NASA solicit mission proposals to measure global winds and trace gasses densities at 100-150 km. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-bb0b2de10960702abc663a3d8b2a9f01_JiaYue_LTC_white_paper_complete_v3.docx"
"20","15 August 2022 4:56:35 pm","Anne","Smith","0000-0003-2384-5033","National Center for Atmospheric Research","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F246-54545ebb8f095401ef22d3b31578382a_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","Measurements of the mean structure, temperature, and circulation of the MLT","The mean state of the MLT (mesosphere - lower thermosphere) is key in the exchange of energy, momentum, and trace species between the middle and upper atmosphere. Knowledge of the mean state wind and temperature is endangered by an upcoming gap in measurements. Needed actions include continued operation of existing space-borne instruments and rapid development of replacement options.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-dcbb61e823c9456e3caa49e9b400ae4b_SmithAnneK.pdf"
"21","16 August 2022 3:19:43 pm","Jeffrey","Hayes","0000-0003-1001-349X","NASA Science Mission Directorate & Space Communications and Navigation Organization.","Gregory","Erica","","","","Heckler","Weir","","","","","","","","","","","","","","","","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","Ground-based;Space-based","NASA's Space Communications & Navigation Program's available services and future plans.","The Space Communications and Navigation Program has assembled this white paper to provide an overview of the communications and tracking services that are so pivotal to the success of NASA science endeavors, and to provide insight into future plans, including the use of commercial services in the near-Earth domain, upgrades to the deep space infrastructure, and access to radio frequency spectrum.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-1d989fb724c9c610ae8a09aec9ab51b1_SCaN_White_Paper_for_SMD_Decadals_Input_Final.pdf"
"22","16 August 2022 4:45:11 pm","James","Burch","orcid.org/0000-0003-0452-8403","Southwest Research Institute","Harald","Stephen","William","Robert","","Frey","Mende","Lotko","Ergun","","0000-0001-8955-3282","0000-0001-5511-3668","0000-0002-3859-1593","0000-0002-3096-8579","","[email protected]","[email protected]","[email protected]","[email protected]","","University of California, Space Sciences Laboratory, Berkeley, CA","University of California, Space Sciences Laboratory, Berkeley, CA","Dartmouth College, Hanover, NH","University of Colorado, LASP, Boulder, CO","","","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","BurchJamesL.docx","Observatory for Heteroscale Magnetosphere-Ionosphere Coupling (OHMIC) is a moderate four-spacecraft mission combining high-time-resolution plasma and fields measurements in the auroral acceleration region with high-resolution local and global auroral imaging to determine the processes by which electromagnetic energy is converted into kinetic energy of charged particles in a collisionless plasma.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-77bcd2c87e3bd4100e94ad7ba32222bb_BurchJamesL.docx"
"23","17 August 2022 4:31:04 am","Robert F.","Wimmer-Schweingruber","0000-0002-7388-173X","Christian-Albrechts-University, Kiel","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-ca88d2ab1b5f324a154654ef86d11226_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","STELLA - In situ Investigations of the Very Local Interstellar Medium","Voyager 1 & 2, Ulysses, Cassini, and IBEX have shown that the interaction between interstellar medium and solar wind is much more complex and involved than previously believed. This whitepaper proposes to study this interaction in situ at the heliospheric boundaries and to explore the very local interstellar medium beyond with new instrumentation that is built to investigate this final frontier. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-435289c96a6d9ead2a4eb8369be8874b_Wimmer-SchweingruberRobertF.pdf"
"24","17 August 2022 3:35:36 pm","Amy","Keesee","0000-0002-9719-3229","University of New Hampshire","Earl","","","","","Scime","","","","","","","","","","[email protected]","","","","","West Virginia University","","","","","","Basic Research;Space Weather Applications","Planetary Magnetospheres;Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop","","","","","","Space-based","KeeseeAmyM1","Technology development needed to enable magnetosphere missions: While some progress in technology described in the previous Decadal Survey and Heliophysics Roadmap have been made, continued work and support is needed in the coming decade to realize missions described in the previous Decadal Survey as well as new mission concepts, particularly constellation missions. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F160-63da01ffe42bde655932b27d78a099cb_KeeseeAmyM1.pdf"
"25","19 August 2022 2:12:42 pm","James","Green","0000-0002-4625-9216","NASA Headquarters","Chuanfei","Michael","C. Alex","Vladimir","","Dong","Hesse","Young","Airapetian","","","","","","","[email protected]","[email protected]","[email protected]","vladimir.airapetian","","Princeton University","NASA Ames Research Center","NASA Goddard Space Flight Center","NASA Goddard Space Flight Center","","","Space Weather Applications","","","","Space Weather Pipeline from Research to Application to Operations;Other Space Weather","","","","","","Ground-based;Space-based","Space Weather Observations, Modeling, and Alerts in Support of Human Exploration of Mars","Space Weather (SW) observations and modeling at Mars have begun but it must be significantly increased to support the future of Human Exploration on the Red Planet. the next Heliophysics Decadal Survey must include a new initiative to meet expected demands for SW information in support of humans traveling to and living and working on the surface of Mars.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-0bb604cb23579a30145fb914bb1f5cd7_GreenJamesL.pdf"
"27","19 August 2022 5:17:54 pm","Juan","Rodriguez","","University of Colorado CIRES","J. Scott","Jerry","Phillip","","","Evans","Lumpe","Oakley","","","","0000-0002-8754-702X","","","","[email protected]","[email protected]","[email protected]","","","Computational Physics, Inc.","Computational Physics, Inc.","Ball Aerospace","","","","Basic Research;Space Weather Applications","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment;Other Space Weather","","","","","","Space-based","Continuous Global Far Ultraviolet Auroral and Thermospheric Imagery from a Highly Elliptical Orbit","Continuous Global Auroral Imaging provides key forecasting information for space weather events and their effect on technology and infrastructure. This includes geomagnetically induced currents in power grids, spacecraft surface charging, and satellite drag. With two spacecraft per hemisphere in a highly elliptical Tundra orbit we can provide high resolution auroral and thermospheric imagery.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-b513b4c2fc4e6c9953bed0e78fb66d39_RodriguezJuan.pdf"
"28","19 August 2022 6:30:29 pm","Jennifer","Gannon","","Computational Physics, Inc.","","","","","","","","","","","","","","","","","","","","","","","","","","","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","NOAA’s Space Weather Prediction Testbed: Our community’s interface to the space weather end user","The NOAA Space Weather Prediction Testbed (SWPT) and related efforts should be a priority for heliophysics throughout the next decade.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F239-b3d646d2efa6ffbbf379127238a2e999_GannonJenniferL1.pdf"
"29","19 August 2022 6:55:16 pm","Jennifer","Gannon","","Computational Physics, Inc.","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F239-7db70c07c01a0c28fe83995445c164a0_SSPHWhitePaperAuthorInformationForm.xlsx","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","Other Programmatic","","","Ground-based;Space-based","Funding Expansion for NASA Space Weather R2O","An expanded budget is needed for the newly-formed NASA Heliophysics Space Weather Program, at a level of $100-200M per year, in parity with the budgets of LWS and STP, and consistent with the recommendations of the previous Decadal Survey. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F239-7c817ce5baac46903f493e283de3d952_GannonJenniferL2.docx"
"30","20 August 2022 8:05:58 am","V Lynn","Harvey","0000-0002-7928-0804","Laboratory for Atmospheric and Space Physics, University of Colorado Boulder","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F187-5d3792fd15da96e8879c1fd740f96ab8_SSPH_White_Paper_Author_Information_Form_Harvey.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","Improving ionospheric predictability requires accurate simulation of the mesospheric polar vortex","The mesospheric polar vortex plays a critical role in coupling the atmosphere-ionosphere system, so its accurate simulation is imperative for robust predictions of the thermosphere and ionosphere. Unfortunately, representation of the MPV is generally not accurate in state-of-the-art general circulation models.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-6a2769915587836f358507dbf714f593_HarveyVLynn.pdf"
"31","20 August 2022 11:48:25 pm","Jerry","Goldstein","0000-0002-6715-7083","Southwest Research Institute","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-f15ac91fe3512d8b5e083e77b7d69254_SSPH_White_Paper_Author__REFILLING.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","Geospace Core Plasma Supply and Refillling (CPSR): Science and Observations for the Next Decade","Geospace core plasma supply and refilling (CPSR) are fundamentally important, but fall within a major knowledge gap. Understanding the life cycle of this enormous plasma mass—as important to magnetospheric dynamics as solar-wind driving—has been hindered by the absence of primary cold plasma measurements. This white paper discusses CPSR science gaps and the needed new in-situ/imaging observations.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-33ae6e4d69534fbc6dc659ef0642b7bd_GoldsteinJerry1.pdf"
"32","20 August 2022 11:52:48 pm","Jerry","Goldstein","0000-0002-6715-7083","Southwest Research Institute","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-5888a6c737d714cba571faefe0d92f5a_SSPH_White_Paper_Author_SOURCE.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","Synchronized Observations of Upflow, Redistribution, Circulation, and Energization (SOURCE) mission concept","This white paper proposes the Synchronized Observations of Upflow, Redistribution, Circulation, and Energization (SOURCE) mission concept, a constellation of imaging & in situ observatories. SOURCE is a systems-level mission that targets the full life cycle of core plasma, from its ionospheric origin to its magnetospheric energization and impact. SOURCE comprises five (5) spacecraft.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F160-aaf6c9d630ff32fbbbfe284c6307fd27_GoldsteinJerry2.pdf"
"34","22 August 2022 4:23:44 am","Roberto","Guenzani","","NgEHT-TH","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research","Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","Space-based","Plasma Laws Fractionalization in Solar System and Anthropic Units","I propose multimessenger Heliophysics from Embodied Cognition by syntactic representation of information as a quantum process in Microgravity where Wavelength-Radiance stratified on Space Station orbits could unveil resonances. By Rigidity vs Fluidity, Parity violation weights Bootstrap for QCD-Solar Spectra, IFT-Neutrino Wind Mixing under Astropshere synchronism with BH Tanh amplification.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-6f65e6dbc9b732a0171f651d2a1d1141_GuenzaniRoberto.pdf"
"35","22 August 2022 10:08:28 am","Kareem","Sorathia","0000-0002-6011-5470","JHUAPL","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-c410dbb06751de99285202a052b321f4_SorathiaKareem.Authors.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Ground-based;Space-based","First-Principles Geospace Modeling in the Next Decade","In the next decade, we can build on advances in model sophistication and the power of exascale computing to create the first generation of cross-scale holistic geospace models. Accomplishing this will require a funding environment and heliophysics profession that can attract and retain a workforce spanning applied mathematics, physics, computer science, data science, and software engineering. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F85-2937ff419009cca0f8b66a92124aab95_SorathiaKareem.pdf"
"36","22 August 2022 12:35:37 pm","Federico","Gasperini","0000-0001-9754-5776","Orion Space Solutions","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-6868f3856cf310d1b3c459b2d9ada802_GasperiniFederico_WP_SSPH_Author_Information.xlsx","Basic Research","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","Ionosphere-Thermosphere-Mesosphere Variability imposed by Waves from Below in Future Climates","The structure and dynamics of the Ionosphere-Thermosphere-Mesosphere (ITM) system are significantly influenced by waves from the lower atmosphere. Understanding of the physical mechanisms at play and trends is impaired by data sparsity. This white paper reviews current knowledge in this area and highlights the importance and critical need for new, global, height-resolved observations of the ITM.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-8ae659fb154c7e9e6ac05fba6e9eb0b1_GasperiniFederico.pdf"
"37","22 August 2022 5:36:46 pm","Pawel","Swaczyna","0000-0002-9033-0809","Princeton University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-23c5d25c1b38534b0660368832e1cce0_SwaczynaPawel.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","Ubiquitous Nature of Pickup Ions in the Outer Heliosphere and Beyond","Interstellar pickup ions (PUIs) hold most of the internal solar wind pressure and are preferentially accelerated at shocks in the outer heliosphere. In the whitepaper, we briefly present limitation of existing PUI observations and identify related knowledge gaps. We recommend prioritizing a dedicated PUI instrument to observe PUIs in the heliosheath and beyond.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-9b61e0afa981fbd3730db8b9eb53c6db_SwaczynaPawel.pdf"
"38","22 August 2022 10:29:28 pm","Angelos","Vourlidas","0000-0002-8164-5948","JHU/APL","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-57a94667ec000765b1e4864f69624194_VourlidasAngelos1_WP_Author_Information.xlsx","Space Weather Applications","","","","Space Weather Research to Operations to Research Loop;Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","Space-based","Solving The Space Weather Problem: A 15+ Year Roadmap to Revolutionize Space Weather Research, Protect NASA Space Assets, and Enable Robust Operations","The White Paper (WP) describes a roadmap to address the Space Weather (SpWx) problem. It presents a strategic vision of how a community-wide effort could be organized and implemented to enable transformative advancement in SpWx research and ultimately, in applications. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-6b74be7b03cba2c398eb6044de466904_VourlidasAngelos1.pdf"
"39","23 August 2022 2:28:12 am","Devin","Huyghebaert","0000-0002-4257-4235","UiT The Arctic University of Norway","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-83ce067f57b68be323894d7e512b2604_HuyghebaertDevinR_white_paper_coauthors.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","The Future of Auroral E-region Plasma Turbulence Research","The heating caused by ionospheric E-region plasma turbulence has documented global implications for the energy transfer from space into the terrestrial atmosphere. It is proposed to enhance and expand existing ionospheric radar capabilities and fund research into investigating the effects of E-region plasma turbulence on the terrestrial magnetosphere, ionosphere, and neutral atmosphere.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-016e31fe6f77ecbf37764486861d9eed_HuyghebaertDevinR.pdf"
"40","23 August 2022 1:18:33 pm","Larry","Gordley","","GATS","Benjamin","David","","","","Marshall","Fritz","","","","","","","","","[email protected]","[email protected]","","","","GATS","GATS","","","","","Basic Research","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","DWTS (Doppler Wind and Temperature Sensor): A paradigm shift in remote sensing of winds and temperatures from low-Earth orbit","A major advance in global mesosphere and lower thermosphere (MLT) wind and temperature observation is ready to be demonstrated from LEO using an instrument named DWTS (Doppler Wind and Temperature Sounder). This white paper describes the DWTS concept, a soon to be launched pathfinder instrument and the goal of observing global MLT winds and temperatures using a constellation of DWTS CubeSats. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F239-f4dea72aea41a30a46ae906776c82a91_GordleyLarryL.pdf"
"42","23 August 2022 4:15:57 pm","Joseph","Smith","0000-0001-6489-4603","NeXolve","James","Brandon","Lynn","","","Moore","Farmer","Rodman","","","0000-0001-8860-2361","0000-0001-6256-6139","0000-0002-9803-5388","","","[email protected]","[email protected]","[email protected]","","","NeXolve","NeXolve","NeXolve","","","","Basic Research","Basic research that is driven by space weather user needs;Other topic relevant to solar and space physics/heliophysics","","","","","","","","","Space-based","Advancements in Thin Film Solar Array Technology to Enable Heliophysics Missions","Combining thin film solar array technology and solar sail technology will result in a large area thin film solar array that can achieve more than 300W/kg from a vehicle platform as small as a CubeSat. Investing in research and development projects that will close the technology gaps identified in this paper will enable future heliophysics missions to meet any high-power requirements.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-24706fff7aea1d967223c93f832b3439_SmithJosephC.pdf"
"43","23 August 2022 4:52:22 pm","Samuel","Maddox","0000-0003-4707-8692","NeXolve","James","Jim","","","","Moore","Pearson","","","","0000-0001-8860-2361","","","","","[email protected]","[email protected]","","","","NeXolve","NeXolve","","","","","Basic Research;Space Weather Applications","Basic research that is driven by space weather user needs;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Space-based","Advancements in Large Solar Sail Technology for Heliophysics Missions Requiring High Efficiency Propulsion and High Inclination Solar Orbits","This white paper advocates for the need of advanced research and development of large solar sails as the in-space propulsion system for heliophysics missions requiring high efficiency propulsion for space weather research, monitoring, and high inclination solar orbits.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-e3994b4a7a3145950ba6fab1d1fe7a6d_MaddoxSamuelK.pdf"
"44","23 August 2022 5:11:40 pm","Hanli","Liu","0000-0002-6370-0704","National Center for Atmospheric Research","Astrid","Nicholas","Kevin","John","","Maute","Pedatella","Pham","De","","0000-0003-3393-0987","0000-0002-8878-5126","","0000-0002-2119-8242","","[email protected]","[email protected]","[email protected]","[email protected]","","National Center for Atmospheric Research","National Center for Atmospheric Research","National Center for Atmospheric Research","National Center for Atmospheric Research","","","Basic Research","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","","From Mesoscale to Global Scales in Atmosphere-Geospace System: Research Enabled by Exascale Computing","Mesoscale processes impact atmosphere-geospace in fundamental ways. Capturing the interactions among different scales self-consistently on a system level requires a whole atmosphere modeling approach. Resolving mesoscale to global scales in such models will become feasible with exascale computing. We discuss the necessity, model readiness, and strategies to address key challenges in this effort.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F187-32a6b7eeffc826c3cc6e1cf14a74345b_LiuHanli.pdf"
"45","23 August 2022 5:18:04 pm","Michael","Taylor","","Utah State University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F239-64acd2c3cd9257b37f6bf9b6848ed29f_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Measurements of gravity wave global distributions and trends in the ITM"," Global measurements to characterize gravity wave (GW) parameters, distribution and main trends in the ITM are crucial. This white paper summarizes current GW measurement techniques operated from ground-based to space borne platforms. The capabilities and limitations of each technique are described & discussed. The gaps in current global GW measurements are identified and solutions are suggested. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F5-7c53e17e2800dd38bb2aebb1ccb7aa6f_TaylorMichaelJ.docx"
"46","23 August 2022 6:21:37 pm","Katariina","Nykyri","0000-0002-6905-9487","Embry-Riddle Aeronautical University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-68b4b8ca2caf1be1c9e77d40f37e2654_WP1_Science_Motivation_for_7_Sisters_Mission.xlsx","Basic Research","Laboratory space plasma physics;Basic research that is driven by space weather user needs","","","","","","","","","Space-based","Critical Solar Wind Measurements Required For the Next Generation Space Weather Prediction Mission: Science Motivation for the Seven Sisters Mission","This paper motivates new multi-point, multi-scale, critical measurements in the solar wind (SW) that are required to improve our fundamental understanding of the 3-D, large to intermediate-scale structures and processes in the SW; their azimuthal variation, radial evolution; and impact on particle acceleration, heating, and transport, thus motivating the Seven Sisters mission concept. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-5548346d581dadb6652266d428a79739_WhitePaperScience_v2-2.pdf"
"47","24 August 2022 10:44:27 am","Rebecca","Ringuette","0000-0003-0875-2023","ADNET Systems Inc, and NASA/GSFC/CCMC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-b92d886895ff4e8043ee654db861dc0f_RinguetteRebeccaA1_v2.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","Advocating for Equality of Contribution: The Research Software Engineer (RSE)","Heliophysics depends on RSEs to properly engineer software. However, RSEs receive unequal treatment compared to their science counterparts, resulting in unsustainable talent loss. These restrictions include lack of credit for their contributions and insufficient training. This paper describes what a RSE is and proposes solutions, including implementing appropriate recognition standards.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-44680fcb818f0e4cbcf3b492533c8bf0_RinguetteRebeccaA1_v2.pdf"
"48","24 August 2022 11:03:22 am","Rebecca","Ringuette","0000-0003-0875-2023","ADNET Systems, Inc and NASA/GSFC/CCMC","Ryan M.","Alexander","Thomas Y.","Barbara J.","","McGranaghan","Engell","Chen","Thompson","","0000-0002-9605-0007","0000-0001-9254-9057","","0000-0001-6952-7343","","[email protected]","[email protected]","[email protected]","[email protected]","","NASA/GSFC and Orion Space Solutions","NextGen Federal Systems","Columbia University","NASA/GSFC","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Developing a Vision for Heliophysics Infrastructure","The current infrastructure in heliophysics acts as a barrier towards progress due to the lack of intelligent connections between the many valuable resources in our field. Due to the large scale of this problem, the path to a productive infrastructure requires community collaboration towards a common vision. This white paper presents a broad overview of what that vision could be and a path forward.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-f3f2cf7376ca2d4ca7b9b12af810f537_RinguetteRebeccaA2.pdf"
"49","24 August 2022 11:17:59 am","David","Malaspina","0000-0003-1191-1558","University of Colorado","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-9ad6deb9f4b781b32695557b03723c21_SSPH_White_Paper_Author_Information_Form_MalaspinaDavidM.xlsx","Basic Research","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","'Follow the mass': the Science Case for Transformational Multi-scale Observations of Mass and Energy Flow Dynamics in Earth’s Magnetosphere","This paper describes the science motivation for transformational multi-scale observations of mass and energy flows in Earth's magnetosphere, demonstrating why this is a persistent and critical Heliophysics knowledge gap. A spaceflight mission concept, Plasma Imaging LOcal and Tomographic experiment (PILOT), is described, which can provide the observations required to close this knowledge gap. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-2ac31c9921d5b439b8bb0c64afd9380f_MalaspinaDavidM.pdf"
"50","24 August 2022 1:29:23 pm","Katariina","Nykyri","0000-0002-6905-9487","Embry-Riddle Aeronautical University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-0dcdd640cc90e39890f345da5fe232c3_WP2_7_Sisters_Mission_Concept.xlsx","Basic Research;Space Weather Applications","Laboratory space plasma physics;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Space-based","Seven Sisters–Pathfinder Mission to Protect Humanity from Space Weather","This white paper summarises the Seven Sisters solar wind (SW) mission concept and engineering report. The mission will collect critical measurements of the thermal and suprathermal plasma, and magnetic fields utilizing Venus-Sun Lagrange (VL) points, to resolve the science enabling eventual operational space weather mission and next generation space weather model development. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-5d12134c82d19aae688488d806a62088_Seven-Sisters-Space_Mission-Concept-Nykyri_NAS_Whitepaper.pdf"
"51","24 August 2022 8:00:26 pm","Stella","Ocker","0000-0002-4941-5333","Cornell University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-4ef62450b3d17ba24e42103b4b7bcfa1_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","","Heliosphere Meets Interstellar Medium, in a Galactic Context","The physical conditions within our heliosphere are driven by the Sun's motion through an evolving interstellar environment that remains largely unexplored. We discuss the critical science enabled by interdisciplinary studies that connect spacecraft observations of the heliosphere's immediate interstellar environment to remote observations of the interstellar medium and other star-ISM interactions.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-08b6d4fad9a8b4132d4c21d39d9fc93b_OckerStellaK.pdf"
"52","24 August 2022 10:12:41 pm","Shawn","Usman","0000-0002-3546-3967","Rhea Space Activity, Inc","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-b98fcc46063c95c900ff275976099d08_UsmanShawn1_WP_Author_Information.xlsx","Space Weather Applications","","","","Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","Space-based","Spitzer-Resurrector Mission: An Out-of-the-Box Approach for Space Weather Research & Operations","The Spitzer-Resurrector Mission (SRM) concept leverages an unusual funding opportunity, an interdisciplinary team from academia and industry, a novel mission design, and recent research and technical advances in Heliophysics to reach a cost-effective, yet innovative, solution to both research and operations gaps in SWx.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-10d2b3462a34c525f057e05c32f85e85_UsmanShawn1.pdf"
"54","24 August 2022 11:21:57 pm","Parisa","Mostafavi","0000-0002-3808-3580","Johns Hopkins University Applied Physics Lab","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-fe17bb9af7c45c5b7a0ffb38fc383892_Mostafavi_etal_Coauthor_form_decadal_2022.xlsx","Basic Research","Outer Heliosphere","","","","","","","","","Space-based","Shock Waves Propagation Beyond the Heliosphere: How Far Does the Sun’s Influence Extend into the Interstellar Medium?","This white paper is about the propagation of shock waves in the outer heliosphere and the very local interstellar medium (VLISM). We present how their structure would change as they propagate in different medium. We propose a need for a future dedicated mission to venture far from the Sun and make new discoveries about the shocks in the outer heliosphere and VLISM.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-93e64b05a72f6d8bc0e530572345f623_Mostafavi_shock_whitepaper_decadal.pdf"
"55","25 August 2022 11:44:49 am","Eric","Zirnstein","0000-0001-7240-0618","Department of Astrophysical Sciences, Princeton University","Daniel B.","Robert","Paul H.","","","Reisenfeld","DeMajistre","Janzen","","","0000-0003-1874-9450","0000-0003-0191-0287","","","","[email protected]","[email protected]","[email protected]","","","Los Alamos National Laboratory","Applied Physics Laboratory, Johns Hopkins University","Department of Physics and Astronomy, University of Montana","","","","Basic Research","Outer Heliosphere","","","","","","","","","Space-based","Revealing the 3D Structure of the Heliosphere through Long Baseline ENA Parallax and Tomography","Energetic neutral atoms (ENAs) are created in the solar-interstellar interaction, reflecting properties of the heliosphere. We demonstrate that with a spacecraft near the Sun and another on an interstellar-bound trajectory, the separation between them can be used to detect parallax motion of the Ribbon's source, and 3D tomography may be used to reconstruct the inner heliosheath source of ENAs.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-34cadfeee02b1f75b25efe2886f41ef7_ZirnsteinEricJ.pdf"
"56","25 August 2022 11:51:26 am","Kristina","Lynch","https://orcid.org/0000-0001-9006-1138","Dartmouth College","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-64a7ec2bc1ea14fd8a6688bf54dd539f_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Decadal Survey White Paper Reprising 2012 Decadal “Platforms” Working Group report: Infrastructure needs for optimal system science efforts","The previous Decadal Survey included a Working Group report on ""Explorers, Suborbital, and Other Platforms"", included in the Decadal as ""Appendix C"". The original working group members are listed below. While the detailed descriptions of specific platforms are now somewhat dated, the original motivation of support for diversified observational platforms remains and is even more important now.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-2422071c83fd773ff27f006ffecd0329_LynchKristinaA1.pdf"
"57","25 August 2022 3:50:16 pm","Andrew","Inglis","0000-0003-0656-2437","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-4a26443e5b7d580c0386414acdbe3ac2_author_information_InglisAndrewR.xlsx","Basic Research","Solar Physics","","","","","","","","","","Quasi-periodic pulsations in solar flares: a key diagnostic of energy release on the Sun","To fully understand solar flare energy release we require flare-focused rapid cadence multi-wavelength solar imaging, with sufficient sensitivity and dynamic range to observe quasi-periodic pulsations (QPPs). This must be combined with multidisciplinary funding and initiatives that will narrow the gap between numerical models of this fundamental phenomenon and observations.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-14925c20c2afecc566a2c5faf28cad5e_InglisAndrewR.pdf"
"58","25 August 2022 4:01:36 pm","Katherine","Goodrich","0000-0002-4288-5084","West Virginia University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-40462fed720a0889e7fba0aa39ae647d_SSPH_White_Paper_Author_Information_Form_goodrich.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","Space-based","The Persistent Mystery of Collisionless Shocks","The partitioning of energy down- stream of collisionless shocks is not well understood, nor are the processes which perform energy conversion. This paper stresses the need for the first ever spacecraft mission specifically designed and dedicated to the observation of both the terrestrial bow shock as well as Interplanetary shocks in the solar wind.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-9a7f17ef961a6fe2e2a8f549347062f5_MAKOS_Science_White_Paper_final.pdf"
"59","25 August 2022 8:53:03 pm","Mark","Cheung","0000-0003-2110-9753","Lockheed Martin Solar & Astrophysics Lab","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-58cfb2dafbf404754ece639679f5b25c_Magnetogram_whitepaper_author_form.xlsx","Basic Research;Space Weather Applications","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","Space Weather Research to Operations to Research Loop;Other Space Weather","","","","","","Ground-based;Space-based","Improved Observational Coverage of the Solar Magnetic Field","Full-disk magnetograms are only routinely available along the Sun-Earth line. The lack of 360 deg and 4pi steradian coverage introduces large systematic errors in models of the global coronal magnetic field, solar wind, coronal mass ejections and energetic particle events. A systems approach and community driven modeling effort is needed to determine a constellation mission to fill this gap.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-13ee0b3441684a79b329c45973407c4d_Whitepaper_for_the_Heliophysics_2024_Decadal_Survey.pdf"
"60","26 August 2022 9:25:41 am","McArthur","Jones Jr","https://orcid.org/0000-0002-0569-0093","U.S. Naval Research Laboratory","John","Quan","Jia","","","Emmert","Gan","Yue","","","","","","","","[email protected]","[email protected]","[email protected]","","","U.S. Naval Research Laboratory","LASP, University of Colorado Boulder","NASA Goddard Space Flight Center/Catholic University of America","","","","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","Other Space Weather","","","","","","Space-based","On the importance of neutral composition and temperature measurements in the 100-200 km altitude region","The purpose of this position paper is to highlight the importance and critical need for new, global, height-resolved neutral composition (O,O2,N2) and temperature measurements in the new ignorosphere: the 100-200 km region of the thermosphere.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-3d8b2959183926ed7961c022b69d7e9e_JonesJrMcArthur1.pdf"
"61","26 August 2022 3:53:49 pm","Hadi","Madanian","","University of Colorado Boulder","Randal","Robert","Shotaro","","","Bryant","Lillis","Sakai","","","","","","","","[email protected]","[email protected]","[email protected]","","","Carnegie Mellon University","University of California Berkeley","Tohoku University","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Increased Science Return of Long Duration Missions Exploring Distant Environments through Autonomous Spacecraft Design","This document describes the need for new initiatives by NASA to invest in enabling technologies. It describes some of the main technological obstacles in designing exploration missions that can consistently produce science results even at extremely far distances from Earth. It recommends solutions to overcome those obstacles that can be considered in future technology development efforts.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-a233a87a61720fbd43c8385563bb7e88_MadanianHadi1.pdf"
"63","26 August 2022 5:42:35 pm","Bryan","Holler","0000-0002-6117-0164","STScI","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-6e20aea24b3bd74563cdac4ce79369ae_HollerBryanJ_AuthorForm.xlsx","Basic Research","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Other topic relevant to solar and space physics/heliophysics","","","","","","","","","","Interstellar Probe at the Intersection of Heliophysics & Planetary Science: Probing Endo- & Exo-Heliospheric Environments with Trans-Neptunian Objects","While the near-term Interstellar Probe mission will revolutionize our understanding of our astrosphere, it will provide only a snapshot of the history of the heliosphere. Trans-Neptunian objects (TNOs), with numerous options located along any Interstellar Probe trajectory, provide an opportunity to study the history of the heliosphere using the colors, spectra, and geologies of their surfaces.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-9aeeb32d5ada790d5da9eba6b0eb73a6_HollerBryanJ.pdf"
"64","27 August 2022 5:05:04 pm","Richard","Eastes","0000-0003-3679-9793","Labortory for Atmospheric and Space Physics","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-cfb2958f3205a9d448c1a1c3a7102cbd_SSPH_White_Paper_Author_Information_Form_-_EastesRichardW.xlsx","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres","","","Space Weather Research to Operations to Research Loop;Other Space Weather","","","","","","Space-based","Geostationary Far Ultraviolet Imager for Space Weather Information and Science","Far Ultraviolet (FUV) remote sensing is a critical tool for providing data that is essential for advances in thermosphere-ionosphere (T-I) science. FUV remote sensing from geostationary Earth orbit benefits both space physics/heliophysics basic research and space weather research/application. Capabilities for both will be enhanced by hosting FUV imagers in separated, geostationary orbits. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-042b37a87acc0673d52aef9dfc6519a9_EastesRichardW.pdf"
"66","29 August 2022 10:05:42 am","McArthur","Jones Jr.","https://orcid.org/0000-0002-0569-0093","U.S. Naval Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-e1760e7adcbf4a2fb7b6d5c00a7d208f_SSPHWhitePaperAuthorInformationForm_JonesJrMcarthur2.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Other Programmatic","","","","Recommendations on Simple but Transformative Diversity, Equity, and Inclusion Measures in Heliophysics over the Next Decade","This position paper outlines three recommendations to make the Heliophysics community more diverse, equitable, and inclusive. These recommendations are: performing consistent collection and analysis of demographic data across different agencies, reimaging undergraduate heliophysics internships using the SOARS model, and providing conference funding for DEI speakers outside of Heliophysics.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-05d78f4f1c6d4828c0480b2c87c80c11_JonesJrMcArthur2.pdf"
"67","29 August 2022 10:45:59 am","Jonathan","Makela","0000-0002-9031-3080","University of Illinois Urbana-Champaign","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-53f5c3e166c561fcb7fff6aeb0b7286e_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Ground-based infrastructure for improved space weather specification at low latitudes","A notional deployment of a heterogeneous network of ground-based instrumentation is proposed. The scientific rationale for the deployment is to gain a comprehensive suite of measurements pertinent to improving our understanding of the longitudinal variability in the equatorial and low-latitude ionosphere/thermosphere system and the irregularities that can exist, therein. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-32e5e89b27fa838e558ff65531197e52_MakelaJonathanJ.pdf"
"68","29 August 2022 11:54:50 am","Justyna","Sokol","0000-0002-4173-3601","Southwest Research Institute, San Antonio, TX","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-39d6c6b2c42c5a15e124171c7908d8c6_SSPH_White_Paper_Author_Information_Form_SokolJustynaM.xlsx","Basic Research","Outer Heliosphere","","","","","","","","","Space-based","Measurements Beyond 1 au are Necessary for Exploration of the Outer Heliosphere and Local Interstellar Medium","Heliospheric missions operating in the outer heliosphere and beyond are necessary for understanding the heliosphere and its interstellar neighborhood","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-80a5744f5b720e267708a8aad8956d4c_SokolJustynaM.pdf"
"69","29 August 2022 12:52:00 pm","Seth","Claudepierre","0000-0001-5513-5947","UCLA","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-f8226592cb5c0f34aaf83c5c440bb309_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","","Scientific Priorities for the Earth’s Coupled Inner Magnetosphere: A System-of-Systems Perspective","We encourage our community to approach the science of the inner magnetosphere as a true system-of-systems (within the broader solar - solar wind - magnetosphere - ionosphere - atmosphere system-of-systems), combining advancement in new, fully-coupled systems modeling with cutting-edge data-driven analysis, and a new, coordinated and orchestrated series of missions. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-153c7a53844fa53bf7d2d8fa31ec0055_ClaudepierreSethG.pdf"
"70","29 August 2022 3:13:44 pm","Christopher","Bard","0000-0002-5926-0566","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-83c2dee410c570478b9aa4d27e8b460f_BardChris.Authors.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","","Building a Transdisciplinary, Exascale-Capable Workforce for Geospace Science","First-principles, self-consistent geospace modeling will require at least exascale-level computing capabilities. Taking full advantage of exascale resources requires both the creation of trans-disciplinary teams of physicists, computer scientists, data scientists, and applied mathematicians, and the stable, consistent, long-term support of these teams.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-3ebc19b6548bf9cb2e6cf114ea92d18d_BardChristopherM.pdf"
"71","29 August 2022 4:47:01 pm","Alphonse","Sterling","0000-0003-1281-897X","NASA/MSFC","Ronald","","","","","Moore","","","","","0000-0002-5691-6152","","","","","[email protected]","","","","","University of Alabama Huntsville","","","","","","Basic Research","Solar Physics","","","","","","","","","Space-based","Future High-Resolution and High-Cadence Observations for Unraveling Eruptive Solar Features","This White Paper proposes development of instrumentation focused on multi-wavelength observations of jet-sized-scale (base widths of a few tens to about 100 arcseconds) eruptive solar activity, as a window to understanding both larger-scale and smaller-scale eruptive solar events. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-ad8196fa57ed847241efefcfd0a78fcd_SterlingAlphonseC.pdf"
"72","29 August 2022 5:08:58 pm","Alex","Antunes","0000-0002-3098-2602","Johns Hopkins University Applied Physics Laboratory","Jon","Dmitriy","James","Kiley","Pontus","Vandegriff","Bekker","Mason","Yeakel","Brandt","0000-0002-0781-1565","0000-0002-0293-8938","0000-0002-3783-5509","0000-0002-2177-0579","0000-0002-4644-0306","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","Johns Hopkins University Applied Physics Laboratory","Johns Hopkins University Applied Physics Laboratory","Johns Hopkins University Applied Physics Laboratory","Johns Hopkins University Applied Physics Laboratory","Johns Hopkins University Applied Physics Laboratory","","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Research to Operations to Research Loop","","","Other Programmatic","","","","Smarter Onboard Science to Increase Science Yield","High resolution high cadence instruments create too much raw data , and science yield can be greatly increased with onboard smart processing to create high value data products. NASA can provide avenues for improving the TRLs for smarter onboard science through ROSES, facilitating research and publication, and encouraging how flight software can be updated during extended mission phases.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-2d52017a2804918ae74b88bb1e3d3c3d_AntunesAlexK.pdf"
"73","29 August 2022 5:38:27 pm","Robert","DeMajistre","https://orcid.org/0000-0003-0191-0287","The Johns Hopkins University Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-903120930c6bef21aa94acaa2334bbf7_DeMajistreRobertSSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","Sensing the Shape, Dynamics and Global Structure of the Heliosphere","We present here a means for unambiguously determining the shape, structure and solar cycle variation of our astrosphere via remote sensing measurements from vantage points well beyond the inner heliosphere. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-3374b0db3969b7adf91a741b2837c68f_DeMajistreRobert.docx"
"74","30 August 2022 8:58:06 am","Alexa","Halford","0000-0002-5383-4602","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-87718ddd302297554f1ec58adfc2f390_Cultivating_Inclusivity_Author_List.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Other Programmatic","","","","An Inclusive Heliophysics Community","A uniquely fundamental question will drive science innovations and discoveries in the coming decades: What research environment and community will we build? The most innovative scientific ideas and discoveries develop in safe, inclusive, diverse, accessible, and collaborative environments. If we ignore this critical aspect, current issues regarding diversity, retention, & succession will persist. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-73e287337c6c8cdcf15c912b7c323081_HalfordAlexaJ_1.pdf"
"75","30 August 2022 9:13:11 am","Alexa","Halford","0000-0002-5383-4602","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-e7c0402d599e1b92615cea539bf6097d_Pipeline_Author_List.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","The Importance of Policies: It’s not just a pipeline problem","We have identified a need to cultivate a positive, safe, inclusive, and effective environment. However, we need both cultural and programmatic changes. We will try to identify systemic issues that inhibit many from fully participating and potential solutions, as well as groups and fields producing best practices for creating and enabling effective environments where innovation can occur.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-088705c28ece24cc046614afe68a5760_HalfordAlexaJ_2.pdf"
"76","30 August 2022 9:45:20 am","Alexa","Halford","0000-0002-5383-4602","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-91435ded1df2967268040ba0ca90438a_Mentoring_Matters_Author_List.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","Mentorship within Heliophysics","In this paper, we discuss mentoring , and how it can help minority and underrepresented groups navigate the systemic issues which inhibit many from fully participating in the scientific endeavor. We are not able to cover the whole topic of mentorship, its benefits, and best practices. However, we hope that this paper will inspire agencies to implement more structured mentorship programs.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-dd5f8b7cb1f753635b8c147b3aa064f2_HalfordAlexaJ_3.pdf"
"77","30 August 2022 10:07:10 am","Alexa","Halford","0000-0002-5383-4602","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","This is a cry for help","Heliophysicists from across career levels, came together to support the position papers titled ""Cultivating a culture of inclusivity in Heliophysics,"" ""The Importance of Policies: It's not just a pipeline problem."" While writing, the number of people who privately shared terrifying stories and experiences was astounding. And if we don't do something now, our field will continue to suffer.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-cc7ffa31e28b05f66fe0d166f77d4fa0_HalfordAlexaJ_4.pdf"
"78","30 August 2022 3:51:08 pm","Jon","Vandegriff","0000-0002-0781-1565","JHU Applied Physics Lab","","","","","","","","","","","","","","","","","","","","","","","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Connecting Heliophysics Missions to Community-focused Analysis Tools","A significant fraction of the effort spent developing Heliophysics analysis tools happens in the context of mission development. Funding agencies can encourage analysis tool development to look beyond the needs of the current mission to focus on creating or bolstering community-focused tools. This paper discusses ways to promote the growing trends that support community development. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-f3fae152ffe5a9421f9ffe78c174e3b6_VandegriffJonD.pdf"
"79","30 August 2022 3:54:22 pm","Hantao","Ji","0000-0001-9600-9963","Princeton University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-42fb92d5eff274e4a0a2494e158ad595_SSPH_White_Paper_Author_Information_Form-Ji.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Laboratory space plasma physics;Fundamental space plasma theory (not specific to a particular region)","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Major Scientific Challenges and Opportunities in Understanding Magnetic Reconnection and Related Explosive Phenomena in Heliophysics and Beyond","Magnetic reconnection underlies many explosive phenomena in heliosphere and across the Universe. New capabilities in simulations, observations, and laboratory experiments provide the opportunity to solve the grand challenges summarized here. Success requires enhanced investments, increased interagency partnerships, and collaborations among heliophysics, astrophysics, and laboratory communities.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-19ca6c542b7909ac4c2d82464c4b26bb_JiHantao.pdf"
"80","30 August 2022 4:50:37 pm","Maria","Usanova","0000-0002-0406-6387","Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-99a8ee049535c464d0f0b437329624d8_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop","","","","","","Space-based","Cold ion heating in Earth’s magnetosphere","This white paper discusses the importance of improved cold ion measurements, the measurement requirements for future missions, and the role of wave-particle interactions in cold plasma heating. It highlights the need for better physics-based models in combination with machine learning to augment our understanding of coupling between different plasma populations in Earth's magnetosphere. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-45bc87267d60ea62de15b02b83bb506e_MariaUsanova.pdf"
"81","30 August 2022 6:43:53 pm","Alexa","Halford","0000-0002-5383-4602","NASA Goddard Space Flight Center","Adam","Irfan","","","","Kellerman","Azeem","","","","0000-0002-2315-936X","0000-0002-8928-9837","","","","[email protected]","[email protected]","","","","University of California, Los Angeles","NOAA/NESDIS","","","","","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Space Weather Mission Extensions: A new look at life extensions and the senior review.","We know that kp & ap are not great measures of many types of dynamics - however we default to them due to their longevity. If we want to improve our understanding, our forecasts, & our relationships with users of our research, we must continuously & reliably provide newer datasets which better describe the underlying conditions. We suggest ways to extend mission lifetime & encourage long datasets.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-d58e0d08220b9563d205db19a89a1307_HalfordAlexaJ_5.pdf"
"82","30 August 2022 10:35:28 pm","Astrid","Maute","0000-0003-3393-0987","High Altitude Observatory/NCAR","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-9bfd80787f078a6cd1d3fff1d8d19cca_Maute_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","","","","","","","","Next generation electrodynamic model for geospace","The electrodynamics are a key geospace component important for understanding variability, geomagnetic storm time response, and plasma instabilities. To make progress new electrodynamic modeling capabilities are needed: * High resolution electrodynamics * Adaptive local refinement techniques * Seamless coupling between geospace domains * Local 3D electrodynamics * Fast, efficient, stable solvers ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-a23a70338e141558f767ceecbc675480_MauteAstridI.pdf"
"83","31 August 2022 8:50:35 am","Vicki","Toy-Edens","0000-0002-6921-2525","Johns Hopkins Applied Physics Laboratory","Sandy","Jon","Wenli","","","Antunes","Vandegriff","Mo","","","","0000-0002-0781-1565","0000-0002-9179-9801","","","[email protected]","[email protected]","[email protected]","","","Johns Hopkins Applied Physics Laboratory","Johns Hopkins Applied Physics Laboratory","Johns Hopkins Applied Physics Laboratory","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","","Heliophysics Big Data: Cloud Infrastructure for Open Science","Heliophysics is in the era of big data and is at an inflection point in the need for a new computing environment. We recommend creating a network of institutions with a standard cloud framework that mimics researchers' local environments. This type of network can increase collaboration, support open science and data reproducibility, and unlock fundamentally different heliophysics research.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-db1abc80402a0989a2dc1d96332161ca_Toy-EdensVickiL.pdf"
"84","31 August 2022 11:18:24 am","Daniel","Weimer","0000-0003-1264-3612","Virginia Tech","Piyush","Rebecca","Thomas","Romina","","Mehta","Ringuette","Chen","Nikoukar","","0000-0002-5240-2322","0000-0003-0875-2023","0000-0002-0294-3614","0000-0002-8608-2822","","[email protected]","[email protected]","[email protected]","[email protected]","","West Virginia University","ADNET Systems, Inc, and NASA/GSFC/CCMC","Columbia University","Applied Physics Laboratory, Johns Hopkins University","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-1c568af122b468259f77d3b171e93511_WeimerDaniel.pdf","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations;Other Space Weather","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","","Empirical Modeling of Geospace","Empirical models have made significant contributions to both basic research and predictive applications. However, dedicated support for empirical modeling has faded over time. Additionally, the numerical techniques is losing its footing in graduate school curriculums. We recommend consideration of dedicated investment across agencies in support of research and educational efforts. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-71ccbb39dfb828b21851d64b0f717dfc_WeimerDaniel.pdf"
"85","31 August 2022 11:21:56 am","Alexander","Boyd","0000-0002-9725-508X","The Aerospace Corporation","Robert","Thomas Paul","Matthew","","","Rutledge","O'Brien","Worstell","","","","0000-0002-1606-3386","","","","[email protected]","[email protected]","[email protected]","","","The Aerospace Corporation","The Aerospace Corporation","The Aerospace Corporation","","","","Space Weather Applications","","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Space-based","Future Needs for Space Weather Forecasting","Discussion of objectives to produce accurate and actionable forecasts that provide value to end users. Here, we advocate for four focus areas: 1) shift to probabilistic forecasting, 2) Continued development of applied tools to link space environment drivers with satellite impact 3) Providing historical and contextual information, 4) Providing measurements and tools for non-GEO orbits. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-71b94742386ae0db46a9b37085d17a01_BoydAlexanderJ.docx"
"86","31 August 2022 2:13:05 pm","James","Hecht","0000-0001-6826-8810","The Aerospace Corporation","Lynette","","","","","Gelinas","","","","","0000-0001-5050-6091","","","","","[email protected]","","","","","The Aerospace Corporation","","","","","","Basic Research","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","Some Outstanding Questions on Atmospheric Gravity Wave Phenomena in the Upper Mesosphere and Lower Thermosphere","The global extent of atmospheric gravity waves is one of the great unknowns in upper atmospheric dynamics. New space-based techniques have been developed that have the potential of supplying much-needed data on their global distribution. The discussion in this paper is meant to alert the community of these techniques with the hope that one or more could be supported in future space-based missions.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-15961efacc94ab5e151025625f24c1bb_HechtJamesH.docx"
"87","31 August 2022 2:17:45 pm","Shikha","Raizada","0000-0002-9138-0584","Arecibo Observatory/UCF, Space and Atmospheric Sciences, Arecibo, Puerto Rico, USA","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-9d4c491b2d24bc4659964692cf226f3a_SSPH_Call_for_White_Papers_updated_7_22.pdf","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Characterizing the variability and structures in the coupled/complex ionosphere-atmosphere system","This paper highlights the significance of Arecibo Observatory, geomagnetically a mid- latitude while geographically a low latitude site with unique aeronomical consequences. Its unequaled location in terms of its proximity to Equatorial Ionization Anomaly (EIA), the conjugate point of South Atlantic Magnetic Anomaly (SAMA), cannot be debated and offers a bridge between equatorial and mid-latitudes.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-a97a4c6c3394f4d84af89acaf443ecf3_DecadalSurvey_v3.pdf"
"88","31 August 2022 2:30:48 pm","Manbharat","Dhadly","0000-0003-0731-788X","US Naval Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-9f4db2ea9d053ca351f01191448621ee_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop;Other Space Weather","","","","","","Ground-based;Space-based","Neutral Winds from Mesosphere to Thermosphere – Past, Present, and Future Outlook","Global geospace neutral winds have remained one of the least sampled state parameters of the Earth's upper atmosphere and are still poorly characterized even after multiple decades of observations. This white paper presents an overview of historical neutral wind measurements and the critical need for their global height-resolved measurements.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-b252bd3dc4aa7744d168b07c31312ced_DhadlyManbharatS.pdf"
"89","31 August 2022 4:50:44 pm","Drew","Turner","0000-0002-2425-7818","Johns Hopkins Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-6184476620a0fa41c6a49cb1e0ccfc2d_SSPH_White_Paper_Author_Information_Form_TurnerDrewL_SWx.xlsx","Space Weather Applications","","","","Other Space Weather","","","","","","","Data-Informed Prediction of State is the Key to Space Weather: The Significance and Value of Forecasts, Nowcasts, Hindcasts, and Climatology","Currently, much attention is dedicated to SWx forecasting, but here, we argue that nowcasting, hindcasting, and climatological modeling are all of equally significant importance as forecasting. All combined, the true priority of improved SWx risk mitigation is prediction of the relevant state conditions at any point in time: past, present, future, and probabilistic.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-8086b75d89244df029d3f41c61dc07c2_TurnerDrewL1.pdf"
"90","31 August 2022 4:53:46 pm","Drew","Turner","0000-0002-2425-7818","Johns Hopkins Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-8d21036773bcadfcb0b237519b46f82e_SSPH_White_Paper_Author_Information_Form_TurnerDrewL_EPP.xlsx","Basic Research","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","","Atmospheric and ionospheric impacts of energetic particle precipitation (EPP) from Earth’s ring current and radiation belts","Explore and establish the consequences of and causal role between energetic particle precipitation (i.e., ring current, radiation belt, and solar energetic particles) and: i) transient events of mesospheric NOx and HOx production, ozone depletion, and stratospheric and tropospheric warming and ii) localized, transient structures and sporadic intensification of the D- and E-region ionospheres.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-d87e125f78d02085a08dad4c715ac6ee_TurnerDrewL2.pdf"
"91","31 August 2022 4:57:14 pm","Drew","Turner","0000-0002-2425-7818","Johns Hopkins Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-02fa2996240cb3c2ef33fa2988c63354_SSPH_White_Paper_Author_Information_Form_TurnerDrewL_Shx.xlsx","Basic Research","Fundamental space plasma theory (not specific to a particular region);Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","","Cross-scale physics and the acceleration of particles in collisionless plasmas throughout the Heliosphere and beyond: I. Collisionless shocks","Shocks in astrophysical plasmas are a fundamental, ubiquitous process considered responsible for accelerating many of the most energetic particles that we observe in the Universe, including galactic and anomalous cosmic rays (GCRs and ACRs) and solar energetic particles (SEPs). We present suggestions for focused, dedicated research of particle acceleration at shocks in the next decade.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-bd987b21d725d22090c04359a94ad4b7_TurnerDrewL3.pdf"
"92","31 August 2022 4:59:56 pm","Drew","Turner","0000-0002-2425-7818","Johns Hopkins Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-e3e9295f4460a2cb675273fcb4fa5af0_SSPH_White_Paper_Author_Information_Form_TurnerDrewL_Rx.xlsx","Basic Research","Fundamental space plasma theory (not specific to a particular region);Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","","Cross-scale physics and the acceleration of particles in collisionless plasmas throughout the Heliosphere and beyond: II. Magnetic reconnection","Earth's magnetotail is an ideal natural laboratory to study particle acceleration associated with magnetic reconnection; dedicate research there. Heliophysics should also consider studying reconnection-related acceleration in other space plasma environments including: solar and solar wind; Jupiter's magnetosphere; Uranus' magnetosphere; the heliosheath, heliopause, and local interstellar medium.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-f3e9472dc5b253e8287fa694cc0d8bcc_TurnerDrewL4.pdf"
"93","31 August 2022 5:01:42 pm","Drew","Turner","0000-0002-2425-7818","Johns Hopkins Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-b40e6c47083696e70f86a1853cc49fe9_SSPH_White_Paper_Author_Information_Form_TurnerDrewL_RBs.xlsx","Basic Research","Fundamental space plasma theory (not specific to a particular region);Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","","Cross-scale physics and the acceleration of particles in collisionless plasmas throughout the Heliosphere and beyond: III. Radiation belts","Radiation belt systems are found at all the sufficiently magnetized and sized planets in our Solar System, implying that particle trapping and acceleration in magnetospheric systems is a universal process. We should be conducting more advanced comparative systems science at these accessible radiation belt systems to understand the distinctive and universal processes at each. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-9a02fcc4aa64c9f01b2c376745cb7825_TurnerDrewL5.pdf"
"94","31 August 2022 11:45:55 pm","Colby","Haggerty","0000-0002-2160-7288","Institute for Astronomy, University of Hawaii, Manoa","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-37e61f36d75d7f0a9a50f80729cc6821_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","","The Physics of Collisionless Dissipation in the Heliosphere","The physics of collisionless dissipation is an essential part of heliospheric plasma systems and advancements in this topic in the next decade are needed to develop a comprehensive understanding of the heliosphere. We report recent advances in the study of collisionless dissipation, identify key outstanding problems, and encourage support for research in theory, modeling and observations.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-9554eba07be291ad0a9be834d5064522_HaggertyColbyC.pdf"
"95","1 September 2022 10:05:23 am","Haosheng","Lin","0000-0002-4504-3165","University of Hawaii","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research","Solar Physics","","","","","","","","","","Development of Integral Field Spectrographs to Revolutionize Spectroscopic Observations of Solar Flares and other Energetic Solar Eruptions","Resolving the physics behind solar flares and CMEs requires continuous 2D spectra throughout these events. Advanced Integral Field Spectrographs now provide previously unachievable multiplexing, making this challenging goal nearly attainable. Immediate technology investment will deliver IFSs enabling space instruments that revolutionize our ability to study the active sun in the coming decade.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-d8e8f47f82d3569563a5c22b6ee31176_Helio_Decadal_IFU_White_Paper_vf_9-1-22.pdf"
"96","1 September 2022 10:20:40 am","Jason","TenBarge","0000-0003-0143-951X","Princeton University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-5ff77ee3a50edf9720467310108ce143_TenBarge_Turbulence_White_Paper_Author_Information_Form.xlsx","Basic Research","Laboratory space plasma physics;Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","","Disentangling the Spatiotemporal Structure of Turbulence Using Multi-Spacecraft Data","This white paper prepared for the 2024 Decadal Survey for Solar and Space Physics concerns the importance of research related to multi-spacecraft missions to address fundamental questions concerning plasma turbulence. In this white paper, some of the important questions facing the turbulence community that can only be addressed by funding research related to multipoint measurements are presented.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-7cb8a2bb40dfc5c1502315df51ce883c_TenBargeJasonM.pdf"
"97","1 September 2022 12:45:45 pm","Noé","Lugaz","0000-0002-1890-6156","University of New Hampshire","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-3ea2babfc7f2113794a07b9f4811e92a_SSPH__CME_author_list.xlsx","Basic Research","Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","","","","","he Importance of Fundamental Research on the Upper Coronal and Heliospheric Evolution of Coronal Mass Ejections","Coronal mass ejections are a cornerstone of heliophysics. It is essential to address the evolution of CMEs in the upper corona and inner heliosphere, independent of their space weather impact through a comprehensive research program. Such a program should include components of data analysis, theory, model and simulation development and lead to new missions and instrumentation. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-6ee69a2172d389864a71ae7a7912faad_LugazNoe1.pdf"
"98","1 September 2022 2:39:16 pm","Katherine","Goodrich","","West Virginia University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-09c4e36e1cdaf7669fecce6164530280_GoodrichKatherineA2.xlsx","Basic Research","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","Space-based","Multi-point Assessment of the Kinematics of Shocks (MAKOS): A Heliophysics Mission Concept Study","Collisionless shocks are fundamental processes that are ubiquitous in space plasma physics throughout the Heliosphere and most astrophysical environments. This white paper describes a conceptual mission design to address these outstanding questions and advance our knowledge of the nature of collisionless shocks.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-b60926d544ebb584de92988ebc8719f5_GoodrichKatherineA2.pdf"
"99","1 September 2022 4:46:44 pm","George","Carson","0000-0002-3485-8924","Dickinson College","Jason","Joseph","Blerta","David","Brian","Kooi","Helmboldt","Markowski","Bonanno","Hicks","0000-0002-5595-2522","0000-0002-2123-0441","","","","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","U.S. Naval Research Laboratory","U.S. Naval Research Laboratory","U.S. Naval Research Laboratory","U.S. Naval Research Laboratory","U.S. Naval Research Laboratory","","Basic Research","Solar Physics;Other topic relevant to solar and space physics/heliophysics","","","","","","","","","","DLITE - an Inexpensive, Deployable Interferometer for Solar Radio Burst Observations","Solar radio bursts can provide unique insights into the coronal plasma structure where emission occurs. The Deployable Low-band Ionosphere and Transient Experiment (DLITE) array was designed to probe the Earth's ionosphere; however, DLITE can also provide detailed observations of SRBs at 30-40 MHz with a 1.024-second temporal resolution and 16.276-kHz frequency resolution.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-67de218c12bcaa100fd66f50cf92f531_CarsonGeorge.pdf"
"100","1 September 2022 6:49:59 pm","Jason","Kooi","0000-0002-5595-2522","U.S. Naval Research Laboratory","David","Elizabeth","Brian","","","Wexler","Jensen","Wood","","","0000-0002-5763-6267","0000-0003-0216-6621","0000-0002-4998-0893","","","[email protected]","[email protected]","[email protected]","","","University of Massachusetts Lowell","Planetary Science Institute","U.S. Naval Research Laboratory","","","","Basic Research;Space Weather Applications","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","Other Space Weather","","","","","","Space-based","Multipoint Radio Probe of the Solar Corona: the Trans-Coronal Radio Array Fleet (T-CRAF)","The Trans-Coronal Radio Array Fleet (T-CRAF) is a mission concept designed to continuously probe the magnetic field and plasma density structure of the corona at heliocentric distances of 2-10 solar radii. T-CRAF consists of thirty small satellites orbiting the Sun-Earth Lagrange Point L3 in order to provide thirty lines of sight for ground- or space-based radio propagation studies.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-aaf3c9e2dd9b904167d73adeede3d21c_KooiJason1.pdf"
"101","1 September 2022 8:18:06 pm","Linsky","Jeffrey","0000-0003-4446-3181","University of Colorado","Redfield","Moebius","","","","Seth","Eberhard","","","","0000-0003-3786-3486","0000-0002-2745-6978","","","","[email protected]","[email protected]","","","","Wesleyan University","University of New Hampshire","","","","","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","What Lies Outside of the Heliopause: Connecting the Outer Heliosphere with the Very Local Interstellar Medium","The size, shape, and plasma properties of the outer heliosphere depend critically on the neutral density, and magnetic field of the surrounding Very Local Interstellar Medium. Major questions concern the interactions of the heliosphere with its environment, and how astrospheres should differ from the today's heliosphere as a result of different properties in their interstellar environments.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-fb5d5f5d09317df1bdd75f057986fa71_Heliodecadal.pdf"
"102","2 September 2022 10:12:24 am","James","Mason","0000-0002-3783-5509","Johns Hopkins University Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-82ce3269dc6258ee6797aa4ac7ce1cfc_SSPH_White_Paper_Author_Information_Form_SmallSats.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","","Small Platforms, High Return: The Need to Enhance Investment in Small Satellites for Focused Science, Career Development, and Improved Equity","Small satellites presently fill an appropriate niche in the cost versus mission-class ecosystem; are highly productive as measured by papers/year/$M; present the rare opportunity to develop a career in spaceflight leadership. Equity goals can be met sooner by increasing the number of opportunities to lead smallsats. But current funding levels are a bottleneck that prioritized budgets could amend","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-47bc579270d09d136a3c2382d21732fa_MasonJamesP1.pdf"
"103","2 September 2022 10:18:16 am","James","Mason","0000-0002-3783-5509","Johns Hopkins University Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-b549f7f578029289c47bba08bd60cbe2_SSPH_White_Paper_Author_Information_Form_Deep_Learning.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Leveraging Artificial Intelligence to Enhance the Science Return of 4π Solar Constellations","Constellations have an inherent tension between the scientific benefit of including more satellites and the additional cost that imposes. There are many calls to recommend constellations, particularly to obtain 4π observations of the Sun. AI methods can enhance the science return and forecasting capabilities of these constellations, e.g., via virtualized observatories. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-9b416378fec8d50dcc6ec625bbabc581_MasonJamesP2.pdf"
"104","2 September 2022 10:23:25 am","James","Mason","0000-0002-3783-5509","Johns Hopkins University Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-6205ddd54f116a386a18f8b1dd2c3626_SSPH_White_Paper_Author_Information_Form_Middle_Corona_CMEs.xlsx","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Other Space Weather","","","","","","","Uninterrupted Tracking of Coronal Mass Ejections","CMEs have been well observed in the low/high corona + interplanetary space; but they mostly accelerate in the middle corona (1.5-6 Rs). We have numerous models to explain how they are triggered and accelerated, but insufficient observational constraints. New tech is now available to remedy that. We should prioritize acquisition of these observations from multiple lines-of-sight.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-15817619c341e6af88ffbd0f2b11ae1c_MasonJamesP3.pdf"
"105","2 September 2022 10:44:35 am","Ian","Cohen","0000-0002-9163-6009","JHU/APL","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-27ecee4fec53bc3742825a1e79bbb2f9_CohenIanJ1.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Toward a more comprehensive understanding of the underexplored region of Earth’s atmosphere from ~80 to ~160 km altitude","Looking toward the future, it is important to consider technological and programmatic solutions that will enable exploration of the woefully underexplored region of Earth's atmosphere from ~80 to ~160 km altitude. A range of potential solutions are possible from orbital to suborbital missions, but require technological development and programmatic changes.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-fcee7e6e12480c018de60ba6e1a2c3c0_CohenIanJ1.pdf"
"106","2 September 2022 10:48:09 am","Ian","Cohen","0000-0002-9163-6009","JHU/APL","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-c00c11cd078e0baab7155e48072d3818_CohenIanJ2.xlsx","Basic Research","Planetary Magnetospheres;Planetary ionospheres/upper atmospheres","","","","","","","","","","The case for studying other planetary magnetospheres and atmospheres in Heliophysics","Studying planetary systems with Heliophysics objectives, comprehensive instrumentation, and new opportunities for analysis and modeling would enable a novel understanding of fundamental and universal processes of space plasma physics. As such, the community should be prepared to consider, prioritize, and fund dedicated efforts to planetary targets to study space physics and aeronomy objectives.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-3325126a6b3d91c7fdee214afccb34da_CohenIanJ2.pdf"
"107","2 September 2022 11:01:50 am","Andrew","Stephan","0000-0002-9487-6235","U.S. Naval Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-08d00fb3b4c48ef99412542ac80946af_StephanAndrew_SSPH_White_Paper_Author_Information_Form.xlsx","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","A Constellation of Compact EUV/FUV Spectroscopic Imagers for Global Ionosphere-Thermosphere Specification","Accurate space weather forecasts must include measurements of the temporal and spatial evolution of the ionosphere and thermosphere system. A constellation of UV airglow profilers can create continuous, routine, 3D space weather maps to inform scientific and operational interests. New investment to develop these compact remote sensors will lead to a next-generation space weather mapping network. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-bffb26888b52f30dfc0ecc268061cb6c_StephanAndrewW.pdf"
"108","2 September 2022 1:13:47 pm","Kristina","Lynch","https://orcid.org/0000-0001-9006-1138","Dartmouth College","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Ionosphere-thermosphere system science and the use of distributed heterogeneous data arrays: vector fields, volumetric densities, auroral imagery","This Helio2050 white paper encapsulates the system science justifications of the recent Midex CSR for the ARCS mission, a localized swarm of 32 cubesats over a dedicated groundbased imagery array of 32 Alaskan camera sites, with localized tomography between the two. This heterogeneous, multiplatform, distributed measurement system constrains physics-based modelling of auroral plasma physics.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-633a542ce596c121ea7c922e29febd6d_LynchKristinaA2.pdf"
"109","2 September 2022 3:11:09 pm","Shun-Rong","Zhang","https://orcid.org/0000-0002-1946-3166","MIT Haystack Observatory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-54120a76f01d1ab229ceaae76e47674d_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Inner Heliosphere and solar wind interaction with unmagnetized bodies;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Ground-based","Long-term space climate monitoring","It is important to maintain efficient long-term investments to monitor space climate. Proper observational configuration and networks to measure key physical parameters is a practical approach. It is necessary to balance the needs for building cutting edging new instruments and ensuring the longevity of existing key facilities. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-57646ed182033e180cbfdb526b968eeb_Decadal_Survey__long_term_trends.pdf"
"110","2 September 2022 1:40:32 pm","Mark","Moldwin","0000-0003-0954-1770","University of Michigan","Nicholas","Christina","","","","Gross","Cohen","","","","0000-0002-4826-6575","0000-0002-0978-8127","","","","[email protected]","[email protected]","","","","Boston University","California Institute of Technology","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","Role and Opportunity of Solar and Space Physics Summer Schools to Change Culture","Summer schools to support the academic and professional development of students and early career (SEC) scientists. We call for a more intentional effort to share best practices, scaffold curriculum, rigorously assess impact, to integrate inclusive and active teaching techniques into their programs, focus on developing ethical, open science-supporting, and DEIA-competent SEC.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-3c9c01e5621ce9e1ef33bd73fbeb576a_MoldwinMarkB.pdf"
"111","2 September 2022 1:44:19 pm","Christine","Gabrielse","0000-0001-6905-2288","The Aerospace Corporation","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-7c2931c19511a875ec5ab02bb1a46f53_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","","Mesoscale Phenomena & their Contribution to the Global Response: A Focus on the Magnetotail Transition Region & Magnetosphere-Ionosphere Coupling","An important question that is being increasingly studied across subdisciplines of Heliophysics is ""how do mesoscale phenomena contribute to the global response of the system?"" This white paper focuses on this question within two specific but interlinked regions in Near-Earth space: the magnetotail's transition region to the inner magnetosphere and the ionosphere.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-37d147c05887f2e8f82d2c11af0ee33d_GabrielseChristine.pdf"
"112","2 September 2022 2:39:07 pm","Yuan-Kuen","Ko","0000-0002-8747-4772","U.S. Naval Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-a15ff6c2fa6e28190a49ef94512156e5_SSPH_White_Paper_Author_Information_Form_YKKo.xlsx","Basic Research","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","","","","","Spectroscopy in the Middle Corona: Probing the Kinetic Processes in the Nascent Solar Wind and Solar Energetic Particle Production","Spectroscopic observations in the Middle Corona enable us to probe into the underlying kinetic processes at work and provide powerful diagnostic capabilities for understanding how the solar wind is heated and accelerated, how a CME interacts with the corona to obtain its characters, and how and when a CME develops a shock that accelerates the ambient solar wind to SEPs.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-2991d617950a43438ac37ffbf738fc3a_KoYuan-Kuen.pdf"
"113","2 September 2022 2:50:07 pm","Marc","Kornbleuth","0000-0002-3479-1766","Boston University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-ae309690acfbca304de0a91221f0b200_Solar_Magnetic_Field_CoAuthors.xlsx","Basic Research","Outer Heliosphere","","","","","","","","","Space-based","The Importance of Understanding the Solar Magnetic Field in the Heliosphere using the Interstellar Probe","The heliospheric community needs an interstellar probe. An interstellar probe with a proper onboard magnetometer would provide observational data to answer many questions about the magnetic field in the heliosphere, including the effect of magnetic reconnection on ion acceleration in the heliosheath and the draping of the interstellar magnetic field around the heliopause.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-770eab5d468334c2729edb6611155727_Kornbleuth_WhitePaper_SolarMagneticField_Final.pdf"
"114","2 September 2022 3:06:34 pm","Rafael Luiz","Araujo de Mesquita","0000-0003-4681-8679","The Johns Hopkins Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-0cd73685660f342b14d6d9585e57b136_SSPHWhitePaperAuthorInformationForm_RM_GroundBased.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","Ground-based","On the exploration of mesospheric and thermospheric dynamics through a large ground-based instrument network","The fundamental physical drivers and coupling processes underlying mid-to-large scale phenomena in the mesosphere and thermosphere are poorly understood due to a lack of cross-hemispheric, coordinated observations. The solution is a large network of ground-based instruments funded on a facility level to observe these phenomena and make substantive progress in the science of these phenomena.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-4b735653b83c45821fd0b0134fd554a3_DecadalWhitePaper_GroundBasedNetwork_FINAL.pdf"
"115","2 September 2022 3:20:39 pm","Benjamin","Boe","0000-0002-6396-8209","Institute for Astronomy, University of Hawaii","Shadia","Adalbert","","","","Habbal","Ding","","","","0000-0003-4089-9316","0000-0001-6573-7810","","","","[email protected]","[email protected]","","","","Institute for Astronomy, University of Hawaii","Institute of Optics and Atomic Physics, Technische Universitaet Berlin and Institut fur Technische Physik","","","","","Basic Research;Infrastructure, Workforce, Other Programmatic","Solar Physics","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","The Need for a New Generation of Space-based Visible and Near-IR Emission Line Observations of the Corona","Visible and near-infrared (V+NIR) coronal emission lines have proven diagnostic potential for probing the physics of the middle corona from 1.5 to 6 Rs. Current ground- and space-based coronagraphs are not able to explore this region. There is a dire need for new space-based assets to measure a wide range of V+NIR emission lines beyond 1.5 Rs with both spectrometers and narrowband imagers.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-91b130c8b907d8ab8bad691ace3857a3_BoeBenjaminR.pdf"
"116","2 September 2022 3:20:57 pm","Shun-Rong","Zhang","0000-0002-1946-3166","MIT Haystack Observatory","Astrid","Ruth","Claudia","","","Maute","Lieberman","Stolle","","","","","","","","","","","","","NCAR High Altitude Observatory","NASA Goddard Space Flight Center","Leibniz Institute of Atmospheric Physics","","","","Basic Research","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Other topic relevant to solar and space physics/heliophysics","","","","","","","","","Ground-based;Space-based","Neutral wind dynamo and ionospheric electrodynamics at low and mid- latitudes","The wind dynamo is the essential cause of ionospheric electrodynamics, driving ionospheric variability on various spatial-temporal scales at low- and mid-latitudes. In order to advance the heliosphere science in the new decade for characterizing and forecasting ionospheric variability, substantial observational and modeling efforts are needed with a focus on the wind dynamo and its drivers.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-898b6e920e2c4fb318756e99d10f92e8_Decadal_Survey__wind_dynamo.pdf"
"117","2 September 2022 3:31:08 pm","Ayris","Narock","0000-0001-6746-7455","NASA/GSFC; ADNET Systems Inc.","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-c464667976f6ba6fb0409cf0f76cd530_NarockAyrisA_SSPH_White_Paper_Author_Information_Form.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Responsible Machine Learning in Heliophysics","Machine learning has become embedded in the field of Heliophysics. Ethical and responsible use of these methods encompasses many aspects that create necessary additional burden to the individual researcher and the research community as a whole. Sustained financial and infrastructural support from affiliated agencies and institutions is needed in addition to community-based governance strategies. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-54a052e28c1e3bf27580e1d768044670_NarockAyrisA.pdf"
"118","2 September 2022 4:47:59 pm","Ian","Cohen","0000-0002-9163-6009","JHU/APL","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-47b34faab9cad83e0d3e087b68f698ef_CohenIanJ3.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Other Programmatic","","","","Reimagining Heliophysics: A bold new vision for the next decade and beyond","Heliophysics has a branding problem. We need an answer to the question: ""What is Heliophysics?"" The answer should clearly and succinctly define our science in a compelling way that simultaneously introduces a sense of wonder and exploration into our science and our missions. Moving forward, our community needs to be bold and unabashed in our definition of Heliophysics and its big questions.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-15ae97d7b3d301b7bfbb20b84331470f_CohenIanJ3.pdf"
"119","2 September 2022 5:47:37 pm","Samuel","Schonfeld","0000-0002-5476-2794","Institute for Scientific Research, Boston College","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-190b9fddda303fbd553defa34d15ad0b_SSPHWhitePaperAuthorInformationForm.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Expanding the Deep Space Network to support the Heliophysics System Observatory","As heliophysics satellites move beyond low Earth orbit, heliophysics research and space weather forecasting increasingly depend on the Deep Space Network (DSN). Already the primary constraints in mission scope and design are data downlink limitations, not instrument capabilities. Enabling future heliophysics discoveries requires expansion of the DSN and investment in communication technologies.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-fb7d0856327977f60467437497993b47_SchonfeldSamuelJ.pdf"
"120","2 September 2022 8:06:00 pm","Astrid","Maute","0000-0003-3393-0987","High Altitude Observatory/NCAR","Alexa","","","","","Halford","","","","","","","","","","[email protected]","","","","","NASA/Goddard Space Flight Center","","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","","Slowly Heating the Pot - Time to Measure the Temperature","We need a strong, healthy, diverse workforce but hear that scientists are stressed and overwhelmed. We suggest to evaluate the situation. 1. A new phenomena or a continuation of old practices? 2. Evaluate change of work-place, -load, and -culture. 3. Examine funding characteristics over time and survey the workforce of our community. 4. Data needs to be anonymized and made public.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-6853e10889ac761a5cad61d73040c602_MauteAstridI2.pdf"
"121","2 September 2022 10:04:20 pm","Sona","Hosseini","0000-0002-9504-6989","JPL-Caltech","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-f3bc9fae6bb75461cd58aad05089ad7a_HosseiniSona_WP_Author_Information.xlsx","Basic Research","Solar Physics;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","Spatial Heterodyne Spectroscopy: A Powerful Technique for Remotely Measuring the State of Plasmas from the Solar Atmosphere to Geospace to Heliopause","Spatial Heterodyne Spectroscopy (SHS) is a revolutionary new technique for Heliophysics capable of obtaining spectral line profiles at ultrahigh spectral resolution from a compact, robust, cost-effective instrument with no moving parts suitable for spaceflight. This white paper recommends maturing and developing SHS-based instruments to study key Solar and Heliophysics objectives from space. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-404bdd03bbd67f5a9d3905a321f63042_HosseiniSona.pdf"
"122","3 September 2022 9:35:49 am","Joseph","Lazio","","Jet Propulsion Laboratory, California Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-735fdb23fc382488957fb88850487507_SSPH_White_Paper_Author_Information_Form.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","Ground-based","The Deep Space Network: Enabling Richer Data Sets for Future Solar & Space Physics Missions","From the first interplanetary spacecraft to current Heliophysics missions, the Deep Space Network has been integral to NASA Science. Several improvements have been implemented and are planned for the DSN. These improvements would enable the science described in community workshops and submitted white papers. However, without continued support, some of these planned improvements are at risk.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-5370c81c591b453074792e619691a6e8_LazioJoseph.pdf"
"123","3 September 2022 10:06:09 am","Angelos","Vourlidas","0000-0002-8164-5948","JHUAPL","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-09ea2f9644cc83d9ac11882a30f8e955_VourlidasAngelos2_WP_Author_Information.xlsx","Basic Research","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","","","","","The Critical Coronal Transition Region: A Physics-framed Strategy to Uncover the Genesis of the Solar Wind and Solar Eruptions","The corona within 10 Rs is the host of physical processes critical for understanding solar activity. We argue that the exploration of this Coronal Transition Region will answer two of the most central Heliophysics questions, 'How and where does the solar wind and CMEs form?' by unifying hardware/software/modeling development and seemingly disparate research communities and frameworks.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-bc5ead4f7d01f9a451162208dff8a840_VourlidasAngelos2.pdf"
"124","3 September 2022 10:24:00 am","merav","opher","0000-0002-8767-8273","Boston University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-126a1f63492c8cfef1a281f900f89569_Opher_WP.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","","Our Heliospheric Shield, a Case of a Habitable Astrosphere: Need to Revisit this region with In-Situ Measurements with Modern Instrumentation","This white paper describes some of the current science questions and advocates the need to send in the next decade a probe, such as Interstellar Probe, to take in-situ measurements with modern instrumentation within the next decade. It also discusses recent works relate the location of the Sun within the interstellar medium to terrestrial effects. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-0dac235446366b890a3645ee021f4ea8_Solar_Space_Physics_Decadal_HabitableAstrsophere_Sep03.pdf"
"125","3 September 2022 10:50:23 am","Yeimy","Rivera","0000-0002-8748-2123","Center for Astrophysics | Harvard & Smithsonian","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-cf92e8b2e42e19fc13f8f7e3930a728f_SSPHWhitePaper_atomicphysics.xlsx","Basic Research","Laboratory space plasma physics;Other topic relevant to solar and space physics/heliophysics","","","","","","","","","","Advancing Solar and Heliospheric Science through the Ongoing Development and Support of Atomic and Laboratory Plasma Physics","This white paper outlines the necessity for the availability, accessibility, and expansion of atomic physics data and analysis tools for the meaningful interpretation of spectroscopic and polarimetric observations through the ongoing development and support of atomic and laboratory plasma physics.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-9806c518cc29f3eb9f06ddd416c95380_RiveraYeimyJ1.pdf"
"126","3 September 2022 4:01:03 pm","Roberto","Guenzani","","NgEHT-TH","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research","Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","Remote Sensing of Heterocyclic Life in Solar System and in Generalized Clusters Unfolding","A ray of State of Existence gives a Tree of limit Experience that can be traced from literal calculus and, in S-Language, propagates heterocycles in not equivalent syntactic Replica beyond Page Curve Tautology. Stratifying semantic stability in Space I prospect Irrational Unbalance as S-Flare Precession and a Tree of Unfolding of granular Life as Astrobiology solution of Hawking Paradox. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-f28ce0ed41d773977dbadd64825c4721_GuenzaniRoberto2.pdf"
"127","3 September 2022 6:44:08 pm","Angelos","Vourlidas","0000-0002-8164-5948","JHUAPL","Jesper","","","","","W. Gjerloev","","","","","0000-0002-7277-9004","","","","","[email protected]","","","","","JHUAPL","","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Other Programmatic","","","","A Fresh Approach to PI-led Mission & Hardware Solicitation Model","We argue that the current solicitation model for PI-led missions and hardware investigations leads to an unnecessary waste of precious resources, and it largely limits these opportunities to a large institutions and thereby is inherently elitist and non-inclusive. We propose a simple solution that overcomes these problems. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-ba099fb1ce239ced9bc74af2ee92bc3b_VourlidasAngelos4.pdf"
"128","3 September 2022 6:50:21 pm","William H.","Matthaeus","0000-0001-7224-6024","University of Delaware","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-e4cd4cc7576758bef559680655532d10_Matthaeus-Multispacecraft-SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","Solar Physics;Fundamental space plasma theory (not specific to a particular region)","","","Space Weather Research to Operations to Research Loop","","","","","","Space-based","The essential role of multi-point measurements in investigations of heliospheric turbulence, three-dimensional structure, and dynamics","Space plasmas are three-dimensional and dynamic; single-spacecraft measurements cannot unravel their complete space-time structure. Only multispacecraft missions can dramatically advance knowledge in Space Weather, heliospheric dynamics and plasma turbulence theory. We describe the theoretical requirements and several types of heliospheric missions for resolving space plasma space-time structure.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-1b6277b652f77d2812c77d9c8a077c23_MatthaeusWilliamH.pdf"
"129","3 September 2022 8:00:26 pm","Periasamy K","MANOHARAN","0000-0003-4274-211X","Arecibo Observatory, University of Central Florida, Arecibo, Puerto Rico 00612, USA","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research;Space Weather Applications","Solar Physics;Other topic relevant to solar and space physics/heliophysics","","","Space Weather Research to Operations to Research Loop;Other Space Weather","","","","","","Ground-based","Regular Solar Radio Imaging at Arecibo: Space Weather Perspective of Evolution of Active Regions","Mapping of the Sun at X-band (8.1 -- 9.3 GHz) with the 12-m radio telescope at the Arecibo Observatory allows monitoring of the evolution of the brightness temperature of active regions in association with the development of magnetic complexity, which can lead to strong eruptions. Such observations have tremendous potential to understand the magnetic activity of solar eruptions in advance.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-92031cc9698ff7bc07d005c3f405add2_pkm_AO_white_paper_final_03sep2022.pdf"
"130","4 September 2022 4:49:09 pm","Shadia","Habbal","0000-0003-4089-9316","Institute for Astronomy, University of Hawaii","Benjamin","Colby","Adalbert","","","Boe","Haggerty","Ding","","","","","","","","[email protected]","[email protected]","[email protected]","","","IfA, U. Hawaii","IfA, U. Hawaii","ITP, Germany","","","","Basic Research","Solar Physics","","","","","","","","","Ground-based","A Total Solar Eclipse Earth-Based Mission: Multi-wavelength Observations from Land, Sea and Air to Probe the Critical middle Corona","Total solar eclipses continue to yield key plasma parameters of the inner and middle corona, by capitalizing on the V+NIR coronal emission lines. This critical coronal space remains inaccessible to existing and to-be launched coronagraphic instrumentation in the next decade. This white paper calls for the urgent need to continue to fund TSE observations over the next solar cycle.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-3df32575328ac0e3c4170dedacafdb98_HabbalShadiaR.pdf"
"131","4 September 2022 5:00:52 pm","Kristopher","Klein","0000-0001-6038-1923","University of Arizona","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-52460e611b3f75a58455bdf26a20bf8d_HelioSwarm_White_Paper_Author_Information_Form.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Fundamental space plasma theory (not specific to a particular region)","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence","HelioSwarm (HS), a NASA MidEx multispacecraft observatory with inter-spacecraft separations covering MHD and ion scales, will measurement the structure and dynamics of magnetized turbulence. This paper surveys turbulent systems that constitute compelling areas of heliophysics research and describes how HS will measure energy transport across scales in turbulent plasmas throughout the universe.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-74759a9ef03ff1818ae0ddefd1c05ea9_KleinKristopherG.pdf"
"132","5 September 2022 2:09:11 am","Louise","Harra","0000-0001-9457-6200","PMOD/WRC & ETH-Zürich","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-5c1de373135f232c122cbbbe0a56f78d_SSPHWhitePaperAuthorInformationForm_harralouisek.xlsx","Basic Research;Space Weather Applications","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","Other Space Weather","","","","","","Space-based","Firefly: the science case for a full view of the solar sphere","This white paper indicates the support of the European and Japanese communities for the Firefly mission concept (see white paper led by Nour Raouafi). An ambitious mission such as Firefly provides extensive opportunities to answer scientific questions that remain unanswered due to our restricted views of the Sun. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-12ab3014df34471bc89b2c24c630e86d_HarraLouiseK.pdf"
"133","5 September 2022 2:13:20 am","Konstantinos","Dialynas","0000-0002-5231-7929","Office of Space Resesearch and Technology, Academy of Athens, 4 Soranou Efesiou Street, GR-11527, Athens, Greece","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-95fecc4ed4bc42b937511bcf86bb120d_DialynasKostas_White_Paper_Author_Information_Form.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","Space-based","A future Interstellar Probe on the dynamic heliosphere and its interaction with the very local interstellar medium","Following the Interstellar Probe study report, this paper aims to highlight the importance of studying the physics of the interactions pertaining to the expanding solar wind that meets the plasma, gas and dust flows of the VLISM that form the heliosphere. We focus on three fundamental open science questions that can be addressed by a combination of in-situ observations with remotely sensed ENAs.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-57efe8c4e6902b070026c772fbc26d42_DialynasKostas.pdf"
"134","5 September 2022 11:29:24 am","Theodore","Sarris","0000-0002-0336-2678","Democritus University of Thrace","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-2a26abf959386c7a0bf9a4867c26741d_SSPH_White_Paper_Author_Information_Form_2.xlsx","Basic Research","Planetary ionospheres/upper atmospheres","","","","","","","","","Space-based","Plasma-Neutral Interactions in the Lower Thermosphere-Ionosphere: The need for in situ measurements to address focused questions","There is a need to advance our understanding of the Lower Thermosphere-Ionosphere and of the neutral-plasma interactions that shape it. A mission that provides comprehensive in situ measurements down to altitudes where ion-neutral interactions maximize (120 km or lower) is feasible and mature, and will explore, for the first time, the dominant processes in the atmosphere-space transition region.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-08e8956a43fe11bce9ff5073e66e849f_TheodoreSarrisE.pdf"
"135","5 September 2022 11:40:52 am","Guiping","Liu","","University of California Berkeley","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-fe1aba9b3d1f835691245f91ba775d9e_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Planetary ionospheres/upper atmospheres","","","","","","","","","","New observational capabilities for the thermosphere and ionosphere towards understanding the impacts of the lower atmosphere wave forcing","Supporting the overall concepts of the GDC and DYNAMIC missions, and continuing or enhancing capabilities like ICON, TIMED, Aura MLS, and GOLD will be of high value in moving towards the ultimate goal of a full understanding of the roles of tides and planetary waves in driving IT variability.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-1424fe84f0e99941f36e2c933c891cd4_LiuGuiping1.docx"
"136","5 September 2022 11:49:39 am","Guiping","Liu","","University of California Berkeley","Guan","","","","","Le","","","","","0000-0002-9504-5214","","","","","[email protected]","","","","","NASA Goddard Space Flight Center","","","","","","Basic Research","Planetary ionospheres/upper atmospheres","","","","","","","","","","Enhance ionospheric electric field and current observations to better understand the E-region electrodynamics","Utilizing multi-point and multi-platform observations such as those from the planned GDC and DYNAMIC missions and the ground-based magnetometer network that include the electric current variations will advance our understanding of the ionospheric E-region electrodynamics. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-c33196ad7f2d41425b20ec449f5a5277_LiuGuiping2.docx"
"137","5 September 2022 12:12:57 pm","Benoit","Lavraud","0000-0001-6807-8494","Laboratoire d'astrophysique de Bordeaux, Univ. Bordeaux, CNRS, Pessac, France","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-51d02dd65df3e5ce149f79d60b51a197_LavraudBenoit.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","","What is the Heliopause? Importance of magnetic reconnection and measurement requirements","We highlight the importance of magnetic reconnection at the Heliopause (HP), both as a key processe driving the interaction between solar and interstellar media, but also as an element of the definition of the HP itself. We explain that discriminating between current interpretations of plasma and magnetic field data near the HP necessitates appropriate measurements which are lacking on V1 and V2.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-a7b69731973181d9a9bb950e2208cf06_LavraudBenoit.pdf"
"138","5 September 2022 2:03:07 pm","Joseph E","Borovsky","0000-0002-2325-3348","Space Science Institute","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research","Planetary Magnetospheres;Planetary ionospheres/upper atmospheres","","","","","","","","","Ground-based;Space-based","The Missing Connections in the Magnetosphere-Ionosphere-Thermosphere System: The Science Motivation for the Magnetosphere-Ionosphere Observatory (MIO)","This paper describes the scientific motivation for the NASA HMCS study of the MIO mission, which involves a relativistic-electron accelerator operated in the equatorial magnetosphere. MIO will reveal the connections between magnetospheric phenomena and ionospheric phenomena enabling the magnetospheric drivers of various aurora, ionospheric phenomena, and field-aligned currents to be determined.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-f944caaf02c48e67253397e58f9ad9f8_BorovskyJosephE1.pdf"
"139","5 September 2022 2:58:44 pm","Yeimy","Rivera","0000-0002-8748-2123","Center for Astrophysics | Harvard & Smithsonian","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-99f719003329edb67ad10c13b58adef2_SSPHWhitePaper_heavies.xlsx","Basic Research","Solar Physics","","","","","","","","","","Deciphering the Birth Region, Formation, and Evolution of Ambient and Transient Solar Wind Using Heavy Ion Observations","This white paper outlines the key scientific topics to address in the upcoming decade using observations of heavy ion composition that include the understanding the drivers behind the corona's variable chemical composition, the creation of the solar wind, and identifying the principle mechanisms driving solar wind evolution from the Sun.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-7cccef21c39b14db212f13d6be2d0129_RiveraYeimyJ2.pdf"
"140","5 September 2022 3:39:03 pm","Nicholas","Pedatella","0000-0002-8878-5126","High Altitude Observatory, National Center for Atmospheric Research","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-799b7645102583b3dd05107829efbf86_SSPH_White_Paper_Author_Information_Form_NP.xlsx","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop;Other Space Weather","","","","","","","Development of Data Assimilation Systems for the Ionosphere, Thermosphere, and Mesosphere","To fully realize the capabilities of ionosphere, thermosphere, and mesosphere (ITM) data assimilation (DA) systems for both scientific investigations and operations, several critical advances are needed. This white paper outlines the outstanding challenges facing ITM DA that need to be addressed in the coming decade, and details how these will benefit the scientific and operational communities.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-f27c97358a319a88eae8869d6068350d_PedatellaNicholasM.pdf"
"142","5 September 2022 5:39:43 pm","Rachael","Filwett","0000-0002-5497-7867","University of Iowa","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-17d8703b91239d96db719c5379308e8c_SSPH_White_Paper_Author_Information_Form_CIR.xlsx","Basic Research","Basic research that is driven by space weather user needs;Other topic relevant to solar and space physics/heliophysics","","","","","","","","","","Importance of Stream Interaction Regions to Space Weather and Energetic Particle Predictions","Stream Interaction Regions (SIRs), also known as Corotating Interaction Regions (CIRs) play an extremely important role in particle acceleration and transport in the heliosphere. Understanding SIRs is important to fundamental understanding of particle acceleration and better space weather predictions. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-e663acae3404a2f4e7844762e8136d36_FilwettRachaelJ2.pdf"
"143","5 September 2022 7:36:31 pm","Aimee","Merkel","0000-0001-9751-6481","Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-614c67b31100e1820ec12f628af755b6_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Other topic relevant to solar and space physics/heliophysics","","","Other Space Weather","","","","","","Space-based","Importance of satellite constellations to measure global ionosphere- thermosphere-mesosphere composition, temperature and winds","An opportunity for high impact science linking vertical coupling in the ionosphere- thermosphere-atmosphere region through the facilitation of constellation missions. It is our recommendation that a continual system of low Earth orbit constellations > 3 satellites each (i.e., A Starlink system for heliophysics, with the continuity of the GOES program) be a high priority in the 2024 decadal survey.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-019028c10286d7c0a0df2683a49a6608_Decadal_white_paper-Merkel_final.pdf"
"144","5 September 2022 8:52:35 pm","Glen","Fountain","0000-0001-7018-0586","Johns Hopkins University Applied Physics Laboratory","Nancy","Smith","Brandt","Diventi","","Lindsey","Clayton","Pontus","Anthony","","","","","","","[email protected]","[email protected]","[email protected]","[email protected]","","NASA","JHU/APL","JHU/APL","NASA","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","","Supporting Common Space Mission Needs -- An Integrated View To Enhance NASA's Science Missions","The paper recommends that the Decadal Survey recognize common resource demands and process challenges and recommend that these resources and challenges be managed across the Agency with greater specificity that currently. These include PuO2 for missions needing RPS and DSN downlink capacity. In addition, new processes are needed to guide the development of long duration missions.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-a118a1c71a71f01f7bba40cca8718565_FountainGlenH.pdf"
"146","5 September 2022 9:42:56 pm","Graham","Kerr","0000-0001-5316-914X","The Catholic University of America","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-4af2eabbfeaa501ffbae6c788f7cc4c1_GKerr_AuthorInfoForm_GradualPhase.xlsx","Basic Research","Solar Physics","","","","","","","","","","Requirements for Progress in Understanding Solar Flare Energy Transport: The Gradual Phase","Solar flares are a fundamental component of solar eruptive events . Flare emission is the first component of a SEE to impact the Earth's ionosphere which can set the stage for the later effects of the space weather event. In this white paper we discuss the flare gradual phase, setting out gaps in our understanding and paths towards resolving those gaps, including specific recommendations. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-3956342f79c8cf6bd7ebbd767475a229_HelioDecadal_Kerr_FlareEnergyTransport_Gradual.pdf"
"147","5 September 2022 10:08:16 pm","Graham","Kerr","0000-0001-5316-914X","The Catholic University of America","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-ed42c660672f09b5f4b41ec2a84bde60_GKerr_AuthorInfoForm_ImpulsivePhase.xlsx","Basic Research","Solar Physics","","","","","","","","","","Requirements for Progress in Understanding Solar Flare Energy Transport: The Impulsive Phase","Solar flares are a fundamental component of solar eruptive events . Flare emission is the first component of a SEE to impact the Earth's ionosphere which can set the stage for the later effects of the space weather event. In this white paper we discuss the flare impulsive phase, setting out gaps in our understanding and paths towards resolving those gaps, including specific recommendations. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-26e1ac1877b0cf807c7b8fa8600aa1da_HelioDecadal_Kerr_FlareEnergyTransport_Impulsive.pdf"
"148","6 September 2022 12:01:39 am","Vincent","Ledvina","0000-0003-0127-5105","Predictive Science Inc.","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-1ea780c46a12f4058bc3b92d62045599_LedvinaVincentE1.xlsx","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","How Open Data and Interdisciplinary Collaboration Improve Our Understanding of Space Weather: A Risk & Resiliency Perspective","By utilizing open data science, cross-disciplinary collaborations, information systems, and citizen science, we can forge stronger partnerships between science and industry and improve our readiness as a society to mitigate space weather impacts. These ideas fit into a broader space weather ""risk–resiliency framework"" that can be used to further assess areas of improvement in the field.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-1ef98847a323ee83a271bed0e637c49c_LedvinaVincentE1.pdf"
"149","6 September 2022 4:52:40 am","Paolo","Desiati","0000-0001-9768-1858","University of Wisconsin - Madison","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-8f2c72e67b5bd11d165833b76114c543_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Ground-based","Using TeV Cosmic Rays to probe the Heliosphere’s Boundary with the Local Interstellar Medium","The outer heliosphere regulates cosmic ray penetration into near-Earth space, reduces space radiation, and makes life possible in our solar system. Voyager and IBEX in-situ and remote observations of the outer heliosphere and the distorted local interstellar magnetic are important for heliospheric modeling. TeV cosmic rays provide a new tool to study the heliosphere interstellar medium boundary.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-9c4c96c05c3119f746fe5afffb86bbb4_Decadal_Survey_for_Solar_and_Space_Physics__Heliophysics__2024_2033_-_2022-09-06.pdf"
"150","6 September 2022 5:00:36 am","Leonardo","Regoli","0000-0002-7628-1510","Johns Hopkins Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-3ece4ea37e621dcc3c90281ab6ed6fae_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Planetary Magnetospheres;Planetary ionospheres/upper atmospheres","","","","","","","","","Space-based","Understanding the Evolution of Planetary Atmospheres: the need for an Earth-based atmospheric escape mission","Planetary atmospheres evolve with time in a complex way. To this point, we do not even understand what factors affect atmospheric escape. The only way to improve our understanding is by filling the observational gaps that exist to date. We present an attractive mission architecture to fill this gap by studying (and quantifying) atmospheric escape from our own planet, Earth. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-ae28cc0c2dd65fdf08a9d50becd7ec7f_RegoliLeonardoH.docx"
"151","6 September 2022 8:05:56 am","Christopher Stephen","Arridge","0000-0002-0431-6526","Physics Department, Lancaster University, UK","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-b2849575669ca984b3b81f8b16281366_ArridgeChristopherS.xlsx","Basic Research","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","Fundamental Space Physics in Uranus’ Magnetosphere","Uranus is one of the most under-explored and least understood planetary magnetospheres in our Solar System. Some features in the single Voyager 2 flyby cannot be explained, or for which we only have a limited explanation, highlighting fundamental gaps in our Space Physics. This requires new data to resolve and in this White Paper we urge Heliophysics to support a Uranus Flagship mission.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-186b9eba87eb9f08db2f20e83ede6beb_ArridgeChristopherS.docx"
"152","6 September 2022 8:20:35 am","Surajit","Mondal","0000-0002-2325-5298","New Jersey Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-eb7ffd4d98056d71ea8c59542c565b7f_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics","","","","","","","","","Ground-based","Weak transients and heating of the quiescent solar corona","Here we describe how FASR, a proposed radio interferometer, would be able to detect and characterise the nonthermal emission of small-scale coronal transients like microflares and nanoflares. This would ultimately would allow quantification of the nonthermal energy budget and its importance in the total coronal energy budget, a question which has been around for several decades now.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-897840d760001da4b9b549f5bb0ca7a5_MondalSurajit.pdf"
"153","6 September 2022 8:33:58 am","fabrizio","sassi","0000-0002-9492-7434","Naval Research Laboratory","Nicholas","","","","","Pedatella","","","","","0000-0002-8878-5126","","","","","[email protected]","","","","","High Altitude Observatory/NCAR","","","","","","Basic Research","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","","","","","","","","SassiFabrizio2.pdf","This white paper discusses the importance of whole atmosphere modeling and the need to continue to support this activity in the next decade for the Heliophysics community. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-48caf224958111f2d0a595bfe68a4665_SassiFabrizio2.pdf"
"154","6 September 2022 11:24:56 am","Jason","Kooi","0000-0002-5595-2522","U.S. Naval Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-131459962ba261eae2dc3f18c2a0d90f_SSPH_White_Paper_Author_Information_Form_AdvancingFR.xlsx","Basic Research","Solar Physics;Other topic relevant to solar and space physics/heliophysics","","","","","","","","","","How to Advance Studies of Coronal Faraday Rotation","Detection of Faraday rotation (FR) is one of the best radio remote-sensing methods for probing the plasma structure, including the magnetic field, of the solar wind and coronal mass ejections (CMEs). We outline several recommendations to continue developing FR methods over the next decade.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-5178b855d3af831806c533d934531569_KooiJason2.pdf"
"155","6 September 2022 11:54:39 am","Gerard","Daelemans","","NASA Goddard Space Flight Center","Steven","","","","","Christe","","","","","0000-0001-6127-796X","","","","","[email protected]","","","","","NASA Goddard Space Flight Center","","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Other Programmatic","","","Space-based","Enabling increased access to space for scientists from all backgrounds","This presentation will describe how past approaches used to successfully enable low cost quick reaction experiments from a diverse set of PIs on the NASAs Space Shuttle provide key features required of a new paradigm of partnering and project implementation between NASA and the science community and underrepresented Minority Serving Institutions, HCBUs, etc.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-08396d14f05664c755fb0ec8f9b1992a_DaelemansGerardJ.pdf"
"156","6 September 2022 11:57:43 am","John","Haiducek","0000-0002-4027-8475","US Naval Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-d5fcb0dfc23b6948380585823c27602d_HaiducekJohnD1.pdf","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","","Space physics is behind the curve in terms of statistical rigor","Statistical hypothesis tests and checks for statistical significance are standard in other fields of science, but relatively uncommon in space physics. Lack of statistical rigor can create obstacles for reproducibility and harm the reputation of the field. I recommend increased education in statistics and that statistical rigor be considered when evaluating submissions for funding or publication.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-d8a1b67259ff693d8853d6bf38808f3f_HaiducekJohnD1.pdf"
"157","6 September 2022 12:06:12 pm","John","Haiducek","0000-0002-4027-8475","US Naval Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-cd52c8168285731f10811c82a6d88e5a_HaiducekJohnD2.pdf","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","","Space physicists need to up their software development game","Most space physicists have little or no formal training in computer science or software engineering. This leads to shortcomings in software development efforts, harming the reliability of the software and the reproducibility of research. In addition, poor understanding of software licensing leads to license violations and misleading statements about software licenses.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-b4923e8890150dc00f78973dac5ac129_HaiducekJohnD2.pdf"
"158","6 September 2022 12:10:20 pm","Serena","Criscuoli","0000-0002-4525-9038","National Solar Observatory","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research;Infrastructure, Workforce, Other Programmatic","Solar Physics;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","GROUND-BASED MONITORING OF THE VARIABILITY OF VISIBLE SOLAR SPECTRAL LINES FOR IMPROVED UNDERSTANDING OF SOLAR AND STELLAR MAGNETISM AND DYNAMICS","We illustrate the scientific return and explore the technical requirements of a network of spectrographs devoted to long-term monitoring disk-integrated, solar spectral variability at high spectral resolution and high photometric accuracy. The proposed sun-as-a-star observations offer the opportunity for a variety of multidisciplinary studies including stellar variability and Sun-Earth connection.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-5264a76f5a95ee99513691561b9979be_CriscuoliSerena1.pdf"
"159","6 September 2022 12:19:38 pm","William","Kurth","0000-0002-5471-6202","University of Iowa","Stuart","","","","","Bale","","","","","0000-0002-1989-3596","","","","","[email protected]","","","","","Univ. of California/Berkeley","","","","","","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","","KurthWilliamS.pdf","This white paper advocates for radio and plasma wave measurements in the Very Local Interstellar Medium (VLISM) to provide accurate plasma densities and temperatures as well as remote-sensing evidence of solar transient-induced perturbations The wave observations also provide a measure of dust flux for 0.1 to ~few micron dust grains.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-cc1499da2a3f113c24e14b4f70171341_KurthWilliamS.pdf"
"160","6 September 2022 12:30:56 pm","Emily","Mason","0000-0002-8767-7182","Predictive Science Inc.","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-ae592b8ff52d9353acf62e814049087d_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","Inner Heliosphere and solar wind interaction with unmagnetized bodies;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","Space Weather Pipeline from Research to Application to Operations","","","","","","","Enabling Critical Solar Wind Research via Consistent, Comprehensive Inner Heliosphere Data Coverage","Solar wind creation and early evolution is fundamental to Heliophysics. Advances require reliably tracking individual packets of solar wind from the low corona to 1 AU. We need 360˚, high-resolution, high-cadence coronal and solar wind measurements. These are bottom-line requirements to advance basic research, space weather modeling, and operational forecasting.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-10c987201aa10c0d14ed6c19011baab0_MasonEmilyI.pdf"
"161","7 September 2022 1:09:01 pm","Bea","Gallardo-Lacourt","0000-0003-3690-7547","NASA-GSFC/CUA","Gareth","Bharat","Carlos","","","Perry","Kunduri","Martinis","","","0000-0002-4690-5783","0000-0002-7406-7641","0000-0002-1085-7871","","","[email protected]","[email protected]","[email protected]","","","New Jersey Institute of Technology","Virginia Tech","Boston University","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-c365e0180fea539fe5dab682894c9a95_Subauroral_White_Paper_Author_Information_Form.xlsx","Basic Research","Planetary Magnetospheres;Planetary ionospheres/upper atmospheres","","","","","","","","","","The importance of extreme dynamic signatures in the sub-auroral region","In recent years it has become increasingly clear that there are several unexplored aspects of the sub-auroral region that remain elusive in part due to instrumental and observational limitations. This white paper highlights some of the open questions in the sub-auroral region that have arisen since the previous decadal survey and provides recommendations on how science advances can be achieved.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-78dbbdc73ff5d1e8a42ec079479d2720_Subauroral_WhitePaper.pdf"
"162","6 September 2022 12:42:30 pm","Jasper","Halekas","0000-0001-5258-6128","University of Iowa","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-407e5cd8880f21100bfb893016dc6b19_Moon_Heliophysics_White_Paper_Author_Information.xlsx","Basic Research;Space Weather Applications","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Planetary Magnetospheres","","","Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","","The Value of the Moon for Heliophysics","The Moon represents an ideal heliophysics laboratory for the investigation of kinetic plasma physics, in situ measurements of the interplanetary and terrestrial environment, and remote measurements of geospace and beyond. Frequent future planned launches to the lunar vicinity, and international interest, make the Moon an appealing and accessible target for valuable heliophysics investigations.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-878c61ce386b12678b157ef920ab46c7_HalekasJasperS.pdf"
"163","6 September 2022 12:53:13 pm","Rafael Luiz","Araujo de Mesquita","0000-0003-4681-8679","The Johns Hopkins Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-bfb8cc816506a6dc4273ebf8f85b48b7_SSPHWhitePaperAuthorInformationForm_RM_OnDemand.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","Space-based","On-demand deployables: From sounding rockets to space-based missions in the study of E-region neutral- and electrodynamics","Small and mid-scale phenomena in Earth's thermosphere and E-region are severely under-sampled. Satellite observations are horizontally smeared and ground-based observations are insufficient. The solution: a modernization of the falling spheres technique to probe in situ the neutral and electrodynamics between 80 and 200 km. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-af01214e4dcf5de9aca08e87785ad275_DecadalWhitePaper_OnDemandDeployables_FINAL.pdf"
"164","6 September 2022 1:36:54 pm","Sadie","Elliott","0000-0001-8661-7252","University of Minnesota","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-b8789347399597e2de5e40fbc5a5ab52_SSPHWhitePaperAuthorInformationForm_Elliott.xlsx","Basic Research;Space Weather Applications","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Space-based","Understanding the properties, wave drivers, and impacts of electron microburst precipitation: current understanding and critical knowledge gaps","Understanding and quantifying the underlying causes and consequences plus relative importance of microburst precipitation represent outstanding questions in radiation belt physics. Important questions remain about the nature of the resonance generating the microbursts and the overall importance of the precipitation. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-25e9b590219f5e74e97fbdb4d3965d83_ElliottSadieS.pdf"
"165","6 September 2022 1:41:27 pm","Alfred","de Wijn","0000-0002-5084-4661","National Center for Atmospheric Research","Steven","Joan","Roberto","Giuliana","","Tomczyk","Burkepile","Casini","de Toma","","0000-0001-7399-3013","0000-0002-9959-6048","0000-0001-6990-513X","0000-0002-8439-6166","","[email protected]","[email protected]","[email protected]","[email protected]","","National Center for Atmospheric Research","National Center for Atmospheric Research","National Center for Atmospheric Research","National Center for Atmospheric Research","","","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Ground-based","COSMO ChroMag: The Chromosphere and Prominence Magnetometer","We discuss the Chromosphere and Prominence Magnetometer (ChroMag) of the Coronal Solar Magnetism Observatory. ChroMag will provide the community with synoptic observations of magnetic field in the chromosphere that are currently unavailable yet critical to many outstanding questions about the processes that operate on both short and long timescales in the outer solar atmosphere.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-9a2ecd41f1e6b12da520057c1b747249_DeWijnAlfredG.pdf"
"166","6 September 2022 3:05:16 pm","William","Dunn","0000-0002-0383-6917","University College London","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-a8229af404a28d8d8c05e91c0e5cb7b0_SSPHWhitePaperAuthorInformationForm_Jupiter_X-rays.xlsx","Basic Research","Planetary Magnetospheres;Other topic relevant to solar and space physics/heliophysics","","","","","","","","","Space-based","Exploring Fundamental Particle Acceleration and Loss Processes in Heliophysics through an Orbiting X-ray Instrument in the Jovian System","In companion Decadal white papers(Clark+,2022;Kollmann+,2022;Turner+,2022), we present the case for exploring fundamental acceleration & loss processes in heliophysics through the natural laboratories of Jupiter's radiation belts and mission concept COMPASS. Here, we focus on using X-rays for global context, to address longstanding questions & to provide a stepping-stone to astrophysical systems.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-abbbfc01c6c86d319e750fe035fe5372_Helio_Jupiter_X-rays_White_Paperv2-1.pdf"
"167","6 September 2022 3:13:41 pm","Jeffrey P.","Thayer","0000-0001-7127-8251","University of Colorado","Tomoko","Robert","Theodoros","Weijia","Nickolay","Matsuo","Pfaff","Sarris","Zhan","Ivchenko","0000-0002-2754-1224","0000-0002-4881-9715","0000-0002-0336-2678","","0000-0003-2422-5426","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","Ann and H.J. Smead Department of Aerospace Engineering Sciences, University of Colorado at Boulder, CO","Goddard Space Flight Center","Department of Electrical and Computer Engineering, Democritus University of Thrace, Xanthi, Greece","Space Weather Technology, Research, and Education Center, University of Colorado","Royal Institute of Technology KTH, Stockholm, Sweden","","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Ground-based;Space-based","Understanding High-Latitude Frictional Heating and Momentum Exchange in the I-T System","This white paper identifies key observations and methods required to make advancements in determining collisional exchange processes at high latitudes that will improve our ability to predict and interpret the I-T system response . Collisional exchange processes involve momentum and energy transfer between neutrals and ions. The high-latitude F-region is of particular focus.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-47c169801aaa65f1a09a4e762942f2d2_ThayerJeffreyP.pdf"
"168","6 September 2022 3:28:04 pm","Alex","Glocer","0000-0001-9843-9094","NASA/GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-2e74f21fcc8881d4a088ce13d7659278_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Planetary Magnetospheres;Planetary ionospheres/upper atmospheres","","","","","","","","","","The Outflow and Recirculation of Ionospheric Plasma","The omnipresence of ionospheric plasma throughout geospace affects every aspect of Earth's magnetosphere and is critical for modeling space weather. Ionospheric escape is a universal process at every planet and is crucial for understanding atmospheric evolution and space weather. This white paper discusses open issues in ion outflow and plasma recirculation in the magnetosphere.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-e4030adddcf44fc7b7e9b5f9cb384e46_GlocerAlex.pdf"
"169","6 September 2022 3:34:14 pm","Jason","Kooi","0000-0002-5595-2522","U.S. Naval Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-0309f5e2e0a0fb1d4f3222f8b7688216_SSPH_White_Paper_Author_Information_Form_FRtomography.xlsx","Basic Research","Solar Physics;Basic research that is driven by space weather user needs","","","","","","","","","","Progressing Towards Faraday Rotation Tomography of the Solar Wind","We describe the steps necessary to realize Faraday rotation tomographic scanning of the corona. Spacecraft could be used to quickly generate low resolution tomographic scans suitable for studying coronal mass ejections, critical to developing early warning space weather forecasting systems, and natural radio sources would be suitable for studying slowly-evolving coronal structures like streamers.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-9435f5be75b42f11441fee21c9ec93f7_KooiJason3.pdf"
"170","6 September 2022 3:39:25 pm","Jennifer","Gannon","","CPI","Drew","Thomas","Bala","Antti","","Turner","Berger","Poduval","Pulkkinen","","","","","","","[email protected]","[email protected]","","[email protected]","","Johns Hopkins University Applied Physics Lab","University of Colorado - Boulder","University of New Hampshire","NASA Goddard","","","Space Weather Applications","","","","Other Space Weather","","","","","","","Introduction to a Space Weather Community Whiteaper Collection","In preparation for the approaching Heliophysics Decadal Survey, a group of space weather experts and enthusiasts took on an effort to coordinate community-wide action on space weather white paper preparations. This white paper outlines the processes used and lists the white papers included in the collection.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-567ab806c1a2547e9f19992e8f5d0110_GannonJenniferL3.pdf"
"171","6 September 2022 3:49:54 pm","Noé","Lugaz","0000-0002-1890-6156","University of New Hampshire","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-20d870145b2ef836d21dda1c35ff44e5_SSPH__MHM_author_list.xlsx","Basic Research;Space Weather Applications","Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","Other Space Weather","","","","","","Space-based","The Multi-spacecraft Heliospheric Mission (MHM)","The Multi-spacecraft Heliospheric Mission is a versatile mission concept to determine the variations of solar wind streams, transients, and energetic particles in the inner heliosphere and advance our knowledge of how to forecast space weather. MHM fills a clear gap in NASA HSO, identified in the 2003 Decadal Survey and NASA Space Weather Gap Analysis. It can be proposed as a SMEX (MIIST).","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-b80d6e1dfa1cdbc636adae1651356646_LugazNoe2.pdf"
"172","6 September 2022 3:51:11 pm","Mykhaylo","Shumko","0000-0002-0437-7521","NASA's Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-09647a35517c1d230326cd494b3d90b9_MykhayloShumko1_Author_Information_Form.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary Magnetospheres","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Recommendations on Funding Mission Operations and Historical Datasets","NASA's and NSF's small mission grants primarily fund the development and construction of instrumentation. A side effect of this approach is that mission operations tend to be severely under budget (or unfunded). In order to fully utilize current and past missions, we recommend adding new funding sources for mission operations and data analysis of underutilized historical datasets.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-ee555dc39032f222c5db50676825e58c_ShumkoMykhaylo1.docx"
"173","6 September 2022 3:55:53 pm","Kathryn","Whitman","0000-0002-3787-1622","KBR, NASA JSC SRAG","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-07b4ff946df46ae65085eb00267981fc_SEP_Whitman_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","Basic research that is driven by space weather user needs","","","Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","","Advancing Solar Energetic Particle Forecasting","With growing interest from the aviation and satellite industries, and for NASA's upcoming Artemis lunar missions, the need for improved scientific understanding and accurate forecasting of solar energetic particle events has never been stronger. In this paper we discuss the observational, validation and model transition support required to achieve these goals.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-491d22a44bbf328975fb4126b0364fda_WhitmanKathryn1.docx"
"175","6 September 2022 4:15:54 pm","David","Sibeck","0000-0003-3240-7510","NASA GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-b5dd84395343d8b7311fee0ce168d57e_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Ground-based;Space-based","Imaging the End-to-End Dynamics of the Global Solar Wind-Magnetosphere Interaction","This paper describes how a single spacecraft in a circular polar orbit provides observations essential to quantify the system science of the solar wind-magnetosphere interactions using its own observations of the solar wind input, the magnetopause, the auroral oval, the ring current, the plasmasphere, and the exosphere, in conjunction with ground-based observations of the nightside auroral oval.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-3f3d4794a7b336a460e7035693f3cc50_SibeckDavidG.pdf"
"176","6 September 2022 4:23:56 pm","Richard","Morton","0000-0001-5678-9002","Northumbria University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-1f653ec3591fedbf981d455e4600cd0e_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Solar Physics","","","","","","","","","","Revealing the Sun’s Alfvénic waves","Alfvénic waves are thought to be a key mechanism for energy transfer in the Sun's atmosphere. However, details of the waves journey from photosphere to corona to solar wind remain unverified. The Alfvénic waves also offer the chance to explore the difficult to measure coronal magnetic field. New and future instrumentation will provide exciting opportunities to probe the Alfvénic waves. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-7d6a76f7328a77f6fffa7108268e54cb_MortonRichardJ.docx"
"177","6 September 2022 4:40:17 pm","David","Hysell","0000-0001-7410-7335","Cornell University","Anthea","Philip","Roger","","","Coster","Erickson","Varney","","","","","","","","[email protected]","[email protected]","[email protected]","","","","","","","","","Basic Research;Infrastructure, Workforce, Other Programmatic","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Basic research that is driven by space weather user needs","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","A Geospace Radar NSF Midscale Project","We outline a proposal for a Geospace Radar to update the existing NSF AGS Facilities . The whitepaper reviews conclusions from a recent NSF-sponsored workshop and then focuses on the science objectives that could be met with a Geospace Radar deployed in the subauroral zone and the technological developments required to realize it. Workforce development surrounding the project is emphasized.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-fe2657809c79f7988be7cf4a0afe30dc_wp_geospace_midscale.pdf"
"178","6 September 2022 4:45:20 pm","Mihir","Desai","0000-0002-7318-6008","Southwest Research Institute","David","Silvia","Ming","Christina","","Lario","Dalla","Zhang","Cohen","","0000-0002-3176-8704","0000-0002-7837-5780","0000-0003-3529-8743","0000-0002-0978-8127","","[email protected]","[email protected]","[email protected]","[email protected]","","NASA, GSFC","University of Central Lancashire","Florida Institute of Technology","California Institue Of technology","","","Basic Research","Other topic relevant to solar and space physics/heliophysics","","","","","","","","","Space-based","Energetic Particle Propagation in Three Dimensions","Ulysses observations during its rapid transit over the polar regions of the Sun challenged our understanding of SEP transport in 3 dimensions. This white paper provides the scientific justification for obtaining new measurements out-of-the-ecliptic plane so that we can fully understand particle transport in the inner heliosphere.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-22ea42e293e89f82193b876220a01086_Desai_etal-White-paper.pdf"
"179","6 September 2022 4:55:53 pm","Brian","Wood","0000-0002-4998-0893","Naval Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-fe0a443a10a14df3469978d2866eb784_WoodWP_author_list.xlsx","Basic Research","Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","","","","","Sensing CME Magnetic Fields En Route to 1 AU","The central argument of this white paper is that a focus on future CME research should be on improving our ability to observe CME magnetic fields and monitor their evolution from the Sun and into interplanetary space. Field diagnostics discussed include polarimetric measurements in the corona, radio Faraday rotation observations near and far from the Sun, and spacecraft magnetometer data.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-b17295fd19f842b4bc35ad413fba7105_WoodBrianE.pdf"
"180","6 September 2022 4:56:59 pm","Ryan","McGranaghan","https://orcid.org/0000-0002-9605-0007","Orion Space Solutions; NASA/GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-e665f2ca3425a4e079b14cb851b91645_HelioDecadal_WP_Author_Information_-_Knowledge_Commons.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","","The need for a Solar and Space Physics Knowledge Commons","The magnitude and complexity of the problems confronting Solar and Space Physics from 2024-2033 require the integration of many individuals, groups, data sources, and technologies (i.e., the interconnection of all of our knowledge). The solution is a 'knowledge commons.'","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-66d45ca0aca67f6a8995b2a8bbd49379_McGranaghanRyanM1.pdf"
"181","6 September 2022 5:03:20 pm","Karl","Battams","0000-0002-8692-6925","US Naval Research Laboratory","Dogacan","Ramanakumar","Kameswara Bharadwaj","","","Ozturk","Sanka","Mantha","","","0000-0002-8071-2707","0000-0002-6794-7587","","","","[email protected]","[email protected]","[email protected]","","","University of Alaska-Fairbanks,","University of Minnesota","University of Minnesota","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","","Sustainability Support for Heliophysics Citizen Science Projects","We propose enhanced sustainability support for Heliophysics Citizen Science (CS) Projects via: (1) the creation of a centralized Citizen Science Resource Center to provide expertise, support, and resources to new and existing CS projects; and (2) creation of additional funding opportunities to support the technological and resource needs of new and operating CS projects","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-c6f01dba2ebc5acb40b465d2c1bf9040_BattamsKarl.pdf"
"182","6 September 2022 5:19:31 pm","Adam","Kellerman","0000-0002-2315-936X","University of California Los Angeles","Yihua","Alexa","Katherine","Thomas","","Zheng","Halford","Garcia-Sage","Chen","","0000-0002-2569-2950","0000-0002-5383-4602","0000-0001-6398-8755","0000-0002-0294-3614","","[email protected]","[email protected]","[email protected]","[email protected]","","NASA/GSFC","NASA/GSFC","NASA/GSFC","Columbia University","","","Space Weather Applications","","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","","Developing standards, metrics, and systematic approaches for improved model performance verification and validation","Model verification and validation (MVV) are critical to ensure that our models and simulations are reliable and correct. The need for applications that inform decision making is rising every year, and along with it, the need for MVV and clear frameworks to enable research-to-applications-to-research (R2A2R) within and beyond the heliophysics community. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-001bd8e809a7bd5bc26100b0d6d24b67_Kellerman_etal_MVV.pdf"
"183","6 September 2022 5:36:35 pm","Anish","Roshi","","University of Central Florida","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-c16e2c0eb6917afcb9da4731766b435c_SSPHWhitePaperAuthorInformationForm%25281%2529.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Other topic relevant to solar and space physics/heliophysics","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","The Next Generation Arecibo Telescope (NGAT)","Arecibo excelled in three separate, major scientific areas, planetary science, space and atmospheric sciences, and astronomy. We envision a new, unparalleled facility, We present a concept for the Next Generation Arecibo Telescope (NGAT) - an innovative combination of a compact, phased array of dishes on a steerable plate-like structure.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-533522621f1ba667ea0b73ea3303d4e3_NGATwhitePaper.docx"
"184","6 September 2022 5:31:45 pm","Rachael","Filwett","0000-0002-5497-7867","University of Iowa","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-e7a4829b100bda6a29630edf1a8902be_SSPH_White_Paper_Author_Information_Form_Accessibility.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","Accessibility and its Importance to the Future of Heliophysics","The accessibility of the activities and spaces that heliophysics occupies is connected to our ability to maintain a diverse and inclusive group of scientists. We recommend assessing the inclusion of those with disabilities in heliophysics in metrics related to the state of the profession and promoting policies that make gatherings and educational settings more accessible.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-b915a194e82681ae4990017bad624ed3_FilwettRachaelJ1.pdf"
"185","6 September 2022 5:35:26 pm","Stephen","White","0000-0002-8574-8629","Air Force Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-71357784da0ebca08dec7d3a90a77e2e_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","","The Importance of Synoptic Solar Radio Observations","We discuss the results of the long-term monitoring of solar radio fluxes and the importance of maintaining this record. The long history informs our understanding of the solar activity cycle and the physics of the solar atmosphere, and is increasingly important for understanding the context and likely impact of stellar activity on exoplanets.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-c1388f63a2c89a99a55d613384c4e247_WhiteStephenM1.pdf"
"186","6 September 2022 5:45:47 pm","Stephen","White","0000-0002-8574-8629","Air Force Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-e48bcdd5d2757a6b6e1facf53bd99f09_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","","Extreme Solar Radio Bursts","Extreme solar radio bursts can impact several areas of human activity, but there remain many gaps in our understanding of what leads to their occurrence. The properties of extreme bursts are discussed, and shortcomings in our understanding of such events are presented.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-341b991d639f11186c8ef9b1874027bc_WhiteStephenM2.pdf"
"187","6 September 2022 5:56:54 pm","Frank","Crary","0000-0003-2949-8589","University of Colorado, LASP","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-f9f333f97b5e3cac636db25205cbfc64_Helio_White_Paper_Author_Information_Form.xlsx","Basic Research","Planetary Magnetospheres","","","","","","","","","Space-based","The Magnetosphere of Jupiter: Moving from Discoveries Towards Understanding","The magnetosphere of Jupiter has been observed by many spacecraft. The results have been discoveries of the global and general properties of the magnetosphere. They have typically raised more questions than they answered. We present some of the outstanding issues in understanding Jupiter's magnetosphere and argue that this can be accomplished with small, focused missions.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-e1469947da1deb43dba17da749a82c79_CraryFrankJ.pdf"
"188","6 September 2022 6:26:05 pm","Jason","Kooi","0000-0002-5595-2522","U.S. Naval Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-15bf422155a022f381f003c4e4ee0ab6_SSPH_White_Paper_Author_Information_Form_DFRandFRF.xlsx","Basic Research","Solar Physics;Other topic relevant to solar and space physics/heliophysics","","","","","","","","","","Faraday Rotation Methods to Detect Coronal Currents and MHD Wave Activity","Faraday rotation (FR) observations of the solar wind can address questions such as ""How is the solar wind accelerated?"" and ""What is the origin and evolution of the meso-scale plasma and magnetic field structure of the solar wind?"" Differential FR can be used to detect electric currents and short-timescale FR fluctuations can provide information on magnetohydrodynamic wave activity.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-f1e8d8d1bcba2c2787099cb799bb104f_KooiJason4.pdf"
"189","6 September 2022 6:32:52 pm","Douglas","Rowland","0000-0003-0948-6257","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","ACCESS -- Applications of Commercial Constellations for Expanded Science and Space weather","ACCESS is a proposed component of the next-generation LWS architecture that would invest in leveraging commercial constellations to provide high science value to NASA as well as space weather data of national utility. ACCESS comprises a number of recommendations including several that will enable NASA to fly highly-replicated sensors in dense observation networks, producing groundbreaking science.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-a4b15183aca17ad16616abc481cb301f_RowlandDouglasE1.pdf"
"190","6 September 2022 6:32:56 pm","Mikhail","Sitnov","0000-0002-8990-0456","The Johns Hopkins University Applied Physics Laboratory, Laurel, MD","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-2d3a50535f93443ba587f03df2f46053_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Planetary Magnetospheres","","","","","","","","","","Artificial Intelligence to Enhance Mission Science Output for In-situ Observations: Sparse Data Challenge and Gray-Box Models","To meet the challenge of sparse data sampling in case of in-situ observations in Earth's magnetosphere, we propose to use modern artificial intelligence tools. To use of the acquired data and empirical reconstructions in the first-principles models it is proposed to develop gray-box models that combine simulations (white-box models) and data-derived reconstructions (black-box models). ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-df117de18e8033d09663fbab8da727ac_SitnovMikhailI.pdf"
"191","6 September 2022 6:38:34 pm","Jon","Linker","0000-0003-1662-3328","Predictive Science Inc","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-ca6d8de9b7b024745b6710da4a9ec8b4_Open_Flux_Problem_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","","","","","The Open Flux Problem: The Need for High Latitude Observations","The open magnetic flux is a central feature of the solar corona and heliosphere. Solar observations of the open flux consistently underestimate the measured interplanetary flux. Resolving the poorly measured contribution of the Sun's polar magnetic fields to the open flux requires observing the LOS magnetic field above 65 degrees latitude, with accompanying EUV detections of coronal holes.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-82986a9cfe2f8e82d80b1efd267e551d_LinkerJonA.pdf"
"192","6 September 2022 6:43:25 pm","Alex","Chartier","0000-0002-4215-031X","Johns Hopkins University Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-acc0191887da5b9d1d002eedf5d26417_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop;Other Space Weather","","","","","","Ground-based","Networked HF Sounding to Determine the High-Latitude Ionospheric Conductivity","The critical observational unknown that links the magnetosphere, ionosphere and atmosphere is the conductivity. At present the conductivity is poorly observed. Here we argue that distributed HF remote sensing is the best means of achieving the required observational coverage of this parameter, due to its relatively low cost, proven success in operational applications, and scalability. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-4659a0bf524a798942448decb8ca2d05_ChartierAlexT.pdf"
"193","6 September 2022 6:45:33 pm","Jason","Kooi","0000-0002-5595-2522","U.S. Naval Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-ef831cdf28c6763f0b00d39a52201786_SSPH_White_Paper_Author_Information_Form_CMEFR.xlsx","Basic Research","Solar Physics;Basic research that is driven by space weather user needs","","","","","","","","","","Probing the Magnetic Field Structure of Coronal Mass Ejections with Faraday Rotation","Observation of Faraday rotation (FR) is the most promising candidate to provide remote-sensing measurements of CME magnetic fields. FR methods have finally matured to the point where they can be used to return the strength and, most importantly, the orientation of CMEs shortly after eruption. We discuss how to continue progressing towards using FR for space weather monitoring and forecasting.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-e50ef42c5c1b85a6489753d3a69583ee_KooiJason5.pdf"
"194","6 September 2022 6:47:58 pm","Alex","Chartier","0000-0002-4215-031X","Johns Hopkins University Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-bb0ac5bb9a9a66f446a4c36d61387c29_SSPH_White_Paper_Author_Information_Form_copy.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","","","","","","","","Understanding the Transfer of Electromagnetic Energy Between the Earth’s Magnetosphere and Upper Atmosphere","Electromagnetic energy is likely the largest unknown input to the upper atmosphere. Together with precipitating particles, it may constitute the largest overall source of energy during geomagnetic storms. This source of energy is a critical driver of stormtime dynamics, and is responsible for plasma convection, atmospheric upwelling in the cusps, as well as many other important phenomena. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-bfe61d253a85a225a61917888ebcb58f_ChartierAlexT.pdf"
"195","6 September 2022 6:49:20 pm","George","Clark","0000-0002-5264-7194","Johns Hopkins Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-c041e7832bf39d79afc66d49e3666c74_SSPH_White_Paper_Author_Information_Form_COMPASS.xlsx","Basic Research","Planetary Magnetospheres;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","Comprehensive Observations of Magnetospheric Particle Acceleration, Sources, and Sinks (COMPASS)","In this white paper, we present COMPASS, a novel mission concept designed to explore the uncharted and hazardous regions of Jupiter with highly capable instrumentation with the goal of making fundamental discoveries in space physics. The basic motivation to explore such a hazardous region is to expand the frontiers of Heliophysics in the next decade by investigating extreme radiation environments.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-1ec7e3cd1d519ac59b45e11010a8a8e2_ClarkGeorgeB.pdf"
"196","6 September 2022 6:52:54 pm","Alex","Chartier","0000-0002-4215-031X","Johns Hopkins University Applied Physics Laboratory","Tom","Kate","","","","Sotirelis","Zawdie","","","","","","","","","[email protected]","[email protected]","","","","Johns Hopkins University Applied Physics Laboratory","Naval Research Laboratory","","","","","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","Space-based","STP Mission Concept: A Remote-sensing Ionospheric Network in Geospace","We propose a conceptual Remote-Sensing Ionospheric Network in Geospace (RING) mission for the Solar-Terrestrial Probes Program to observe the global electromagnetic and kinetic energy inputs, and the global ionospheric system response. The proposed constellation consists of 100+ observing platforms in low Earth orbit to determine global E, dB, and particles, plus 3D electron density. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-2205e23ca39e3c1eca5e6451731327db_ChartierAlexT.pdf"
"197","6 September 2022 7:00:32 pm","Alex","Chartier","0000-0002-4215-031X","Johns Hopkins University Applied Physics Laboratory","Adrienn","Frank","Paul","Devin","","Luspay-Kuti","Lind","Bernhardt","Huyghebaert","","","","","","","[email protected]","[email protected]","[email protected]","[email protected]","","Johns Hopkins University Applied Physics Laboratory","Massachusetts Institute of Technology","University of Alaska-Fairbanks","UiT Tromsø, Arctic University of Norway","","","Basic Research","Planetary ionospheres/upper atmospheres","","","","","","","","","Ground-based","Interplanetary Ionospheric Topside Sounding from Earth","We propose that planetary ionospheres be observed using terrestrial radio transmitters and receivers. Planetary ionospheres have long been recognized as high-value targets, but measurements are scarce. Planets as far as Jupiter may be observable using current technology, while observation of outer bodies requires construction of new systems and creation of temporary holes in Earth's ionosphere. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-d0a452fa601aeb29a3f3f5302d23b27e_ChartierAlexT.pdf"
"198","6 September 2022 7:10:07 pm","Russell","Howard","0000-0001-9027-8249","Johns Hopkins University Applied Physics Laboratory","Paulett","Angelos","","","","Liewer","Vourlidas","","","","0000-0002-5068-4637","0000-0002-8164-5948","","","","[email protected] < [email protected]>","[email protected]","","","","JPL Calech","JHU APL","","","","","Basic Research;Space Weather Applications","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","","On the Impact of Viewing Coronal Mass Ejections From a Position Off the Ecliptic Plane","Getting out of the ecliptic plane by 40deg is very advantageous for a non-degenerate view and to help better determine the topology of coronal mass ejections.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-41282556a90e1e9edbfadc15cf9ab36c_HowardRussellA.docx"
"199","6 September 2022 7:21:05 pm","Peter","Kollmann","0000-0002-4274-9760","Johns Hopkins University Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-53b871e325018bcdf9f5a1a30e5a702f_KollmannPeter1.xlsx","Basic Research","Planetary Magnetospheres;Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","","Jupiter’s radiation belts as a target for NASA’s Heliophysics Division","Jupiter is the largest particle accelerator in the solar system and therefore an ideal laboratory to study fundamental heliophysics.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-06684e9c790c809b240f366f137825e6_KollmannPeter1.pdf"
"200","6 September 2022 7:21:50 pm","Peter","Kollmann","0000-0002-4274-9760","Johns Hopkins University Applied Physics Laboratory","Drew L.","George","Ian J.","Elias","","Turner","Clark","Cohen","Roussos","","","","","","","","","","","","Johns Hopkins University Applied Physics Laboratory","Johns Hopkins University Applied Physics Laboratory","Johns Hopkins University Applied Physics Laboratory","Max Planck Insitute for Solar System Research","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","The Need for High Signal-to-Noise Charged Particle Measurements","We keep finding that our particle measurements need to have a large signal-to-noise ratio (SNR) and argue that there has been and will be a critical need to develop technologies and instrument designs with high SNR.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-a7da2a6a5f513bc1e4d110d84daaee01_KollmannPeter2.pdf"
"201","6 September 2022 7:22:28 pm","Alexa","Halford","0000-0002-5383-4602","NASA Goddard Space Flight Center","Benoit","Sabrina","Joe","Gina Luca","","Lavraud","Savage","Borovsky","Delzanno","","0000-0001-6807-8494","0000-0002-6172-0517","0000-0002-2325-3348","0000- 0002-7030-2683","","[email protected]","[email protected]","[email protected]","[email protected]","","Laboratoire d'astrophysique de Bordeaux, Univ. Bordeaux, CNRS, Pessac, France","NASA Marshall Space Flight Center","Space Science Institute","LANL","","","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Other Programmatic","","","","The need for reference-able and peer reviewed position papers","Decadal survey position papers can be a broader community resource if made easily searchable. Cite-able, peer reviewed position papers will further enhance the community support and strategic discussion for the future of our field. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-50c7306fc435249233f8b7692576d7b9_Citable_Decadal_Contributions.pdf"
"202","6 September 2022 7:25:10 pm","Emily","Lichko","0000-0003-1945-8460","University of Arizona","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-f4f4be1a7f1a7c2a67927ec7060765c4_Copy_Coauthor_Form.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Laboratory space plasma physics;Fundamental space plasma theory (not specific to a particular region)","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","","Enabling Discoveries in Heliospheric Science through Laboratory Plasma Experiments","Resolving 3D physics occurring on multiple spatial and temporal scales is difficult with spacecraft and computer simulations alone, but can be studied much more easily with laboratory plasma experiments. This white paper proposes increasing funding for both human and physical infrastructure development in existing laboratory plasma facilities.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-efdf7ab1d99312c45cdcc126026209e5_LichkoEmilyR.pdf"
"203","6 September 2022 8:01:55 pm","Gregory","Fleishman","0000-0001-5557-2100","New Jersey Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-d1959fd4a06cc80312cd01f8f6851d3c_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","","","","","Constraining coronal abundances with a combination of high resolution EUV and microwave data","This White Paper emphasizes the new utility of complementing the EUV data with spatially resolved microwave data to determine at the same time the relationship of the magnetic field with plasma parameters, and the composition of the solar corona. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-91a3cc82786b6414cf9905be93e3f0ad_FleishmanGregoryD.pdf"
"204","6 September 2022 8:27:58 pm","Michael","Hartinger","0000-0002-2643-2202","Space Science Institute","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-d80935ab016cfc3d876409792a712c3c_HartingerMichaelD.xlsx","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Ground-based","Global Networks of Ground-Based Magnetometers Enable Cutting-Edge Heliophysics Research, Education, and Space Weather Operations","Ground-based magnetometers used to measure magnetic fields on the Earth's surface (B) are central to Heliophysics research. We summarize present magnetometer infrastructure, describe research needed to improve our understanding of the causes and consequences of B, and describe infrastructure and policies needed to support this research and related space weather models.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-d4a83120fff40ef534e2a13e0a8349d4_HartingerMichaelD.docx"
"205","6 September 2022 9:13:11 pm","Caitlin","Ahrens","","NASA GSFC/NPP","Carey","Michael","Thomas","","","Lisse","Zemcov","Chen","","","","","","","","","","","","","JHU/APL","Rochester Institute of Technology","Columbia University","","","","Basic Research","Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","Infrared Spectral Science Priorities with an Interstellar Probe for Heliophysical Science","The nature of the dust in interstellar/interplanetary medium regarding infrared observations within the Heliosphere can be of interest to several studies and can be analyzed using an Interstellar Probe.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-b362dd8020576500f17d59f742882caa_AhrensCaitlinJ1.pdf"
"206","6 September 2022 9:20:46 pm","Caitlin","Ahrens","","NASA GSFC/NPP","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-27be75d33d2dd3928ba1d076bab5096d_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","","","","","","","","Space Weathering at the Moon: Priorities for Interdisciplinary Heliophysics and Planetary Science Research","The effects of space weathering complicate (or even prevent) the interpretation of compositional remote sensing, or the role of space weathering in the production, destruction, and cycling of volatiles on the surface of the Moon. Each of these mechanisms make the interplay between space weathering studies from the perspective of heliophysics and future lunar exploration a critical endeavor. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-253520587ed59a239114dd7d93bc7966_AhrensCaitlinJ2.pdf"
"207","6 September 2022 9:39:39 pm","Katrina","Bossert","0000-0002-7076-0449","Arizona State University","Christopher","","","","","Heale","","","","","0000-0003-1970-9004","","","","","[email protected]","","","","","Embry-Riddle Aeronautical University","","","","","","Basic Research","Planetary ionospheres/upper atmospheres","","","","","","","","","","The need for thermosphere wind measurements in understanding coupling from below and forcing from above","Global wind and temperature measurements in the thermosphere are currently severely lacking. Not only do these winds determine overall variability and climatology in the thermosphere, but thermosphere winds also contribute to gravity wave (GW) filtering, breaking and secondary GW generation in the thermosphere region. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-2163a07083d35d193a6f19c2bc710d68_BossertKatrina.docx"
"208","6 September 2022 9:49:26 pm","Elizabeth","Jensen","0000-0003-0216-6621","Planetary Science Institute","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-5f2c8c5ed074e77ee44db8078e912788_SSPHWhitePaperAuthorInformationFormFixed.xlsx","Basic Research;Space Weather Applications","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Other topic relevant to solar and space physics/heliophysics","","","Other Space Weather","","","","","","Space-based","The Faraday Effect Tracker of Coronal and Heliospheric Structures (FETCH) Instrument","The Faraday Effect Tracker of Coronal and Heliospheric structures (FETCH) instrument, one of ten instruments proposed to be hosted on the MOST mission spacecraft will analyze solar wind CMEs and other disturbances. Through radio propagation, FETCH will obtain plasma magnetic field, density, and variability with Faraday rotation, Total Electron Content, and plasma velocity.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-a4d020dd4153934f93eb439d24d7b950_FETCH_White_Paper_Final.pdf"
"209","6 September 2022 9:52:53 pm","John","Noto","0000-0003-0274-6669","Orion Space Solutions","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-4fa8bdfffc9fbd2efdfd8c03401ef8a4_SSPHWhitePaperAuthorInformationForm-Jnoto.xlsx","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Ground-based","Advancing our understanding of ionospheric structure and variability via TEC measurements from buoys","Discussed here is a new capability that allows the deployment of GPS receivers on ocean buoys, a capability first deployed in 2018. Also discussed in a possible array deployment of receivers in a longitudinal array that will help ameliorate the dearth of data over ocean regions that hinders the comprehensive modeling and characterization of the ionosphere. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-25de918da205a2e722fcb09174242870_NotoJohn.pdf"
"210","6 September 2022 9:54:03 pm","Alexa","Halford","0000-0002-5383-4602","NASA Goddard Space Flight Center","E. J.","Lutz","T. Y.","","","Rigler","Rastaetter","Chen","","","","","","","","[email protected]","[email protected]","[email protected]","","","USGS","NASA/GSFC","Columbia","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","","Data Needs to be...","Findable, Accessible, Interoperable, and Reusable (FAIR) data are essential to heliophysics, indeed all scientific research. We make recommendations intended to prioritize resources needed to satisfy FAIR data principles, treating them as a fundamental research infrastructure, rather than a simple research product.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-5189e0ecd13e25a1e3b0d61ceda84ef3_Final_Data_Needs_to_be.pdf"
"211","6 September 2022 9:58:30 pm","Stephen","Kaeppler","0000-0003-1932-0330","Clemson University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-71e1380d0805644df3d050c35a2fae2e_KaepplerStephenRSSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Enabling Space Science at Mid-latitudes with a Wallops Island Geophysical Observatory","The purpose of this white paper is to motivate a significant expansion of the Wallops Geophysical Observatory to enable next generation studies of the mid-latitude ionosphere-thermosphere.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-5283d590c27f20d3db13ec9ed4b45a52_KaepplerStephenR.pdf"
"212","6 September 2022 10:04:16 pm","Alexa","Halford","0000-0002-5383-4602","NASA Goddard Space Flight Center","Adam","Barbara","","","","Kellerman","Thompson","","","","0000-0002-2315-936X","0000-0001-6952-7343","","","","[email protected]","[email protected]","","","","University of California, Los Angeles","NASA/GSFC","","","","","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","","Using the Application Usability Levels for tracking the health of Heliophysics","Application Usability Levels (AULs) provide a means of tracking the stages of research development. We suggest that funding bodies use the AULs to help track progress of the heliophysics field. The AULs should be used to help inform where new datasets & thus new missions are needed, determine where new funding lines to develop new models, and determine common roadblocks across the community exist.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-071d7d1ea05ec2f463fb163ec8e88b83_HalfordAlexaJ_8.pdf"
"213","6 September 2022 10:04:45 pm","Mitsuo","Oka","0000-0003-2191-1025","University of California Berkeley","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-cd19f1dd7306ee64236343044b3c0be1_Author_Information_Form_for_WP_on_soft_X-ray.xlsx","Basic Research","Solar Physics;Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","","Particle acceleration in solar flares with imaging-spectroscopy in soft X-rays","Magnetic reconnection plays an important role in solar flares, but it remains unclear if or how magnetic reconnection can further explain particle acceleration to high energies during flares. We argue that the key issue is the lack of understanding of the precise context of particle acceleration, and it can be overcome, in the near future, by performing imaging-spectroscopy in soft X-rays (SXRs). ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-bb37c17df51b2cf0f86803cde45b9a5f_OkaMitsuo.pdf"
"214","6 September 2022 10:11:28 pm","Alexa","Halford","0000-0002-5383-4602","NASA Goddard Space Flight Center","Adam","Katherine","Jeffery","Sophie","","Kellerman","Garcia-Sage","Klenzing","Murray","","0000-0002-2315-936X","0000-0001-6398-8755","0000-0001-8321-6074","","","[email protected]","[email protected]","[email protected]","[email protected]","","University of California, Los Angeles","NASA/GSFC","NASA/GSFC","DIAS Dunsink Observatory","","","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","","AUL Development Ecosystem","The Application Usability Level framework has increasingly been adapted to enable communication of a project's progress towards user defined outcomes. It is important to outline the roles enabling these activities. Individuals and groups can play multiple roles in the same and different projects, and funding and acknowledgment/credit must be given for each of the roles.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-748e0881fbe103ce2f0a85ad5545d43e_HalfordAlexaJ_9.pdf"
"215","6 September 2022 10:21:42 pm","Matina","Gkioulidou","0000-0001-9979-2164","Johns Hopkins Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-f1f46bd572a94affe339721578644375_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","PARAGON mission concept: “Seeing” the Global Geospace in Mesoscale Resolution","We present the PARAGON mission concept, which utilizes coordinated: i) unprecedented spatial and temporal resolution imaging of the ring current, plasma sheet, aurora, and plasmasphere and ii) in-situ particle and fields measurements, from different platforms, in order to discover, quantify, and understand the global impact of mesoscale processes in the development of geomagnetic disturbances.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-65218a6f15c7f290119558836bc134af_GkioulidouMatina.pdf"
"216","6 September 2022 10:55:07 pm","Vincent","Ledvina","0000-0003-0127-5105","Predictive Science Inc.","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-42e3d358925c762476a6387a5c95cd53_LedvinaVincentE2.xlsx","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations;Other Space Weather","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","","Agile Collaboration: Citizen Science as a Transdisciplinary Approach to Heliophysics","Citizen science connects scientists with the public to enable discovery, engaging broad audiences across the world. Agile collaboration makes citizen science an asset to heliophysics. Citizen scientists bring expertise from other fields to scientific teams. Citizen scientists are also a bridge between scientists and the public. These attributes form the framework of agile collaboration.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-f4ac6a2ba11e7efa6356542bb04ee3f3_LedvinaVincentE2.pdf"
"217","6 September 2022 11:04:37 pm","David","Schaffner","0000-0002-9180-6565","Bryn Mawr College","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-bb68cfaa653b83fe67672f776c647584_SSPHWhitePaperAuthorInformationForm.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","Just Say Plasma","A white paper submitted to the Solar and Space Science Decadal Survey 2024-2033 on the importance of including the word ""plasma"" in public outreach, news articles and educational material from the solar and space sciences and beyond.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-0cf2c7e0addbd998b9a69f70fcd4a1e0_SchaffnerDavidA.pdf"
"218","6 September 2022 11:21:39 pm","Patrick","Antolin","0000-0003-1529-4681","Northumbria University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-0c84e20e047a151891335d0b540ba3ff_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Solar Physics;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","Cool Multiphase Plasma in Hot Environments","Cool plasmas embedded in a larger, much hotter medium are ubiquitous in different astrophysical systems such as solar & stellar coronae, the CGM, ISM and ICM media. These cross-disciplinary possibilities call for a high-resolution multi-wavelength imaging and spectroscopic solar instrument able to capture the multithermal, dynamic and pervasive nature of the multiphase plasma in the solar corona.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-dbdaea0f8fea0b2ba43086c6f03778a0_AntolinPatrick.pdf"
"219","7 September 2022 12:07:08 am","Jason","Shuster","0000-0001-9425-2281","Department of Astronomy, University of Maryland College Park","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-e1b89be62c0b064b6eaaf949b4fee9b9_SSPH_White_Paper_Author_Information_Form_Vlasov.xlsx","Basic Research","Planetary Magnetospheres;Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","Space-based","Enabling Unprecedented Exploration of Kinetic Plasma Phenomena: Utilizing and Reaching Beyond the MMS FPI Breakthrough","The spectrometer suites onboard NASA's Magnetospheric Multiscale (MMS) mission offered us an unexpected breakthrough in measurement capability that no spacecraft or laboratory experiment has achieved previously: the ingeniously engineered FPI dual ion and electron spectrometers enable direct measurement of terms in the Vlasov equation for the first time in the history of plasma physics research.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-f23387ac84141c9a9a5d3a9351a48ed8_ShusterJasonR.pdf"
"220","7 September 2022 12:13:59 am","Hazel","Bain","0000-0003-2595-3185","CIRES CU Boulder/NOAA Space Weather Prediction Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-3e5ab852ef81f584946657d62a82c160_SSPH_White_Paper_Author_Information_Form_%25281%2529.xlsx","Basic Research;Space Weather Applications","Basic research that is driven by space weather user needs","","","Other Space Weather","","","","","","","Improved Observations and Modeling for Aviation Radiation","In recent years there has been a growing interest from the aviation community for space weather radiation forecasts tailored to the needs of the aviation industry. Due to a lack of routine observations, radiation modeling is required to specify the dose rates experienced by flight crew and passengers. Support for key observational inputs and further modeling advancements are needed. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-52dc2cbf47c660e22e07dd56163487bb_BainHazelM.pdf"
"221","7 September 2022 12:42:26 am","Gary","Swenson","0000-0003-3412-4952","Univ Illinois Urbana-Champaign","Pete","James","Channing","Scott","","Dragic","Clemmons","Philbrick","England","","","0000-0002-5298-5222","0000-0002-4134-3486","0000-0001-5336-0040","","[email protected]","[email protected]","[email protected]","[email protected]","","Univ Illinois Urbana-Champaign","University of New Hampshire","Ball Aerospace, Broomsfield, CO","Virginia Polytechnic and State University","","","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","","","","","","","Space-based","Atmospheric turbulence and the Richardson (Ri) number in the Mesosphere and Lower Thermosphere (MLT)","An ISS mission will 1) use LIDAR to measure the spatial (Equatorial to ±55o) and intra-annual variation of the Ri (parameterized instability) and turbulence in the 85-110 km altitude region, with a special focus on the data void 96-110 km region, enabling 2) model the vertical distribution of minor constituents with vertical transport and photochemical considerations, 85-140 km altitude.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-089a4255423d807adf8488689b77cb47_SwensonGaryR.pdf"
"222","7 September 2022 1:02:55 am","Yihua","Zheng","0000-0002-2569-2950","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-b1b59838b75d8ba08b464a433916d61e_SSPH_WhitePaperAuthorInformationForm.xlsx","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Research to Operations to Research Loop;Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","Space-based","Recommending Low-Cost Compact Space Environment and Space Weather Effects Sensor Suites for NASA Missions","Measurements of how space environment interacts with different space hardware/electronics have been lacking. We recommend developing or procuring low-cost, low-power consumption, and compact sensor suites and flying them on all future NASA (and, more generally, U.S.) missions in order to measure and quantify space weather impacts in addition to the main instrumentation. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-07722f5da5bdfe243452a894f743182b_ZhengYihua.pdf"
"223","7 September 2022 1:12:20 am","Shun-Rong","Zhang","0000-0002-1946-3166","MIT Haystack Observatory","Larisa","Anthea","Ercha","","","Gocharenko","Coster","Aa","","","0000-0001-9031-7439","0000-0001-8980-6550","0000-0002-5228-4119","","","[email protected]","[email protected]","[email protected]","","","MIT Haystack Observatory","MIT Haystack Observatory","MIT Haystack Observatory","","","","Basic Research;Space Weather Applications","Inner Heliosphere and solar wind interaction with unmagnetized bodies;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","Space Weather Research to Operations to Research Loop","","","","","","Ground-based;Space-based","Midlatitude and subauroral region studies: essential for understanding of key atmosphere - ionosphere - thermosphere - magnetosphere dynamic processes","The subauroral and midlatitude upper atmosphere is much more dynamic and complex than anticipated not too long ago. We should emphasize midlatitude and subauroral science in upcoming observation systems, satellite missions, and modeling efforts. We must synchronously push the boundaries of joint ground and space multi-scale instrument networks for high fidelity and wide-field observations. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-8a54b839e2b3a7fa4236dc5434e9571f_WhitePaper_subauroral.pdf"
"224","7 September 2022 1:34:19 am","Junwei","Zhao","0000-0002-6308-872X","W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305-4085, USA","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-e0134c63d66639404897901ff90056ee_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop","","","","","","Space-based","Multi-Vantage Helioseismology","Almost all helioseismology was done using observations along the Sun-Earth line. But the limited field of view limits our capability to investigating the deeper interior of the Sun or the dynamical processes beneath sunspots. One or more missions in the ecliptic plane, with larger separation angles relative to the Sun-Earth line, will help us advance our understanding of the solar interior. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-2971961a6783362c52f977efe27b6b8c_ZhaoJunwei.pdf"
"225","7 September 2022 1:50:08 am","Alexei","Pevtsov","0000-0003-0489-0920","National Solar Observatory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-ef738ba98c9c07092c6d76328f1288a2_SSPH_White_Paper_Author_Information_Form_PevtsovAlexeiA1.xlsx","Basic Research;Space Weather Applications","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","Other Space Weather","","","","","","Space-based","Solar and Heliospheric Magnetism in 5D","We argue for the urgent need for the multi-vantage observations of the Sun and the heliosphere in the framework of six key science objectives. We further emphasize the critical importance of 5D-``space'': three spatial, one temporal, and the magnetic field components. The importance of such observations cannot be overstated both for scientific research and the operational space weather forecast.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-36fae777d777bf095926c0c20b418206_PevtsovAlexeiA1.pdf"
"226","7 September 2022 2:10:57 am","Natchimuthuk","Gopalswamy","0000-0001-5894-9954","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-7e4f849c1c8a5145524d7751f6975224_GopalswamyNat.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","The Multiview Observatory for Solar Terrestrial Science (MOST)","The large-scale MOST mission will measure solar variability in the solar interior, atmosphere, and the interplanetary (IP) medium as part of the next generation Heliophysics System Observatory. MOST is a 4-spacecraft mission located at, and in the vicinity of, Sun-Earth L4 and L5. A novel radio package to measure Faraday rotation in will accompany 6 remote-sensing and 3 in situ instruments.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-180fa565fa0273aa467b1ce09a6b0be8_GopalswamyNat.docx"
"227","7 September 2022 3:13:02 am","Paul","Loto'aniu","","University of Colorado-CIRES","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-39f902812cb8e41db9e34f8156567e14_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Space Weather Applications","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop","","","","","","Space-based","Solar Sail Missions for Sub-L1 Sampling of the Interplanetary Magnetic Field and Plasma on the Sun-Earth Line","NOAA has a research priority to observe solar wind parameters at sub-L1 points along the Sun-Earth line. We present a proposed mission based on the Solar Cruiser architecture that can meet the first step of these research observations using solar sail propulsion technology. The mission will also fly a science payload to observe the solar wind particles and the magnetic field at sub-L1.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-eb95c5192d1c023d3da7c04ad9395459_LotoaniuPaulTM.pdf"
"228","7 September 2022 3:23:49 am","Thomas","Schad","0000-0002-7451-9804","National Solar Observatory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-3c3afb08d65f366c5c3d23b62b0491ee_SSPH_White_Paper_Author_Information_Form___SchadThomasA.xlsx","Basic Research","Solar Physics","","","","","","","","","Ground-based","Resolving 3D Coronal Loop Physics with Spectropolarimetry and Off-limb Solar Adaptive Optics","Novel constraints on coronal magnetism are available through visible and infrared spectropolarimetry. We advocate for investments in the highest resolution spectropolarimetric methods at large-aperture coronagraphic facilities. We identify necessary instrumentation development and the need for off-limb solar adaptive optics supported by technologies similar to the proposed ORCAS mission.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-ecf64332f6857b001e96fcd26f91b7cd_SchadThomasA.pdf"
"229","7 September 2022 3:30:47 am","Enrico","Landi","0000-0002-9325-9884","University of Michigan","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-71a10fc35373b78bad14d12da25d670a_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Space Weather Applications","Solar Physics","","","Other Space Weather","","","","","","Ground-based","Coronal spectral diagnostics: The Coronal Solar Magnetic Observatory (COSMO)","The coronal magnetic field is the main actor in the physics of the solar corona and of activity events generating Space Weather, but our measurements are sporadic, lack accuracy and can't cover the entire corona. We advocate for a ground based instrument (COSMO-LC) capable of measuring at the same time the coronal magnetic field and plasma properties simultaneously over the whole solar corona.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-297af28e3fce5f76c77d5637352bd327_LandiEnrico.pdf"
"232","7 September 2022 4:52:30 am","Steven","Tomczyk","0000-0001-7399-3013","National Center for Atmospheric Research","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-224fad88e7417351762994d99b12efdd_TomczykSteven.xlsx","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","COSMO: The COronal Solar Magnetism Observatory","The COronal Solar Magnetism Observatory (COSMO) will make the first synoptic, simultaneous measurements of magnetic and plasma properties of the global solar atmosphere, filling crucial gaps in our understanding of the drivers of solar eruptions and the evolution of the coronal magnetic field on time scales from minutes to decades.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-811fdb73eb7201b21fb3b5103d03a5d9_TomczykSteven.pdf"
"234","7 September 2022 6:01:04 am","Federico","Fraternale","0000-0002-4700-2762","The University of Alabama in Huntsville, CSPAR","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-9d38d9e210f1caf2b5bc213ef6237ff1_FraternaleFederico_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","","Exploring Turbulence from the Sun to the Local Interstellar Medium","Turbulence plays a fundamental role in the solar wind - LISM interaction and in controlling energetic particle transport and acceleration. Its properties in the outermost regions of the heliosphere are poorly understood. This paper summarizes the open challenges and voices our support for the development of space missions dedicated to the study of turbulence throughout the heliosphere and beyond.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-352ca414d44df0e156402652bf559702_FraternaleFederico.pdf"
"235","7 September 2022 7:51:45 am","Dogacan","Ozturk","0000-0002-8071-2707","University of Alaska Fairbanks","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-a1e2ac7cc6adc6692a7fcc032ab578c4_OzturkDogacanS_authors.xlsx","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Other Space Weather","","","","","","Ground-based;Space-based","The Significance of Magnetospheric Precipitation for the Coupling of Magnetosphere-Ionosphere-Thermosphere Systems: Sources and Properties","Magnetospheric precipitation plays an important role for the coupling of Magnetosphere, Ionosphere, and Thermosphere (M-I-T) systems. In this paper, we detail some of the important open questions regarding the origins of magnetospheric particle precipitation and how precipitation affects ionospheric conductance. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-5eb56c600bf636959554696c7269b042_OzturkDogacanS1.pdf"
"236","7 September 2022 7:51:52 am","Dogacan","Ozturk","0000-0002-8071-2707","University of Alaska Fairbanks","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-e17e8eac641fb17e158677c8e1622491_OzturkDogacanS_authors.xlsx","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Other Space Weather","","","","","","Ground-based;Space-based","The Significance of Magnetospheric Precipitation for the Coupling of Magnetosphere-Ionosphere-Thermosphere Systems: Effects on Ionospheric Conductance","Ionospheric conductance plays a key role in determining how the magnetospheric energy input is dissipated across the Ionosphere-Thermosphere system. In this paper, we detail how the magnetospheric particle precipitation affects the vertical structure of the ionospheric conductivity and provide recommendations to improve its modelling. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-decba8d4daded2717135d6173f0e6de7_OzturkDogacanS2.pdf"
"237","7 September 2022 8:50:41 am","William","Bristow","0000-0002-7845-8631","Pennsylvania State University","Simon G.","J. Michael","Larry","Toshi","Evan","Shepherd","Ruohoniemi","Lyons","Nishimura","Thomas","","","","","","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","Dartmouth College","Virginia Tech","UCLA","Boston University","Dartmouth College","","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Imaging Ionospheric Electric Fields and Conductances at Small-Scales Globally: Advancing Research on Cross-Scale Coupling in the M-I-T System","The paper discusses the current state and future needs for measuring electric fields and conductances in the ionosphere. The main focus is on characterizing these fields across as large a range of scales as possible.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-a024c30ff88715ffa1cb3d2dacc3b745_Imaging_Ionospheric_Electric_Fields_at_Small_Composite.pdf"
"239","7 September 2022 9:56:28 am","Brandon","Burkholder","0000-0001-8702-5806","University of Maryland Baltimore County and NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-a72629563c4e8482ddcd2c18a8bf6861_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Space Weather Applications","Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop","","","","","","","Predictive Space Weather Beyond the Single Spacecraft Solar Wind Monitor","Space weather associated with meso-scale solar wind structures, comparable in size to the magnetosphere, has been largely ignored, as it is the standard to predict the solar wind conditions, based on a single monitor at L1. Future space weather monitoring missions should be adequately equipped to predict the gradients associated with meso-scale solar wind structures, and in advance of L1.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-508d17f5747ef3a54e56c9b767d0faae_Decadal_whitepaper.pdf"
"240","7 September 2022 10:29:06 am","Nada","Al-Haddad","0000-0002-0973-2027","University of New Hampshire","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-c57a719dfb41610a19bc1098e51664f2_SSPH__P0_author_list.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Other Programmatic","","","","On the Need for a Coronal and Inner Heliospheric Panel for the 2024 Heliophysics Decadal Survey","The unique recommendation of this WP is that the 2024 Decadal Survey has a panel specifically dedicated to the Physics of the Upper Corona and Inner Heliosphere, separate from a panel on Solar Physics. A split of the solar--heliosphere research area into two panels (solar physics and the physics of the inner heliosphere) is needed, especially if magnetosphere and ITM are separated into two panels.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-2f0f5da6aa4b292c81be091a1149d77e_AlhaddadNada.pdf"
"241","7 September 2022 10:31:31 am","Yuri","Shprits","0000-0002-9625-0834","GFZ German Research Centre for Geosciences","Drew","Jerry","David","Theodoros","Heidi","Turner","Goldstein","Malaspina","Sarris","Nykyri","0000-0002-2425-7818","0000-0002-6715-7083","0000-0003-1191-1558","0000-0002-0336-2678","0000-0002-6905-9487","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","Johns Hopkins University Applied Physics Laboratory, USA","Division of Space Science and Engineering, Southwest Research Institute, San Antonio, TX, USA","Laboratory for Atmospheric and Space Physics (LASP), University of Colorado, BO, USA","Democritus University of Thrace, Department of Electrical and Computer Engineering, Thrace, GR","Physical Sciences Department, Embry-Riddle Aeronautical University, FL, USA","","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","Ground-based;Space-based","The Need for Increased European-US Collaboration in Heliophysics and Space Weather","Joint work between Europe and the US allows sharing data and expertise on measurements and comparing European and US models of the Heliophysics environment. However, there is a clear need to deepen the trans-Atlantic ties further and develop systems, instruments, and models that can facilitate such collaboration. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-389b62e44a6d03990c29aabbee80ec1d_ShpritsYuriY.pdf"
"242","7 September 2022 11:28:57 am","Larry","Paxton","0000-0002-2597-347X","JHU/APL","Karl","William","Yongliang","Kan","","Hibbitts","Swartz","Zhang","Liou","","0000-0001-9089-4391","0000-0002-9172-7189","0000-0003-4851-1662","0000-0001-5277-7688","","[email protected]","[email protected]","[email protected]","[email protected]","","JHU/APL","JHU/APL","JHU/APL","JHU/APL","","","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Ground-based","Novel Observations of the Aurora (NOA) from New Platforms","We recommend a community-wide effort to develop new sensor capabilities for studying the aurora by RF and optical means. We find that polar 'orbiting' balloons and UAVs offer capabilities that are not available to 'ground-based' instruments. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-ee0661ba7c5dececf68b440eefaa94a0_paxtonlarryj1.pdf"
"243","7 September 2022 11:35:03 am","Robert","Allen","0000-0003-2079-5683","Johns Hopkins Applied Physics Lab","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-91fb51a24c3f6a8467de4937572d608e_SSPH_White_Paper_Author_Information_Form_-_InterMeso.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","Interplanetary Mesoscale Observatory (InterMeso): A mission concept to untangle dynamic mesoscale structures throughout the heliosphere","Mesoscale dynamics are fundamental throughout space physics, but fall within an observational gap of current and planned missions. To address this fundamental gap in our knowledge of the solar wind at these scales, the Interplanetary Mesoscale Observatory (InterMeso) concept employs a multi-point approach using four identical spacecraft in Earth-trailing orbits near 1 au.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-10af5dd366401e835eb0c60d04b178e5_InterMeso_Implementation_FINAL.pdf"
"244","7 September 2022 11:35:52 am","Sarah","Vines","0000-0002-7515-3285","Johns Hopkins University Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-62585bc1f94c5ee375cb49bfb5f4f742_SSPH_White_Paper_Author_Information_Form_Vines_AMPERE_and_Beyond.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","Beyond AMPERE-NEXT: Envisioning the Next System of Global High-Latitude Electrodynamics","As a vital resource to the M-ITM community, we advocate for the uninterrupted continuation and delivery of AMPERE data throughout the next decade, and support for enabling the follow-on iteration post AMPERE-NEXT, including expansion of the program for additional applications and sensors to enable multi-scale coverage and complete specification of high-latitude M-ITM electrodynamics.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-daf2981bcb9b1b962431ceb862bf4538_NextGen_AMPERE_HelioDecadal_WP_submitted.pdf"
"245","7 September 2022 11:38:10 am","Daniel","Seaton","0000-0002-0494-2025","Southwest Research Institute, Boulder, CO","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-b30afc04d15af24a68a611e78afbc657_Middle_Corona_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Solar Physics;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","","A Strategy to Close Key Questions about the Middle Solar Corona During this Decade","We review the middle solar corona, its location and key characteristics, outline important open questions about the region, and provide strategic recommendations for research to close these questions, including prioritizing coordinated broadband spectral observations, prioritizing new radio observations, prioritizing 3D magnetic field observations, and improving data assimilation capabilities.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-95c561c1f44d31ece4678f55b0f33b82_Middle_Corona_White_Paper.pdf"
"246","7 September 2022 11:38:59 am","Robert","Allen","0000-0003-2079-5683","Johns Hopkins Applied Physics Lab","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-c0f152a7e9ddbbf115297adb22eeed54_SSPH_White_Paper_Author_Information_Form_-_Mesoscale_Science.xlsx","Basic Research","Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","","","","","The Solar Wind at Mesoscales – Revealing the Missing Link","To address the fundamental gap in our knowledge of the heliosphere at mesoscales, new dedicated mesoscale missions are required in the next decade. This white paper outlines the current gaps in our understanding resulting from limited measurements at this critical scale and the need for an asserted effort in addressing these gaps.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-e7f128117dcc39ac537753c2abe06319_Mesoscale_SW_Science_FINAL.pdf"
"247","7 September 2022 11:41:45 am","Jeffrey","Brosius","","The Catholic University of America at NASA/GSFC","Peter","James","Therese","Adrian","","Young","Klimchuk","Kucera","Daw","","","","","","","[email protected]","[email protected]","[email protected]","[email protected]","","NASA/GSFC","NASA/GSFC","NASA/GSFC","NASA/GSFC","","","Basic Research","Solar Physics","","","","","","","","","","The Case for Comprehensive Spectroscopic Measurements of the Sun: Understanding Solar Flares and Coronal Heating","We discuss spectroscopic capabilities needed to resolve two important unresolved questions in solar physics, namely, ``What heats the solar corona?"" and ``What causes the sudden, rapid release of energy that produces flares?"" We address (1) spectral resolution; (2) sensitivity & dynamic range; (3) T coverage; (4) absolute wavelength scale; (5) areal coverage; (6) spatial resolution; (7) cadence.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-9d5e7fb4061fab975c85458ffc1f494e_BrosiusJeffreyW.pdf"
"248","7 September 2022 11:44:56 am","Robert","Allen","0000-0003-2079-5683","Johns Hopkins Applied Physics Lab","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-c7bfc2ccc2823b33c6d5554309a068af_SSPH_White_Paper_Author_Information_Form_-_Constellations.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Other topic relevant to solar and space physics/heliophysics","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","The Future of Heliophysics Research through Targeted use of Constellations","This white paper seeks to outline the benefits and challenges of constellations, ranging from the Heliophysics System Observatory, to constellations consisting of a small number of spacecraft, to large-number constellations. In moving toward this constellation era, investments are required by our sponsors to best enable our continued scientific advancement in Solar and Space Physics.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-29709d6d7a467db7b5d20c97fa564285_Helio_Constellations_FINAL.pdf"
"249","7 September 2022 11:59:49 am","Xian","Lu","0000-0002-2535-8151","Department of Physics and Astronomy, Clemson University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-b7dfcc1158756cf476f6726dc9b1fd52_LuXian_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","","","","","","","Space-based","Observing Multi-Scale Ionospheric Structures and Modeling I-T Responses","This white paper addresses the current challenges for a more realistic space weather simulation and solicits observational and modeling requirements.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-bbd877afb9c9e4d0ba26c0e7959ecf08_LuXian.pdf"
"250","7 September 2022 12:14:25 pm","Morris","Cohen","0000-0002-7920-5759","Georgia Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-11c7bfc5ffad65c518a3a67feb55c1df_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Other topic relevant to solar and space physics/heliophysics","","","Space Weather Research to Operations to Research Loop;Other Space Weather","","","","","","","The Impacts of Lightning Beyond the Troposphere","We propose that the upcoming Decadal Survey on Solar and Space Physics describe prominent contributions of lightning and its impacts beyond the troposphere, particularly within the NASA Heliophysics portfolio. We present a brief review of several topics highly relevant to NSF and NASA. We opt to unify these topics into one white paper, with longer reviews/references included.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-e79326e30358f1e9b5d69f07a16ccfba_CohenMorrisB.pdf"
"251","7 September 2022 12:28:35 pm","Teresa","Nieves-Chinchilla","0000-0003-0565-4890","Heliophysics Science Division, NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-f40373f861f5aee2fc04055b1ce263fd_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Space Weather Applications","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Fundamental space plasma theory (not specific to a particular region)","","","Space Weather Pipeline from Research to Application to Operations;Other Space Weather","","","","","","","What is a Heliospheric Flux Rope?","This white paper underlines the lack of fundamental understanding of heliospheric flux ropes and provides the motivation to significantly improve the status quo of flux rope research through novel and requisite approaches. The recommendations put forward in this paper will broaden the in-depth knowledge of our nearest star, its dynamics, and its role in its sphere of influence, the heliosphere.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-d01498f705c07e2da229f46f522dc210_Nieves_Flux_Ropes.pdf"
"252","7 September 2022 12:33:04 pm","Teresa","Nieves-Chinchilla","0000-0003-0565-4890","Heliophysics Science Division, NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-ce4efa097a419ab5a0c1c45dab9d5bfc_Inner_Heliosphere_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","","","","","Where Does the Inner Heliosphere End?","This white paper motivates the need to investigate the spatial and temporal shape of the heliosphere in a more extensive manner. The paper addresses the existing status of fundamental heliospheric research and provides possible future recommendations to advance our understanding of our home, the Sun's atmosphere, and the effect of the Sun's activity on the local space environment","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-422172818c015d8d19ea7601b259ede5_Nieves_Inner_Heliosphere.pdf"
"254","7 September 2022 1:04:49 pm","Gian Luca","Delzanno","0000-0002-7030-2683","Los Alamos National Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-2ec4223cfac7cc52961d4ffbbea5ca9e_Decadal_coauthor_form.xlsx","Basic Research","Planetary Magnetospheres","","","","","","","","","","The Need to Understand the Cold Ion and Cold Electron Populations of the Earth’s Magnetosphere","This white paper advocates for a research program combining the development of new measurement techniques, data analysis, and theory and modeling, culminating with a dedicated space mission, to finally understand the cold particle populations of the Earth's magnetosphere. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-ac4f426ab648ceb82987ce42893a290f_cold_plasma_decadal_white_paper-4.pdf"
"255","7 September 2022 1:06:29 pm","Joel","Allred","0000-0003-4227-6809","NASA/GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-95e59505457a24aefb9fb72a523ef3b0_Next-Generation_Comprehensive_Data-Driven_Models_of_Solar_Eruptive_Events.xlsx","Basic Research","Solar Physics","","","","","","","","","","Next-Generation Comprehensive Data-Driven Models of Solar Eruptive Events","We identify the key components necessary for constructing comprehensive data-driven models of solar eruptive events. Using this modeling framework, long-standing questions regarding how solar eruptive events release energy, accelerate particles, and heat plasma can be explored. We recommend that NASA and NSF provide sufficient funding to enable constructing this modeling framework. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-a8d175a52b5836b620abf6d961febf97_AllredJoelC.pdf"
"256","7 September 2022 1:07:26 pm","Larry","Kepko","0000-0002-4911-8208","NASA GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-d84f26cc1685a1a8a2876f9e199d69c7_MagCon_author_list.xlsx","Basic Research","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","Magnetospheric Constellation (MagCon)","MagCon would study the mesoscale flow of mass, momentum and energy through Earth's magnetosphere using a constellation of 36 identically instrumented spacecraft.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-db4d94eecc04c9c2d7f0dacab7e14871_MagCon_White_paper.pdf"
"257","7 September 2022 1:14:14 pm","Charles","Baldner","0000-0002-2307-0808","Stanford University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-30bb40238558392bfb7fb9e8f4def4b6_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Solar Physics","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","Helioseismology of the solar poles","The ability of helioseismology to address important questions about the structure and dynamics of the solar interior at high latitudes is limited by the ecliptic vantage point of all existing observations. Data sets suitable for helioseismology taken from a polar vantage point would allow significant advances in studying these regions and constraining models of solar activity and magnetism.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-3047acf5d6ae84856a44cff7f5182959_BaldnerCharlesB.pdf"
"258","7 September 2022 1:15:47 pm","Ryan","McGranaghan","https://orcid.org/0000-0002-9605-0007","Orion Space Solutions; NASA/GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-4e07415168a6ea6533426cecd0a5209e_HelioDecadal_WP_Author_Information_-_Complexity_Heliophysics.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","","Complexity Heliophysics: A [new] system science that transcends the previous boundaries of our field","The 21st century is the time of complexity. We describe what this means within Heliophysics. With the right foresight, direction, and incentive over the next ten years, Heliophysics can become a beacon for how all of society thinks about and does complexity science and how methods from complexity science can help us address our 'wicked' scientific challenges. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-30b61cf7421055f6a4769265329003f0_McGranaghanRyanM2.pdf"
"259","7 September 2022 1:30:14 pm","Gareth","Perry","0000-0002-4690-5783","New Jersey Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-761aaf2a90c7e5ecc9b7951b725927f4_GWPerry_Citizen_science_is_a_catalyst_authors.xlsx","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres","","","Other Space Weather","","","","","","","Citizen science is a catalyst for scientific discovery in heliophysics","In this paper, we put forward that citizen science has matured to the point where it will foster discovery in heliophysics in the coming decade and beyond. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-635d1918ffc9759e1d35c8ea78207067_PerryGarethW.pdf"
"260","7 September 2022 1:32:25 pm","Angelos","Vourlidas","0000-0002-8164-5948","JHUAPL","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-3e0ab0d34dae31c48d26167e4e9fe0af_VourlidasAngelos3_WP_Author_Information.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Other Programmatic","","","","Ideas on the NASA Senior Review and Mission Extension Process","Extended mission budgets fund a significant part of our community, particularly young scientists who in a relatively short time are exposed to a broad range of experiences and opportunities. We argue that reducing extended mission operations and science budgets will have a ripple effect across the community, reducing employment and training opportunities and lowering the impact of HSO","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-fecc032ced1e137893e6e4247d661f9a_VourlidasAngelos3.pdf"
"261","7 September 2022 1:33:31 pm","Sanjay","Gosain","0000-0002-5504-6773","National Solar Observatory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-8d06bbc23a54b13f0a9a31ccf42e1ab9_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop;Other Space Weather","","","","","","Ground-based","Ground-based Synoptic Studies of the Sun"," This white paper describes contextual observations from a ground-based network needed to fully exploit this new knowledge of the underlying physics that leads to the magnetic linkages between the heliosphere and the Sun. The combined understanding of small-scale processes and the global context will enable a physics-based approach to Space Weather comparable to Terrestrial Weather forecasting.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-523e13eb5896ec88390f7a93926d8a71_Helio2024_Solar_Synoptic_090422.docx"
"262","7 September 2022 1:37:35 pm","Kathryn","Whitman","0000-0002-3787-1622","KBR","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-340d62a135d69e8c01a2c587b7c81dba_SSPH_Sun_Chaser_White_Paper_Author_Information_Form_Alpha.xlsx","Basic Research;Space Weather Applications","Basic research that is driven by space weather user needs","","","Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","Space-based","Sun CHASER - A Mission to the Earth-Sun Lagrangian Point 4","The SunCHASER (L4) mission concept follows high-energy processes around the west limb, combining solar remote sensing & in situ, overseeing the solar radiation hemisphere. It is essential for solar particle event and all-clear forecasting. SunCHASER+ includes L5, providing 240° longitude coverage of photospheric B field, active region magnetic field diagnostics, and continuous view of both poles.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-eb7167bf751c74590ff74ee46190bc90_KathrynWhitman2.docx"
"263","7 September 2022 1:37:47 pm","Lindsay","Goodwin","0000-0001-5302-7889","New Jersey Institute of Technology","Theodoros","Brian","","","","Sarris","Harding","","","","0000-0002-0336-2678","0000-0002-1293-9379","","","","[email protected]","[email protected]","","","","Democritus University of Thrace","University of California, Berkeley","","","","","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres;Fundamental space plasma theory (not specific to a particular region)","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Resolving the O+-O Cross-Section and its Impact on the Upper Atmosphere","O+ velocity distribution distortions are a known result of O+-O collisions, yet the cross-section between these species (and thus the momentum transfer collision frequency) is not known. This white paper calls for an examination of the O+-O collision cross-section and the collision frequency vertical profile using ground-based and space-based (e.g. GDC, DYNAMIC, Daedalus, ASTRE) instrumentation.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-03437461c5d2916b8a98822024830b6d_GoodwinLindsayV1.pdf"
"265","7 September 2022 1:59:43 pm","Luca","Bertello","0000-0002-1155-7141","National Solar Observatory, Boulder, Colorado","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-fffca4e1cb9234745e7293a0112fb739_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Ground-based","MULTI-HEIGHT MEASUREMENTS OF THE SOLAR VECTOR MAGNETIC FIELD","This white paper advocates the importance of multi-height measurements of the vector magnetic field in the solar atmosphere. These measurements are critical for addressing some of the most fundamental questions in solar and heliospheric physics today. They constitute also the primary product for space weather operations, research, and modeling.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-d698a602742eb50892ead55d4b8b7c3d_BertelloLuca.pdf"
"267","7 September 2022 2:02:52 pm","Larry","Kepko","0000-0002-4911-8208","NASA GSFC","Nicholeen","","","","","Viall","","","","","0000-0003-1692-1704","","","","","[email protected]","","","","","NASA GSFC","","","","","","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Fundamental space plasma theory (not specific to a particular region)","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","Mesoscale dynamics – the key to unlocking the universal physics of multiscale feedback","The undersampled mesoscale regime is crucial to study and we believe could be a unifying focus of heliospheric research in the coming decades. Making progress over the coming decades requires a new approach, enabled by advancements in measurement technology and computational power. We suggest 3 initiatives.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-89a2d80fc23d7e21343882fc23d80f11_Mesoscale_dynamics.pdf"
"269","7 September 2022 2:12:59 pm","Phillip","Chamberlin","0000-0003-4372-7405","U. of Colorado, Laboratory for Atmospheric and Space Physics","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-2429b5e562b8fab06ff0ef99ea65aa79_ChamberlinPhillipC1_Author_Information_Form.xlsx","Basic Research","Solar Physics","","","","","","","","","Space-based","The Next Decade of Solar Ultraviolet Spectral Irradiance – Continuity, Modeling, and Physics","Solar spectral irradiance (SSI) has demonstrated a wide range of science advances spanning all NASA Science Disciplines. Additional measurements of solar spectral variability are needed to be made over the coming decade to continue to drive advances. The problem is that there are now significant 'holes' in the solar UV spectral irradiance coverage that is not currently measured or planed to be.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-ff3bd70a2f944fb212603b66ac4cc170_ChamberlinPhillipC1.pdf"
"270","7 September 2022 2:20:11 pm","Alexei","Pevtsov","0000-0003-0489-0920","National Solar Observatory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-2781d6dd79304d74449a9bf65b71adf9_SSPH_White_Paper_Author_Information_Form_PevtsovAlexeiA2.xlsx","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Other Space Weather","","","","","","Ground-based","ngGONG -- Future Ground-based Facilities for Research in Heliophysics and Space Weather Operational Forecast","We advocate for the development of a ground-based network of instruments provisionally called ngGONG to maintain critical observing capabilities for synoptic research in solar physics and for the operational space weather forecast.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-698547ed17542925c7986cb034cd9946_PevtsovAlexeiA2.pdf"
"271","7 September 2022 2:29:48 pm","Susan","Nossal","0000-0002-8398-6439","Physics Department, University of Wisconsin-Madison","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-75a986342690b73a29dbf68bf4fbd3b8_SSPH_White_Paper_Author_Information_Form_NossalSusanM.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Other topic relevant to solar and space physics/heliophysics","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Other Programmatic","","","Ground-based;Space-based","Heliophysics Science Community Contributions to Addressing Climate Change","There are now models that span the surface through the upper thermosphere and aeronomy datasets that span multiple decades. These studies indicate that the middle and upper atmosphere provide multiple vertical footprints for climate change. This white paper outlines recommendations for ways that the heliophysics community might further contribute to global efforts to address climate change.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-222e6ba6c96782eddeb27e7717cb2269_NossalSusanM.pdf"
"272","7 September 2022 2:33:05 pm","Sijie","Yu","0000-0003-2872-2614","New Jersey Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-43ee0e55442b181525bc5c4a6f3f6d73_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Ground-based","Long-Lasting Solar Coherent Radio Bursts and Implications for Solar–Stellar Connection","This white paper motivates open questions in long-lasting solar coherent radio bursts. The answers to these questions would not only advance our understanding of the fundamental physical processes of coherent radio emission on the Sun but also have broad implications for (sub)stellar physics and magnetic ecosystem in the worlds beyond the solar system.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-b91a85c4ee94051c139a98faa3aca5da_YuSijie.pdf"
"273","7 September 2022 2:36:13 pm","Kyoung-Joo","Hwang","0000-0001-9583-8882","Southwest Research Institute, San Antonio, TX","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-d2d80f0067ff5df7ccb774bd2bfb3309_SSPHWhitePaperAuthorInformationForm_Hwang.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","FLANK MAGNETOSPHERE: DYNAMICS AND TURBULENT PATHWAY TO/FROM THE MAGNETOTAIL","We resolve the long-standing Dungey vs. Axford-Hines dichotomy via simultaneous measurements of dayside reconnection (2 polar-orbiters) and flank-side process (2 equator-orbiters at dawn and dusk flanks). Another equator-orbiter probing the near-midnight plasma sheet, for the first time, enables us to address causality between unstable central magnetotail current sheets and flank-side dynamics.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-b77656691f90a3ccb9834d8777412591_HwangKyoung-Joo.pdf"
"274","7 September 2022 2:36:49 pm","Shea","Hess Webber","0000-0002-3631-6491","Stanford University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-d2ead0665da904173176e3ee1bfc460d_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Solar Physics;Other topic relevant to solar and space physics/heliophysics","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","You Get What You Pay for: Scientific Engineering Challenges for Successful Distributed Multi-Satellite Missions in Solar and Heliophysics","Any multi-satellite program will need to address the technical challenges of communication, coordination, calibration, and standardized data access in order to ensure the scientific success of much needed solar-viewing constellation missions in the next decade and beyond. Existing technological advancements must be leveraged for integration into any constellation heliospheric mission.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-1bd76c4394a229de9a768b6fe20c0bd0_HessWebberSheaA.pdf"
"275","7 September 2022 3:11:54 pm","Larry","Kepko","0000-0002-4911-8208","NASA GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-97fd05d3349992348824c0b1719d1779_ISTPNext_Authors.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","ISTPNext","The next era of Heliophysics should focus on the Sun-Heliosphere and Geospace as system-of-systems. We recommend a coordinated, deliberate, worldwide scientific effort to answer long-standing questions that will remain unanswered without a unified program. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-6f16a4a5f0e1beb8e1ebc7fdfacf0f2e_ISTPNext_submitted.pdf"
"276","7 September 2022 2:44:43 pm","Larry","Paxton","0000-0002-2597-347X","JHU/APL","Mary","","","","","Keller","","","","","0000-0003-0669-1298","","","","","[email protected]","","","","","JHU/APL","","","","","","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","Ground-based","GNSS (and other) Observations from Autonomous Seagoing Platforms","Much of the surface of the Earth is available for placing scientific instruments, however this is the open ocean. We suggest that sailing drones, capable of operating autonomously for significant amounts of time off exciting options for providing data to characterize the ionosphere/thermosphere/mesosphere. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-c55e50870bef94a23f746424de5009a0_paxtonlarryj2.pdf"
"277","7 September 2022 2:46:14 pm","Dale","Gary","0000-0003-2520-8396","New Jersey Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-a804759539a2b874061429a1489ff82a_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics","","","","","","","","","Ground-based","Frequency Agile Solar Radiotelescope","The Frequency Agile Solar Radiotelescope (FASR) is a radio spectroscopic imager addressing all of solar science. It has been strongly endorsed as a top community priority by both Astronomy & Astrophysics Decadal Surveys and Solar & Space Physics Decadal Surveys in the past two decades. The community must seize this opportunity to modernize the FASR design and build the instrument in this decade.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-1f4d2fb9daa4d61b515d4781a45048bb_2024_SSP_Decadal_WP___Frequency_Agile_Solar_Radiotelescope.pdf"
"278","7 September 2022 2:58:38 pm","Yaireska","Collado-Vega","0000-0003-3396-196X","NASA GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-5ae9cea2641ee3c205602a4a0bfb9d94_SSPH_White_Paper_Author_Information_Form_ColladoVega.xlsx","Space Weather Applications","","","","Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","Space-based","Space Weather Operations and the need for Multiple Solar Observational Vantage Points","The current operational dimension available for space weather analysis and operations is not suitable for deep space exploration. The initial step is to establish multiple observational points that will improve the current analysis/modeling capabilities. We summarize the value of multiple observational points, outline the current gaps, and propose ideas for missions that will address these gaps. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-bcec0a2d92c8319552f98c3c1d2281bd_ColladoVegaYaireskaM.docx"
"279","7 September 2022 3:00:31 pm","Dale","Gary","0000-0003-2520-8396","New Jersey Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-2c4645a1fb35c664f67f71a2f7037b20_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics","","","","","","","","","","Solar Active Region Coronal Magnetic Fields","Diagnostics of coronal and chromospheric magnetic fields have recently been developed that must be exploited in the next decade, including ultra-broadband radio imaging spectropolarimetry. To capitalize on these developments requires the superior broadband microwave imaging for which the Frequency Agile Solar Radiotelescope (FASR) has been strongly endorsed by several past decadal surveys.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-3e954ced821e01ccb08c86f4ceb1c38f_2024_SSP_Decadal_WP___Active_Region_Gyroresonance.pdf"
"280","7 September 2022 3:01:51 pm","Christopher","Pankratz","0000-0002-4022-8080","University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics (LASP)","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-31a578898c6c5af115edfc15d09f2264_SSPH_White_Paper_Author_Information_Form.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Collaborative and Open-Source Science Data Systems","Recommendations for enabling and evolving toward a community-driven, open-source, modular, flexible framework to quickly deploy mission science data systems.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-8861cb85f6cdf0f9b667ad3ab7282030_PankratzChristopherK.docx"
"281","7 September 2022 3:03:19 pm","Martin","Mlynczak","0000-0002-7578-1003","NASA Langley Research Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-7f8023699246ca825e846afc29113b71_MlynczakMartinG.xlsx","Basic Research","Planetary ionospheres/upper atmospheres;Other topic relevant to solar and space physics/heliophysics","","","","","","","","","Space-based","How is Geospace Changing? Architecture and Measurement Considerations for Continuity of Observations of the Geospace Environment","How is Geospace changing? This fundamental scientific question is motivated by the need to understand the effects of increasing carbon dioxide and ongoing solar variability on the Geospace environment. This White Paper describes the architecture considerations for an observing system to accurately measure trends and changes in Geospace to inform future societal, economic, & policy decisions.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-67c903920137a7fdcebb28af631e6cf6_MlynczakMartinG.pdf"
"282","7 September 2022 3:04:58 pm","Sebastijan","Mrak","0000-0002-3925-760X","University of Colorado Boulder","Anthea","Keith","Romina","","","Coster","Groves","Nikoukar","","","0000-0001-8980-6550","0000-0002-2067-1579","0000-0002-8608-2822","","","[email protected]","[email protected]","[email protected]","","","Haystack Observatory Massachusetts Institute of Technology","Institute for Scientific Research, Boston College","Johns Hopkins Applied Physics Laboratory","","","","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Ground-based infrastructure for observing and characterizing GNSS scintillation-producing ionospheric irregularities at mid-latitudes","We discuss the potential science investigations at mid-latitudes enabled by a modern, space-weather-grade, ground-based Radio-Frequency network of scintillation receivers including GNSS, Beacon receivers, coherent radars, and leveraging radio astronomy infrastructure. We review the current state of knowledge and propose a plan for infrastructure that will enable novel scientific investigations.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-11783ea271f8a029fb5dfc456ad1bd37_MrakSebastijan.pdf"
"283","7 September 2022 3:08:48 pm","Nicholeen","Viall","0000-0003-1692-1704","NASA Goddard Space Flight Center","Joseph","Aleida","Angelos","Samantha","","Borovsky","Higginson","Vourlidas","Wallace","","0000-0002-2325-3348","0000-0003-1380-8722","0000-0002-8164-5948","0000-0002-1091-4688","","[email protected]","[email protected]","[email protected]","[email protected]","","Center for Space Plasma Physics, Space Science Institute","NASA Goddard Space Flight Center","Johns Hopkins University, Applied Space Physics Laboratory","NASA Goddard Space Flight Center, NASA Postdoctoral Program","","","Basic Research","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","","","","","On Solving the Outstanding Questions in Solar Wind Physics","The Sun and the heliosphere is a system-of-systems, where the physics of cross-regional and cross-scale coupling determines the state of the system. We describe the outstanding questions of solar wind physics as well as potential solutions, including the need for coordinated observations, modeling, and data architecture under an umbrella program such as ISTPNext. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-58d9d82af95241fb11319009092ece0a_Decadal_WP_solar_wind_Viall.pdf"
"284","7 September 2022 3:12:16 pm","Gordon","Petrie","0000-0001-8462-9161","National Solar Observatory","Andrew","Valentin","Alexei","Pete","","Marble","Martinez Pillet","Pevtsov","Riley","","","0000-0001-7764-6895","0000-0003-0489-0920","0000-0002-1859-456X","","[email protected]","[email protected]","[email protected]","[email protected]","","CIRES, CU Boulder & NOAA SWPC","National Solar Observatory","National Solar Observatory","Predictive Science Inc.","","","Basic Research;Space Weather Applications","Solar Physics","","","Space Weather Research to Operations to Research Loop","","","","","","Ground-based","Improving Solar Polar Field Observations from the Ground","The Sun's polar fields have global influence over coronal/heliospheric structure, and are believed to seed activity cycles. However, they are difficult to measure from (near) Earth because (1) they are weak overall, and (2) the viewing angle is large. Full-Stokes spectro-polarimetry for the polar fields is a photon-starved problem that we must address with large-aperture telescopes on the ground.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-714df24aa8f5ca29b29f3e44c45b2321_PetrieGordonJD.pdf"
"285","7 September 2022 3:14:40 pm","larry","paxton","0000-0002-2597-347X","jhu/apl","douglas","yongliang","","","","rowland","zhang","","","","0000-0003-0948-6257","0000-0003-4851-1662","","","","[email protected]","[email protected]","","","","nasa","jhu/apl","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-451d76ff817cfe3dea97a002e8904ab0_paxtonlarryj4.pdf","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Space-based","Ion Outflow Measurements via Optical Techniques","We seek an understanding of the processes that shape the evolution of planetary atmospheres as well as those processes that determine how the solar wind interacts with that planet. Ion outflow is a challenging phenomenon to quantify but there are many simple optical techniques that can be used from LEO and GEO to image the extended corona of neutrals and ions around the Earth.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-ccaae7fe7c4ba06e82c97603b2c53c5a_paxtonlarryj4.pdf"
"286","7 September 2022 3:15:12 pm","Dale","Gary","0000-0003-2520-8396","New Jersey Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-51c3e959db57ad48178cbb3594da6325_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics","","","","","","","","","","Particle Acceleration and Transport: New Perspectives from Radio, Optical, X-ray, and γ-Ray Observations","The transformative technique of ultra-broadband radio imaging spectroscopy is discussed, which serves as the observational basis for new insights into particle acceleration and transport. These include the dynamic measurement of coronal magnetic fields, the measurement of the spatiotemporal evolution of the electron distribution function, and the observation of flares and CMEs as coupled systems. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-b7a8f98a8a324e7e8ca54121841cf5df_2024_SSP_Decadal_WP___Particle_Acceleration___Transport.pdf"
"287","7 September 2022 3:17:11 pm","Kate","Zawdie","0000-0001-7192-4356","Naval Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-92668ee656f7b4baa27d16e199924af6_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","","Impacts of Neutral Atmospheric Waves on the Ionosphere","The purpose of this white paper is to outline additional studies and observations that are required in the coming decade to improve our understanding of the impact of neutral atmospheric waves on the ionosphere, as the circumstances under which they generate ionospheric disturbances and seed plasma instabilities are not well understood. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-7f0ac01f9271aa5d16a5c7d6b421f8fc_ZawdieKateA.pdf"
"288","7 September 2022 3:20:28 pm","Sasha","Ukhorskiy","0000-0002-3326-4024","JHU APL","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-ca57c078358fc8f4b6d494935a3083e2_SSPHWhitePaperAuthorInformationForm.xlsx","Space Weather Applications","","","","Space Weather Pipeline from Research to Application to Operations;Other Space Weather","","","","","","","Radiation Belt Space Weather: From Basic Research to Operations","Relativistic electrons and highly penetrating ion radiation can cause substantial economic impact and are hazardous for astronauts in space. Protecting the nation's infrastructure from adverse particle radiation effects requires a community-wide systems solution employing a distributed spacecraft constellation, capable ground-based operations, and comprehensive data-driven modeling infrastructure.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-a71fba1256f5fde57834ad563002bdb9_UkhorskiySasha.pdf"
"289","7 September 2022 3:18:52 pm","Kenneth","Arnett","0000-0002-7572-8034","Perdix, Inc.","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-48b31a064e871de186a788aef8a21799_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Space-based","Using Far-Infrared Emissions to Understand the Thermosphere","The thermosphere is largely composed of neutral atomic oxygen (O). Continuous O density monitoring using a constellation of CubeSats will provide real-time data for atmospheric heating/cooling models in addition to providing a means to accurately determine drag on constellations of low-earth-orbiting communications satellites. This data is fundamental to space weather prediction agencies. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-391e25bf27a2147e1c35e604dae7ad22_ArnettKennethE.pdf"
"290","7 September 2022 3:31:29 pm","Claudio","Corti","0000-0001-9127-7133","NASA/GSFC CCMC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-8f5a6625cdac4b1e2f2b7637571740c8_CisLunar_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Basic research that is driven by space weather user needs;Other topic relevant to solar and space physics/heliophysics","","","","","","","","","Space-based","Galactic Cosmic Rays and Solar Energetic Particles in Cis-Lunar Space","The particle and radiation environment in cis-lunar space is becoming more important as space exploration efforts turn to the Moon and beyond. This paper highlights gaps in energetic particle measurements. We recommend key observations near Earth and distributed measurements in the heliosphere, magnetosphere, and lunar surface to improve the scientific understanding of these particle populations.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-6d260f9a2dab70be35e7ee7ebc68c83b_Cis-Lunar_GCR_SEP_WhitePaper.pdf"
"291","7 September 2022 3:21:23 pm","Kerry","Nock","","Global Aerospace Corporation","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-8e946820a320ba428b5cb1d97db51b2f_GAC2_SSPHWhitePaperAuthorInformationForm.xlsx","Space Weather Applications","","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Space-based","Neutral Atmosphere Density Monitoring System","The conceptual design, scientific rationale and relevance, and technology and programmatic needs of a neutral atmosphere density monitoring system are explored that could monitor atmospheric density in low Earth orbit (LEO) which varies in response to changes in solar activity and Earth's geomagnetic conditions.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-53c5e534e649ff52cd2a25602ecb49cb_GAC_NADMS_White_Paper_v7.pdf"
"292","7 September 2022 3:21:27 pm","Larry","Kepko","0000-0002-4911-8208","NASA GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-ba4e198cbdf8f6465bae2201c8d2e631_geospace_systems.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","","Geospace as a system-of-systems: An orchestrated strategy and roadmap for scientific advancement and discovery in upcoming decades","Magnetospheric physics lacks a cohesive international scientific framework. To make substantial progress during the next decades, we suggest a coordinated, worldwide effort, which we call the International Geospace Systems Program (IGSP), to study Geospace as a system of systems, with particular emphasis on resolving mesoscale dynamics, where significant science questions remain.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-adb5038c0acc1fe39b07212ecd942d46_Geospace_as_a_system_submited.pdf"
"293","7 September 2022 3:23:29 pm","Benjamin","Chandran","0000-0003-4177-3328","University of New Hampshire","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-a23b36e64972312a67773661da8a206e_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Basic research that is driven by space weather user needs","","","","","","","","","Space-based","How Firefly Would Advance Our Understanding of the Solar Wind","The proposed Firefly mission would provide nearly continuous 4pi-steradian measurements of the magnetic field on the solar photosphere, as well as in situ measurements of the high-heliolatitude solar wind. These new observational capabilities would lead to significant advances in our understanding of the solar wind. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-7a56e04ed9b8fd12226af4e1b42381aa_white_paper_Firefly.pdf"
"294","7 September 2022 3:24:04 pm","Mark","Adrian","0000-0002-0932-8403","Auburn University","Conrad","Damon","Sean","Shing","Yu","Schiff","Bradley","Letourneau","Fung","Lin","0000-0003-3923-8326","0000-0002-4305-889X","0000-0002-7392-8550","0000-0002-1216-5553","0000-0001-8003-9252","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","NASA/GSFC","DeepSpace Technologies","KBR Wyle Services LLC","NASA/GSFC","Auburn University","","Basic Research","Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","The Challenges of Determining the Distribution of Cosmic, Heliospheric and Interplanetary Dust within the Heliosphere","The studies envisioned herein seek to fill these voids in our knowledge of heliospheric dust, as well as lay the foundations for a mission specifically designed to study the distribution micron-sized dust near the ecliptic plane of the inner heliosphere.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-48147d774d37abbbde0cf2ce829387c0_The_Challenges_of_Determining_the_Distribution_of_Cosmic%252C_Heliospheric_and_Interplanetary_Dust_within_the_Heliosphere_D2022250.pdf"
"296","7 September 2022 3:27:46 pm","George","Ho","0000-0003-1093-2066","Johns Hopkins Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-e425b0037378cc2208da8e0e4b3264fc_SSPH_White_Paper_Prespectives_on_NASA_Heliophysics_Mission_Program_for_Addressing_System_Investigations.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Other Programmatic","","","Space-based","Perspectives on a NASA Heliophysics Mission Program for Addressing System Investigations","As the heliophysics science matures through previous targeted measurements provided by focused investigations, there is a need to have a new strategic mission line to study complex relationships throughout our Sun and geospace systems. This is the so-called ""system of systems"" architecture that can close the link between the Sun and and the responses of the coupled system.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-69bf49895f94471e7dcb53ea7615a012_Prespectives_on_NASA_Heliosphysics_Mission_Program_for_Addressing_System_Investigations.pdf"
"297","7 September 2022 3:32:23 pm","Albert","Shih","0000-0001-6874-2594","NASA Goddard Space Flight Center","Amir","Jessie","Lindsay","Silvina","Katharine","Caspi","Duncan","Glesener","Guidoni","Reeves","0000-0001-8702-8273","0000-0002-6872-4406","0000-0001-7092-2703","0000-0003-1439-4218","0000-0002-6903-6832","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","Southwest Research Institute","NASA Postdoctoral Program / NASA GSFC","University of Minnesota","American University / NASA GSFC","Center for Astrophysics | Harvard & Smithsonian","","Basic Research;Infrastructure, Workforce, Other Programmatic","Solar Physics;Basic research that is driven by space weather user needs","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","Sustaining high-solar-activity research","Research efforts that require observations of high solar activity, such as multiwavelength studies of large solar flares and CMEs, must contend with the 11-year solar cycle to a degree unparalleled by other segments of heliophysics. We recommend the development of a strategic program that ensures optimal science return for each solar maximum while sustaining the research community between maxima.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-32f96bcd8f9a873176487a6a6dd1c0b3_ShihAlbertY1.pdf"
"298","7 September 2022 3:33:53 pm","Dibyendu","Nandy","0000-0001-5205-2302","Center of Excellence in Space Sciences India, Indian Institute of Science Education and Research Kolkata, Mohanpur 741246, West Bengal, India","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-c191a8b9225741af394d7c9a422dbbab_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","Space-based","EXPLORING THE SOLAR POLES: THE LAST GREAT FRONTIER OF THE SUN","Observations of the Sun's poles is fundamental to understanding and predicting the solar cycle, constraining polar kilo-Gauss flux patches and plasma jets and illuminating the origin of the fast solar wind. This white paper argues the case for novel out-of-ecliptic observations of the Sun's polar region in conjunction with existing or future multi-vantage point heliospheric observatories.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-e68e0ae8d0df6dabd6e28abe775d0b84_NandyDibyendu.pdf"
"299","7 September 2022 3:39:42 pm","Kathleen","Mandt","0000-0001-8397-3315","Johns Hopkins Applied Physics Laboratory","See page 1","","","","","","","","","","","","","","","","","","","","","","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","Advancing Space Science Requires NASA Support for Coordination Between the Science Mission Directorate Communities","There is a growing awareness within the space science community that cross-disciplinary studies will make the greatest advances toward many major scientific objectives. This requires coordination and collaboration between the communities represented by the NASA SMD Divisions . We outline here specific steps that NASA and the community can take to further cross-disciplinary research. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-579f6f2f4cea3c2992ad2ea2ed63a0d9_Mandt_et_al_CrossDivision_WP_helio.pdf"
"300","7 September 2022 3:42:15 pm","Mark","Conde","https://orcid.org/0000-0003-4924-878X","Geophysical Institute, University of Alaska Fairbanks","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-d2ca8f758f596202e0b6a2d07e0211c5_SSPHWhitePaperAuthorInformationForm_conde.xlsx","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Ground-based","The Need for a Large-Scale Dense Array of Ground Based Observatories to Monitor Thermospheric and Space Weather","We recommend establishing a large array of ground-based observatories for monitoring weather in Earth's mesosphere, thermospere, and ionsphere. These would be deployed from the Canadian Arctic down through the Americas to southern Argentina. Observatory instruments would characterize winds, temperatures and electrodynamics above ~80 km altitude, as well as the drivers that force these fields.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-3b0b53cc5a880c1747b9488d2dec032f_CondeMarkG1.pdf"
"301","7 September 2022 3:45:42 pm","Adam","Kobelski","0000-0002-4691-1729","NASA Marshall Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-4a4961861661f54e496d3392ae830270_SSPHWhitePaperAuthorInformationForm_QS_Kobelski.xlsx","Basic Research","Solar Physics;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Ground-based;Space-based","Radio Observations of the Quiet Chromosphere and Corona","Identification of the mechanisms responsible for heating the solar atmosphere remains an outstanding problem. There has been tremendous progress in the past decade. Despite this progress, gaps remain. With dynamic broadband imaging spectropolarimetry, radio observations enable key diagnostics of the solar atmosphere. We briefly discuss the need for radio coverage and discuss the requirements. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-89cd944e5428c1294c02016c6bcaaa20_2024_SSP_Decadal_WP___Radio_Quiet_Sun.pdf"
"302","7 September 2022 3:47:48 pm","Harald","Kucharek","0000-0003-3718-5312","University of New Hampshire","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-3a6336eaed06504ee09498cd34fa554e_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","Space-based","Thermal and Suprathermal Particles: A Prime Science Targets for an Interstellar Probe Mission.","This paper should highlight criticality and importance of proper thermal and suprathermal instrumentation of the Interstellar Probe mission to fill these gaps and complete our understanding of particle acceleration in the heliosphere and beyond.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-504366e32151048af0d391945c0f801e_HaraldKuharek.pdf"
"304","7 September 2022 3:49:39 pm","Slava","Turyshev","0000-0003-4255-9497","JPL","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-01af02c1b14ebee15ede675835957b56_Turyshev-SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","","","","Space-based","The Heliosphere From Top to Bottom: Close Out of the Ecliptic Solar Orbiter Now and Then Beyond the Heliopause","With solar sailing propulsion capable of reaching the velocities of ~5-10AU/year, missions to the Jovian system would take 2 years, and missions to Saturn, 3. Fast, low-cost, maneuverable sailcraft open new opportunities for solar system exploration. Missions may cost only a few tens of millions of dollars and could be modularized to reach different destinations with different instruments. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-912cc20d928a622a2f2ab1899e82dc0e_TuryshevSlavaG.pdf"
"305","7 September 2022 3:52:38 pm","Martin","Laming","0000-0002-3362-7040","Naval Research Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-fa33bc62534e6f4471fb54074c50f345_SSPHWhitePaper_FIP.xlsx","Basic Research","Solar Physics;Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","Space-based","Element Fractionation by the Ponderomotive Force","We describe a qualitatively new effect recently identified in solar physics and astrophysics, that of ion-neutral separation in the chromosphere caused by the ponderomotive force associated with Alfven and fast mode waves. We argue that these abundance anomalies are a promising route to understanding solar atmospheric waves, and hence many facets of solar activity and plasma energization.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-cbc7a55084baef90753d67c336965f56_LamingJMartin.pdf"
"306","7 September 2022 3:54:08 pm","Fan","Guo","0000-0003-4315-3755","Los Alamos National Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-8b836764497cb765d7ab52200876950d_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Fundamental space plasma theory (not specific to a particular region);Basic research that is driven by space weather user needs","","","","","","","","","","Advancing Theory and Modeling Efforts in Heliophysics","Theory and modeling build fundamental understanding and constitute a comprehensive scientific program in heliophysics. As observations analysis become increasingly detailed, it is critical that theory and modeling develop more quantitative predictions. We recommend that enhanced support to expand and create theory and modeling programs to ensure the development of heliophysics research.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-3acb077d57c696674c6d7235cae2bfa1_GuoFan.pdf"
"307","7 September 2022 4:02:54 pm","Phillip","Chamberlin","0000-0003-4372-7405","U. of Colorado, Laboratory for Atmospheric and Space Physics","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-5c06567cdbaf58c9515bc697adc27cc9_ChamberlinPhillipC2_Author_Submission_Form.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Other topic relevant to solar and space physics/heliophysics","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","The Next Decade of Sounding Rockets that will lead the next 40 years of NASA Heliophysics missions","Sounding Rockets have been a critical part of NASA's assets to explore space, even predating the creation of the NASA organization. To this day, they remain the premier testbed for new science and technology payloads that can lead to future missions.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-a16ecfe4aac510b4e6f767520ea1336d_ChamberlinPhillipC2.pdf"
"308","7 September 2022 4:03:57 pm","Larry","Kepko","0000-0002-4911-8208","NASA GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-fd18be6340c5d1d66185e63520bad9d0_helioprobes_authors.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Heliophysics Needs a Mission Element between MIDEX and Flagship","Heliophysics has entered an era in which the nature of our science questions has outpaced the ability of our mission opportunities to adequately address them. We argue that our discipline needs a new PI-led mission element, called HelioProbes, with a ~$500M - $1B (FY22) cost cap that would fill the capability gap between MIDEX ($250M, FY20) and Flagship (~>$1B)","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-ff99816454e417fd2d92c0f7d236a912_Helioprobes_submitted.pdf"
"309","7 September 2022 4:04:34 pm","Andrew","Poppe","0000-0001-8137-8176","Space Sciences Laboratory, University of California at Berkeley","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-aadd71081f9d558471d4fa6e8574d729_PoppeAndrewR_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Outer Heliosphere;Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","","The Interactions of Interstellar Dust with our Heliosphere","We describe compelling open scientific questions and research areas regarding interstellar dust (ISD) grains and their interactions with the heliosphere. Primary open questions include the physical characteristics of ISD, ISD dynamics throughout the heliosphere, and the impacts of ISD on heliospheric structures and composition. Recommendations for future multi-point ISD observations are made.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-1f0c2e8511fbae098d37577d39ccddcc_PoppeAndrewR.pdf"
"310","7 September 2022 4:11:16 pm","Matthew","Cooper","0000-0001-6137-8814","New Jersey Institute of Technology-Center for Solar-Terrestrial Research","Jerry","Thomas","","","","Manweiler","Chen","","","","0000-0002-8800-2128","0000-0002-0294-3614","","","","[email protected]","[email protected]","","","","Fundamental Technologies, LLC","Columbia University","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","Towards Terahertz Communications Systems for Satellites","A white paper outlining a possible route to innovation and technological advancement of terahertz communications systems for on-orbit satellites which would enable data rates well beyond what is current available. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-da59f2fd4e137d4e5d5de6e80d46480f_CooperMatthewB.docx"
"311","7 September 2022 4:20:49 pm","Katherine","Garcia-Sage","0000-0001-6398-8755","NASA/GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-592e52c59bda95d13cadf40282291fbf_Exoplanets-SSPH_Author_Information_Form.xlsx","Basic Research","Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","","Expanding Heliophysics to Engage in Interdisciplinary Star-Planet Interactions Studies","Exoplanetary research enriches heliophysics with an understanding of universal processes that operate in diverse environments. Heliophysics of exoplanetary systems should receive supplementary, interdisciplinary funding opportunities. Here we discuss areas of research for understanding the space environments of exoplanetary systems and observational and collaborative opportunities and challenges.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-644eaa864bc2a18c07a783f319c770ec_ExoDecadalWhitePaper_-_Final_Version.pdf"
"312","7 September 2022 4:21:41 pm","D Aaron","Roberts","0000-0001-6565-2921","NASA GSFC Code 672","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-c283bd398249ac7e6983d1f9eae80059_SSPH_Roberts_White_Paper_Author_Information_Form.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","The Heliophysics Digital Resource Library: An Open, Flexible, Easily Used Infrastructure for Data, Software, Registration, Documentation, and Services","NASA HP provides an infrastructure (""HDRL"") that makes NASA and other HP data easily discoverable and uniformly accessible with standard data and metadata formats. HDRL is building big data computational facilities with both ""on premise"" HEC and NASA-AWS cloud capabilities. Open science based on these services will enable both traditional and new (""big data,"" ""AI/ML"") problem solutions.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-341c5b93fbea8c72417648374ae888fc_RobertsDAaron.docx"
"314","7 September 2022 4:25:50 pm","Albert","Shih","0000-0001-6874-2594","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-497ef0c7d883f76e51d70894440e1457_Shih_-_FIERCE_-_author_information.xlsx","Basic Research","Solar Physics;Basic research that is driven by space weather user needs","","","","","","","","","Space-based","Fundamentals of impulsive energy release in the corona","It is essential that there be coordinated and co-optimized observations in X-rays, gamma-rays, and EUV during the peak of solar cycle 26 (~2036) to significantly advance our understanding of impulsive energy release in the corona. These observations can be achieved through a single flagship mission or through a combination of major missions (e.g., the previously proposed FIERCE mission concept).","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-8163b8bfe331f7530612e6a5444e9578_ShihAlbertY2.pdf"
"315","7 September 2022 4:39:43 pm","Lucas","Tarr","0000-0002-8259-8303","National Solar Observatory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-b6375addf9ad1c67b472bd2da15c9dca_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics","","","","","","","","","","Enabling data-driven modeling and real-time prediction of the dynamic solar atmosphere","Data driven simulations and supporting infrastructure must be advanced such that community members can easily use time dependent dynamic models on a regular basis as a tool to interpret observations and test physical theories for the region between the photosphere and Alfvén surface. This requires tight integration between simulation development, forward modeling, and multi-facility observations.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-5e3eceed78964ea79931fbc92352be5a_TarrLucasA.pdf"
"316","7 September 2022 4:39:01 pm","Carolyn","Ng","","ADNET Systems Inc./NASA HEAT","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-777161db50bd67d595ad9299eeb342e8_SSPH_Spaec_Weather_Literacy_White_Paper_Author_Information_Form_NgCarolynY.xlsx","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Other Space Weather","","","Other Programmatic","","","","Building Space Weather Literacy Through Sustained Engagement","Space weather affects all space systems, both natural and artificial. A rapid growth of awareness and a critical need for space weather prediction requires building space weather literacy within K-14 classrooms. This white paper group recommends an annual celebration of space weather week, covering various topics in heliophysics through sustained engagement beyond celestial and spacecraft events. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-0044aa7a3d8661c309d76879a682b921_NgCarolynY.pdf"
"317","7 September 2022 4:42:12 pm","Pascal","Saint-Hilaire","0000-0002-8283-4556","University of California Berkeley","","","","","","","","","","","","","","","","","","","","","","","","","","","Space Weather Applications","","","","Space Weather Research to Operations to Research Loop","","","","","","Ground-based","Diagnostics of Space Weather Drivers Enabled by Radio Observations","We outline the relevant space weather drivers, describe the potential role of radio observations and list the required measurement approach: namely, ultrabroadband imaging spectropolarimetry. The insights provided by radio observations of space weather drivers will not only inform the science of space weather, they will pave the way for new tools for forecasting and ""nowcasting"" space weather.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-cb1c57192253f534dd6070c1b817545c_Saint-HilairePascal.pdf"
"319","7 September 2022 4:43:20 pm","Bin","Chen","0000-0002-0660-3350","New Jersey Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-734fd8b1446de74d83d0ab22ec119e87_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics;Basic research that is driven by space weather user needs","","","","","","","","","Ground-based","Radio Imaging Spectropolarimetry of CMEs and CME Progenitors","This white paper provides an overview of radio diagnostics for CMEs and CME progenitors, with a particular focus on the unique means for constraining their magnetic field and energetic electron population. We demonstrate the transformative potential of advancing such diagnostics by using broadband radio imaging spectropolarimetry with a high image dynamic range and high image fidelity. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-5296afc1bbb524c84a4607e5762d9e7b_ChenBin1.pdf"
"320","7 September 2022 4:47:39 pm","Kan","Liou","0000-0001-5277-7688","Johns Hopkins University Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-6b91d36794b99768fed691e54d24b02b_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","","","","","","","Space-based","Interhemispheric Conjugacy Explorer (ICE) – A Mission Concept","ICE will provide global, continuous and concurrent observations of aurora, polar cap, thermosphere and ionosphere in the Northern and Southern Hemispheres to transform our understanding of the magnetosphere-ionosphere-thermosphere system from ""local"" to ""global,"" thus allowing us to address interhemispheric asymmetries including both the sources and consequences.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-49ae4e1e0a0f49a95ed9b62cc2845d98_KanLiou.pdf"
"321","7 September 2022 4:48:13 pm","Alessandro","Retino","0000-0001-5824-2852","Laboratoire de Physique des Plasmas, CNRS/Sorbonne Université/Université Paris Saclay/Observatoire de Paris/Ecole Polytechnique/Institut Polytechnique de Paris, Paris","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-60a6c9c9ce36f31b6a01a0d5d6c2f90d_RetinoAlessandro_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","Space-based","Unveiling plasma energization and energy transport in the Earth’s Magnetospheric System: the need for future coordinated multiscale observations","This WP highlights the importance of plasma scale coupling to study plasma energization and energy transport in the terrestrial Magnetospheric System. The Plasma Observatory is an ESA mission concept to resolve fluid and ion scales. MagCon is a NASA mission concept aiming at studying larger mesoscales. Resolving the couplings among all these scales requires a strong international collaboration. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-fae32fc0a4365e31628f8b3a53d12180_RetinoAlessandro.pdf"
"322","7 September 2022 4:50:59 pm","Adam","Szabo","0000-0003-3255-9071","NASA Goddard Space Flight Center","George","Lan","David","Teresa","","Ho","Jian","Lario","Nieves-Chinchilla","","0000-0003-1093-2066","0000-0002-6849-5527","0000-0002-6651-7120","0000-0003-0565-4890","","[email protected]","[email protected]","[email protected]","[email protected]","","Johns Hopkins University Applied Physics Laboratory","NASA GSFC","NASA GSFC","NASA GSFC","","","Basic Research","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Basic research that is driven by space weather user needs","","","","","","","","","Space-based","ICME Structure and Evolution in the Inner Heliosphere","The internal structure and evolution of ICMEs in the inner heliosphere remains poorly understood. Similarly, the transport and diffusion of solar energetic particles on their way to 1 AU is surrounded by controversy. This white paper outlines possible next research objectives and a possible multi-spacecraft mission concept (HELIIX) that would provide the measurements to achieve these objectives.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-5d220d9ac216575f981082f97e3794d5_SzaboAdam.pdf"
"323","7 September 2022 4:58:24 pm","Jeng-Hwa","Yee","0000-0002-8269-424X","JHU/APL","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-b823c64e703b914228fcdd192bd9af9f_YeeJeng-Hwa1.xlsx","Basic Research","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","Circuit: A Mission to Unlock the Secrets of Earth’s Global Current System","This paper presents the foundation for the Circuit mission, a new, bold mid-to-large-scale mission is that with the goal to understand the fundamental mechanisms of momentum and energy transport between the magnetosphere and ionosphere. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-e65d95f3ca701a1e0416ade640b563e2_YeeJeng-Hwa1.pdf"
"324","7 September 2022 4:59:07 pm","James","Klimchuk","0000-0003-2255-0305","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-f0f217a928c1b252fcc9014acae01dba_KlimchukJamesA1.xlsx","Basic Research;Space Weather Applications","Solar Physics;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","Space Weather Pipeline from Research to Application to Operations","","","","","","","Heating of the Magnetically Closed Corona and Physical Models of Solar and Stellar Spectral Irradiances","We present a strategy for answering the question of how the magnetically closed corona is heated. It is focused on the goal of constructing physics-based models that can nowcast and eventually forecast the solar spectral irradiance for space weather operations. Such models will also be invaluable for studying the spectral irradiance from other stars and its effect on the development of life.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-5b103a8b1bec4e487e9cba1c257f435e_KlimchukJamesA1.pdf"
"325","7 September 2022 5:01:01 pm","Joshua","Pettit","0000-0003-3733-6774","George Mason University/NASA GSFC","Sadie","Cora","Alexa","Allison","Katherine","Elloitt","Randall","Halford","Jaynes","Garcia-Sage","0000-0001-8661-7252","0000-0002-4313-4397","000-0002-5383-4602","0000-0002-1470-4266","0000-0001-6398-8755","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","University of Minnesota","University of Colorado/LASP","NASA GSFC","University of Iowa","NASA GSFC","","Basic Research;Space Weather Applications","Planetary Magnetospheres;Planetary ionospheres/upper atmospheres","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Space-based","Investigation of the drivers and atmospheric impacts of energetic electron precipitation","The drivers and impacts of energetic electron precipitation are still an outstanding question in both space physics and atmospheric science. Further investigation is needed to quantify both the causes and effects of this process. We recommend support for research and modeling efforts. Additionally, we advocate for the upcoming GDC mission along with the continuation of the MLS and SABER missions. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-5ffdf793376f05b4622bd4cf1cc0fb01_PettitJoshuaM.pdf"
"326","7 September 2022 5:01:01 pm","Bin","Chen","0000-0002-0660-3350","New Jersey Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-b2cf4c6c41bd4119fd59affd0f90814f_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics;Basic research that is driven by space weather user needs","","","","","","","","","Ground-based","Radio Studies of the Middle Corona: Current State and New Prospects in the Next Decade","The middle corona, defined as the region between ~1.5-6 solar radii, is a critical transition region that connects the highly structured lower corona to the outer corona where the magnetic field becomes predominantly radial. This paper discusses the current state of radio studies on the middle corona, challenges to obtaining a more comprehensive picture, and recommends an outlook. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-0f6c4ca34537b0738d08693bcdd4d44d_ChenBin2.pdf"
"327","7 September 2022 5:02:55 pm","Gordon","Petrie","0000-0001-8462-9161","National Solar Observatory","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research;Space Weather Applications","Solar Physics","","","Space Weather Research to Operations to Research Loop","","","","","","Space-based","Improving Global Solar Magnetic Field Maps: Why Multiple Low- and High-latitude Vantage Points are Necessary","Key solar physics projects rely on complete, up-to-date full-surface maps for the photospheric magnetic field. These projects are frustrated because the maps unavoidably contain out-of-date, inaccurate information. This problem cannot be solved without full-surface observational coverage. A multi-satellite mission providing vantage points in the ecliptic plane and in polar orbits is needed.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-19cb0e2d0313ee3c5e1c8932698e338d_PetrieGordonJD2.pdf"
"328","7 September 2022 5:03:47 pm","Steven","Christe","0000-0001-6127-795X","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-dce525e629d3ed5770394c1f69fbc908_FOXSI_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Solar Physics","","","","","","","","","Space-based","The Focusing Optics X-ray Solar Imager (FOXSI)","FOXSI is a hard X-ray mission that detects emission from high in the tenuous corona, where previous instruments have been blinded by nearby bright features, It will fully characterize the accelerated electrons and hottest plasmas as they evolve in energy, space, and time to solve the mystery of how impulsive energy release leads to solar eruptions, the primary drivers of space weather at Earth.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-9094049a37be20110f9e7170a85ecc6d_ChristeStevenD.pdf"
"329","7 September 2022 5:08:56 pm","Nicholas","Featherstone","0000-0002-2256-5884","Southwest Research Institute, Department of Space Studies","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-805d127edc07ffe06b94b1f723c76a3f_SSPH_Convection_White_Paper_Author_Information.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Solar Physics","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","The Puzzling Structure of Solar Convection: Window into the Dynamo","The operation of the solar dynamo remains an outstanding problem of solar physics owing to continuing uncertainty in the speed and structure of deep-seated convective flows. We discuss the relationship between this aspect of convection and the dynamo. We suggest that observations of the solar poles, coupled with theory and simulation are vital to attain new perspectives on the dynamo.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-99342fb7f4bc9c19fb229353f38fc693_FeatherstoneNicholasA.pdf"
"330","7 September 2022 5:13:12 pm","James","Klimchuk","0000-0003-2255-0305","NASA Goddard Space Flight Center","Spiro","","","","","Antiochos","","","","","0000-0003-0176-4312","","","","","[email protected]","","","","","U. Michigan & U. Maryland","","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","","Expansion of Existing Research and Analysis Programs","Small-grants programs play a vital role in Heliophysics research. They are a modest investment with a huge scientific payoff. We therefore recommend that existing NASA programs like Heliophysics Supporting Research (HSR), Heliophysics Guest Investigator (HGI), and Heliophysics Technology and Instrument Development for Science (HTIDeS) be greatly expanded. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-eadfaf5157b9fe4e5b58278cc4400a3e_KlimchukJamesA2.pdf"
"331","7 September 2022 5:15:15 pm","Jesse","Miller","0000-0001-5071-0412","Boston University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-4ad9679912f76600f22c27d6a092e89d_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","","Near-Earth Supernovae in the Past 10 Myr: Implications for the Heliosphere","We summarize evidence that multiple supernovae exploded within 100 pc of Earth in the past few Myr. These events had dramatic effects on the heliosphere, compressing it to within ~20 au. We advocate for cross-disciplinary research of nearby supernovae, including on interstellar dust and cosmic rays. We urge for support of theory work, direct exploration, and study of extrasolar astrospheres.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-e2e7be0ed14dd93f8df539452bd881e6_MillerJesseA.pdf"
"333","7 September 2022 5:16:50 pm","Nathaniel","Frissell","0000-0002-8398-4222","The University of Scranton","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-f524fd04c8d105fa32d4dada355eaf07_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Ground-based","Amateur Radio: An Integral Tool for Atmospheric, Ionospheric, and Space Physics Research and Operations","This white paper describes the current technical and scientific capabilities of the global amateur radio community and gives recommendation for using these capabilities to advance heliophysics and space weather operations over the next decade.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-c7e812d82a94930981b2c41dd75c713f_FrissellNathanielA1.pdf"
"334","7 September 2022 5:19:17 pm","Nathaniel","Frissell","0000-0002-8398-4222","University of Scranton","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-0bbe7b7d82f0cba0823653ef05c5c0ad_SSPH_White_Paper_Author_Information_Form.xlsx","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Fostering Collaborations with the Amateur Radio Community","This white paper provides recommendations on fostering a collaborative relationship between the professional heliophysics and amateur radio communities.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-2057212dc4278aa97e2376988073f246_FrissellNathanielA2.pdf"
"335","7 September 2022 5:20:05 pm","Muhammad Fraz","Bashir","0000-0003-1933-6375","University of California Los Angeles","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-108218769eb9cf570926c0d4e6d945d6_SSPH_White_Paper_Author_Information_Form_BashirFrazFinal.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Other topic relevant to solar and space physics/heliophysics","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Other Programmatic","","","","Recognition for All: A Way Forward to Enhance Diversity, Equity and Inclusion in Space Physics","The white paper summarizes the current state of different historically marginalized groups in the AGU SPA section including NTF's progress in significantly enhancing the nomination of these groups for AGU honors and awards, the best practices and challenges faced by NTF, and recommendations for improving the nomination process for different societies, agencies, and universities/institutions.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-00a8dcf6ad2fed0f5a317320b1f56437_BashirMFrazfinal.pdf"
"336","7 September 2022 5:22:44 pm","Simone","Di Matteo","0000-0001-6407-7574","The Catholic University of America/NASA-GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-0756b86b4461c4039a80bea0d3171f3f_DiMatteoSimoneSSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop","","","","","","","Solar-Wind/Magnetosphere coupling: Understand Uncertainties in Upstream Conditions","Solar wind parameters that impact the magnetosphere are uncertain due to the variability of the solar wind at L1 as well as physical processes downstream. These uncertainties affect our understanding of magnetosphere response, models, and space weather forecasting. In the next decade, paired with multi-spacecraft missions, we make a case for placing resources in addressing these uncertainties.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-732ee5928592528782effc1e7e6d37c0_DimatteoSimone.pdf"
"337","7 September 2022 5:26:03 pm","Douglas","Rabin","0000-0003-4666-7137","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-64e430691adf994ca8d266311121b1b0_RabinDouglasM_White_Paper_Author_Information_Form.xlsx","Basic Research","Solar Physics;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Ground-based;Space-based","Observing Coronal Microscales and their Connection with Mesoscales","Coronal heating remains a fundamental open problem in space physics. It is expected that thermal structure on scales ≲100 km will be produced by primary heating mechanisms operating on kinetic scales. We consider what could be learned from direct observations of coronal microscales and their connection with larger scales. We briefly outline a mission concept for the Coronal Microscale Observatory.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-cde188693360a73fd9aadd21bd22c45b_RabinDouglasM.pdf"
"338","7 September 2022 5:28:03 pm","Bin","Chen","0000-0002-0660-3350","New Jersey Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-2b55a0daf32ba04f9a894a854830d829_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics;Basic research that is driven by space weather user needs","","","","","","","","","Ground-based","Quantifying Energy Release in Solar Flares and Solar Eruptive Events: New Frontiers with a Next-Generation Solar Radio Facility","This white paper concerns outstanding questions and challenges pertinent to energy release in solar flares and solar eruptions. We demonstrate how a next-generation radio facility with many antenna elements can bring the next revolution by enabling high dynamic range, high fidelity broadband imaging spectropolarimetry with a sub-second time resolution and arcsecond-level angular resolution.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-8380f292c3cb167ae646a9a9aef568a4_ChenBin3.pdf"
"339","7 September 2022 5:32:11 pm","Prabal","Saxena","","NASA Goddard","Natalie","Heather","","","","Curran","Graham","","","","","","","","","[email protected]","[email protected]","","","","Catholic University/CRESST II/NASA Goddard","NASA Goddard","","","","","Basic Research;Space Weather Applications","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment;Other Space Weather","","","","","","","Lunar Samples are Time Capsules of the Sun","The history of the Sun is buried in the surface of the Moon, which is particularly exciting given the upcoming planned efforts for long term human exploration of the Moon and a return of a large mass of diverse lunar samples. The Decadal survey should actively embrace this coming opportunity and facilitate cross-disciplinary efforts to unlock the secrets of the Sun held by the lunar surface. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-9b0a529266f24793293cab6e6f939e4f_SaxenaPrabal.pdf"
"340","7 September 2022 5:33:10 pm","Juliana","Vievering","0000-0002-7407-6740","Johns Hopkins Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-53883c6a1ea4128c5555aee6e66e5560_Early_Flare_Alerts_White_Paper_Author_Information_Form_final.xlsx","Space Weather Applications","","","","Space Weather Research to Operations to Research Loop","","","","","","","Early Flare Physics and Flare Alerts","We advocate for the development of near-term flare predictions: predictions that are more actionable than long-term forecasts and provide earlier notice than current flare alerts do. These predictions will provide insight into early flare physics and value for a range of applications, including coordinated observing campaigns, solar instrument technology development, and space weather alerts. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-86ac29ba6e477bf29c6b64dd0040c221_VieveringJulianaT1.pdf"
"341","7 September 2022 5:33:14 pm","Bala","Poduval","0000-0003-1258-0308","University of New Hampshire","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-12efd5be5563563ea583d9a8b4ba3f9d_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Space Weather Applications","Solar Physics;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","Space Weather Pipeline from Research to Application to Operations;Other Space Weather","","","","","","Ground-based;Space-based","AI-ready Data in Solar Physics and Space Science: Concerns, Mitigation and Recommendations","Extracting scientific information from the existing huge volumes of space science data without the application of artificial intelligence (AI) is becoming impractical. Preparing these data AI-ready is challenging due to various reasons. This white paper compiles known issues and recommends ways of addressing them efficiently for providing repositories of AI-ready data within the next decade.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-1870187ec154eee48664bed68513f0cb_PoduvalBala.pdf"
"342","7 September 2022 5:36:28 pm","Nathan","Schwadron","0000-0002-3737-9283","University of New Hampshire","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-71052df645a442787e950967eca4c1d0_SSPH_White_Paper_Author_Information_Form_Final.xlsx","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Other Space Weather","","","","","","Space-based","Sun-2-Stars (S2S): Unified Understanding of Our Space Environs from the Sun’s Poles through the 3D Solar Wind and Out Toward the Stars","The Sun-2-Stars (S2S) mission uses the first nearly circular-polar orbit (~5 au, 65º inc), enabling a suite of in situ observations and remote imaging to explore the linked system from the polar-3D Sun through the heliosphere and into the interstellar medium. S2S is the next step in Heliophysics, unifying our 3-D view of solar interactions from the Sun out to the galactic environment.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-36bbc625208709f41f27cc42be00d96c_SchwadronNathanA.pdf"
"343","7 September 2022 5:36:42 pm","Romina","Nikoukar","0000-0002-8608-2822","The Johns Hopkins University Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-ab4c089482beab9d8726c3752cf00212_RominaNikoukar1-SSPH_White_Paper_Author_Information_Form.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","","Raising Awareness on Mental Health in the Heliophysics Community","Our research community should also acknowledge the importance of mental health and mental well-being, and work toward addressing mental health issues in our field. We advocate for a cultural change towards eliminating the stigma around mental illness, and encouraging an open culture around mental health discussions and to conduct professionally developed comprehensive mental health surveys.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-0c3259aa0f4f23fa5808412649ef1667_RominaNikoukar1.pdf"
"344","7 September 2022 5:41:51 pm","larry","paxton","0000-0002-2597-347X","jhu/apl","scott","justin","","","","bailey","yonker","","","","0000-0001-7693-0966","0000-0003-1334-426X","","","","[email protected]","[email protected]","","","","vt","jhu/apl","","","","","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Space-based","Understanding MLT Energetics Through Observations of Nitric Oxide","We propose that during the next decade of research, the NSF and NASA community invest in developing and flying Middle Ultraviolet (MUV: 200 to 300nm) spectrographic imagers for mapping the important tracer of ITM processes: Nitric Oxide (NO). Understanding composition changes in response to solar and geomagnetic forcing is crucial to understanding the energy balance of the upper atmosphere. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-3e83eddd81feb586e233ee81d02b3936_paxtonlarryj5.pdf"
"345","7 September 2022 5:47:38 pm","Erika","Palmerio","0000-0001-6590-3479","Predictive Science Inc., San Diego, CA 92121, USA","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-630f507cc9aeb1f40f6c122533043db8_SSPH_White_Paper_Author_Info_Palmerio_et_al.xlsx","Basic Research","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","","","","","New Observations Needed to Advance Our Understanding of Coronal Mass Ejections","This White Paper aims to identify the data sets and observational priorities that are needed to effectively advance our current understanding of the structure and evolution of coronal mass ejections (CMEs) from their eruption at the Sun through their heliospheric propagation, in both the remote-sensing and in-situ regimes.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-9a3a5e9bcbeaa75b982af583b619ed54_PalmerioErika.pdf"
"346","7 September 2022 5:59:25 pm","Douglas","Rowland","","NASA GSFC","Larry","Robert","Alex","Katherine","","Kepko","Pfaff","Glocer","Garcia-Sage","","0000-0002-4911-8208","0000-0002-4881-9715","0000-0001-9843-9094","ORCID iD 0000-0001-6398-8755","","[email protected]","[email protected]","[email protected]","katherine.garcia-sage@ nasa.gov","","NASA GSFC","NASA GSFC","NASA GSFC","NASA GSFC","","","Basic Research","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","","Investigating bidirectional, multiscale, and nonlinear feedback in plasma-neutral coupling, using Geospace to study universal phenomena","Geospace, which extends from Earth's middle atmosphere through the upper atmosphere, ionosphere, and magnetosphere, serves as a ""natural laboratory"" that is readily accessible and can be used to explore how ionized and neutral gases, under a variety of drivers, interact to produce complex, multiscale, and nonlinear feedback that is bidirectional, and which modifies both populations. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-2b669fad1bc487c7f842676017382b08_RowlandDouglasE2.pdf"
"347","7 September 2022 5:54:13 pm","Seth","Dorfman","0000-0001-5955-9552","Space Science Institute","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-289d2d5a40c3841a6b62f4416fd1a1cf_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Laboratory space plasma physics","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Next Generation Machine to Study Heliophysics in the Laboratory","How the solar wind is accelerated, heated, and driven turbulent is among the most important open questions in Heliophysics, but hard to address using spacecraft missions and numerical simulations alone. To complement these approaches, it is important to build a laboratory Solar Wind Machine to isolate, control, and diagnose plasma phenomena responsible for the complex solar wind behavior.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-3c997cea13ab7eae422c0cf8fb082115_DorfmanSeth.pdf"
"348","7 September 2022 5:54:28 pm","Paul","Boerner","0000-0002-4490-9860","Lockheed Martin Solar and Astrophysics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-ef1aac889e8b848502981b445de1a88a_SDC_authors.xlsx","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop;Other Space Weather","","","","","","Space-based","Solar Dynamics Constellation","The Solar Dynamics Constellation is a mission architecture that will take advantage of the convergence of advancing technology and the accelerating commercialization of space to significantly advance the understanding of the global nature of solar activity and dramatically improve the power, relevance, and resiliency of the space weather data that the scientific community and the nation rely on. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-7d169154fe9861b1072e035062fd6f1d_BoernerPaul.pdf"
"349","7 September 2022 5:58:13 pm","Pontus","Brandt","0000-0002-4644-0306","The Johns Hopkins University Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-8d665ed0a72cfe9fe612adb79a67215f_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","Pushing the Frontier of Solar & Space Physics: Exploration of the Heliosphere and the Very Local Interstellar Medium by an Interstellar Probe","The white paper describes the science enabled by an Interstellar Probe and its pragmatic mission implementation for launch in the 2030's.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-44e3f897d3cfbed99df32b2c08f80e6f_BrandtPontusC.pdf"
"350","7 September 2022 5:58:28 pm","Ignacio","Ugarte-Urra","0000-0001-5503-0491","Naval Research Laboratory, USA","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-90bbf5bb00bffdc4ad4a6e350876a8c0_UgarteIgnacio_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics","","","","","","","","","","The Case for Solar Full-disk Spectral Diagnostics","The white paper argues that spatially-resolved spectral diagnostics over the full solar disk should be made a high-priority goal in Heliophysics and lead to the development of a mission providing consistent full-disk sampling of plasma properties (Doppler-shifts, non-thermal velocities, electron densities, elemental composition, etc.) at the dynamic timescales of solar eruptive phenomena.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-b16aef10110656d9607adb3644963cd3_UgarteIgnacio.pdf"
"351","7 September 2022 6:00:09 pm","Robert","Schaefer","0000-0003-3692-0223","Johns Hopkins U. Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-8413ff4a4a43756d06f6a8b40d6c2b52_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop","","","","","","Space-based","Next Generation FUV Spectrographic Imaging for Heliophysics","A big challenge in Ionosphere/Thermosphere science is measuring high latitude particle inputs while also measuring the response of the thermosphere and ionosphere. Far Ultraviolet imagers, like NASA's TIMED/GUVI can provide that capability from low-cost space platforms. Improved gratings and detectors will enable next generation instruments to provide additional information for new science. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-929832d2a08d2cd03c76feab3c546164_SchaeferRobertK.pdf"
"352","7 September 2022 6:02:18 pm","Peter","Young","0000-0001-9034-2925","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research","Solar Physics","","","","","","","","","Space-based","The Case for an SDO Follow-On Mission","I advocate for a future mission to replace the extreme ultraviolet imaging and magnetic field imaging capabilities of the Solar Dynamics Observatory (SDO). ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-f7fccfbaf7946b2a1fe339beb9eedd39_sdo_follow_on.pdf"
"353","7 September 2022 6:01:50 pm","Gregory","Howes","0000-0003-1749-2665","University of Iowa","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-78f918cdd181f370d8f9e5d5d18893d4_HowesGregoryG.xlsx","Basic Research","Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","Space-based","Revolutionizing our Understanding of Particle Energization in Space Plasmas Using On-Board Wave-Particle Correlator Instrumentation","The development of on-board wave-particle correlator instrumentation using existing instrumental capabilities makes it possible to probe the collisionless wave-particle interactions governing plasma heating and particle acceleration in the heliosphere at full measurement cadence while circumventing telemetry constraints, enabling us to maximize the scientific return from future missions.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-6585a2bcef27b86966dfcd9c6264452c_HowesGregoryG.pdf"
"354","7 September 2022 6:04:59 pm","Alexa","Halford","0000-0002-5383-4602","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-ab7c28cc676bc04ee01d1f27e3ecd17f_Artemis_Gateway.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Other topic relevant to solar and space physics/heliophysics","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Other Programmatic","","","Ground-based;Space-based","Artemis, Gateway, the return to the Moon and forward to Mars for Heliophysics","Artemis provides a unique opportunity for heliophysics and space weather. The frequent return to the lunar environment itself provides new science questions we heliophysics can address from the ancient Sun, to interactions with the surface, and impacts on our technology and humans living and working in space. Heliophysics must take advantage of this rare opportunity.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-77a5ae97d29c46566c1574a7284a02d6_HalfordAlexaJ_10.pdf"
"355","7 September 2022 6:06:32 pm","Elena","Provornikova","0000-0001-8875-7478","Johns Hopkins Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-4e4b4318c9653f28b658a41f02a4d745_Authors_WhitePaper_Provornikova_Decadal.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","","Structured solar wind from the Sun to the boundary of the heliosphere: required measurements and simulation tools","We outline open questions on the evolution of large-scale solar wind structures throughout the heliosphere. We recommend in-situ observations on an outward trajectory from the Sun of plasma, fields, suprathermal and energetic particles, interstellar dust, and gas. An Interstellar Probe mission would provide such measurements and enable the needed lead in understanding the solar wind evolution.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-f30391aadc8a16556f0569bd3a712f75_Dynamic_solar_wind_Elena_DecadalWP_FINAL.pdf"
"356","7 September 2022 6:07:04 pm","Samuel","Hart","0000-0003-0508-4912","The University of Texas at San Antonio","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-1943f96c8495653b1354a964790d7c77_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","","Impulsive Solar Energetic Particle Events: A Pathway to Understanding the Sun","The origins and acceleration mechanisms of Impulsive Solar Energetic Particle (ISEP) events remain unanswered. ISEP events are (1) easily identifiable because of their unique abundance enhancement of 3He and (2) fundamental in nature as a direct consequence of magnetic reconnection. Thorough research of ISEP events can strongly develop our understanding of heliospheric physical processes.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-688948cd6edcfe8b103e1590814809a7_HartSamuelT.pdf"
"357","7 September 2022 6:12:24 pm","Kenneth","Marr","0000-0002-8556-7246","U.S. Naval Research Lab","Christoph","John","","","","Englert","Harlander","","","","0000-0002-2145-6168","0000-0002-0625-8948","","","","[email protected]","[email protected]","","","","U.S. Naval Research Lab","St. Cloud State University/SSRC","","","","","Basic Research","Planetary ionospheres/upper atmospheres","","","","","","","","","","The INDI Instrument: A Miniaturized Implementation of the DASH Technique for Measuring Upper Atmospheric Oxygen Winds","The INDI instrument has been designed to measure red-line (=630.0 nm) oxygen emissions in the upper atmosphere with a small footprint that will fit in a 6U cubesat or smallsat. INDI uses a Doppler Asymmetric Spatially Heterodyned (DASH) interferometer to observe the wind-induced Doppler shift of thermospheric airglow emission to determine horizontal wind vectors versus altitude.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-cc2346e711a37e17047dd685b3ecedf3_MarrKennethD.docx"
"358","7 September 2022 6:16:22 pm","Reka","Winslow","0000-0002-9276-948","Space Science Center, University of New Hampshire","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-8715f3000f6b48be66a63d54d5d0eb6f_WinslowRekaM_author_list.xlsx","Basic Research","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","","","","","On the importance of investigating CME complexity evolution during interplanetary propagation","This white paper brings to light the need for comprehensive studies on the evolution of interplanetary coronal mass ejection (ICME) complexity during propagation. To date, few studies of ICME complexity exist. In this white paper, we define ICME complexity and accompanying changes in complexity, describe recent works and their limitations, and outline key science questions that need to be tackled. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-e6a0226de47593a2212e0dc9bfaa5b8e_WinslowRekaM.pdf"
"359","7 September 2022 6:17:02 pm","Valery","Yudin","0000-0002-2134-4430","The Catholic University of America","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-60eab686d0b8aac334f742d9d57d7424_SSPH_White_Paper_Author_Information_Form.xlsx","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Observing System Simulation Experiments (OSSEs) for ITM Monitoring in the Earth Observing System","We recommend developing and coordinating Observing System Simulation Experiments (OSSEs) in the Ionosphere-Thermosphere-Mesosphere for effective utilization of planned multi-platform measurements in the Earth and Geospace observing systems for the space weather forecasts and applications.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-84bce622b2c9130bf99d8e98fddfda53_WP-OSSE-ITM_2022.pdf"
"360","7 September 2022 6:22:52 pm","Douglas","Rowland","0000-0003-0948-6257","NASA GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-01dc6528ac852fe9126bb1b2d44eaa98_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","Cross-Scale and Cross-Regime Coupling in the ITM: Studying Weather, not just Climate, in the Middle and Upper Atmosphere","The ITM regime is a critical region in the geospace system, where the dominant physical processes transition from neutral dynamics to plasma dynamics. This region is sensitive to forcing from both above (Solar radiation, solar wind, and magnetosphere) and below (lower atmosphere). NASA must understand how the ITM system varies at mesoscales, all over the globe, on timescales of minutes to days.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-5b199016a79fdd2a2dbad737f3327109_RowlandDouglasE3.pdf"
"361","7 September 2022 6:24:25 pm","Roger","Varney","0000-0002-5976-2638","University of California, Los Angeles","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-4ff6bc2f846d606a72d70a5b5e86b352_SSPH_White_Paper_Author_Information_Form_2.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","State of the Profession: Maintaining and Expanding Incoherent Scatter Radar Expertise within the US Geospace Community","Incoherent scatter from the ionosphere remains the most powerful, and only, ground-based technique to observe full-altitude profiles of fundamental ionospheric properties such as electron density and electron and ion temperature. Ensuring the future success of incoherent scatter radar (ISR) theory and practice will require extensive new workforce development initiatives.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-41270fe62215d9888638bcae50d3f60a_VarneyRogerH1.pdf"
"362","7 September 2022 6:25:53 pm","Anthony","Mannucci","0000-0003-2391-8490","Jet Propulsion Laboratory, California Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-dee46f45b3496aaa530b19f2459bd76e_SSPHWhitePaperAuthorInformationFormMannucciAnthonyJ.xlsx","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","","The Future of Space Weather Prediction and Forecasting","This white paper is based on recommendations developed after the Chapman Conference on Scientific Challenges Pertaining to Space Weather Forecasting Including Extremes (2019). Continuously available low latency observations relevant to space weather prediction have not advanced to a significant degree. The complexity of space weather requires developing new approaches to predictive modeling.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-ef2e361c67b7d12a60e8bfbc4ec1c181_MannucciAnthonyJ.pdf"
"363","7 September 2022 6:29:23 pm","Roger","Varney","0000-0002-5976-2638","University of California, Los Angeles","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-82efe350d4ab5e790a0cedfa2b7d6ef4_SSPH_White_Paper_Author_Information_Form.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Revitalization and Continuation of Polar Cap Science from the Resolute Bay Observatory","The Resolute Bay Observatory (RBO) in Resolute Bay, Nunavut, Canada provides a unique location for polar cap science. The facility is greatly in need of additional investment and revitalization, especially if operations are to continue into the GDC era. We estimate that a revitalization plan would be comparable in expense to a facility in the NSF Mid-Scale 1 funding line.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-783a54d123e8d70e31ec3efc2f4fdd0a_VarneyRogerH2.pdf"
"364","7 September 2022 6:31:26 pm","Donald M.","Hassler","0000-0001-8830-1200","Southwest Research Institute","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-118d3c9c715a7b73a2ad6e77f8a974a6_Solaris_-_SSPH_WP_Author_Info_Form_-_FINAL_-_7sept22.xlsx","Basic Research;Space Weather Applications","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","Space Weather Research to Operations to Research Loop;Other Space Weather","","","","","","Space-based","Solaris: A Focused Solar Polar Discovery-class Mission to achieve the Highest Priority Heliophysics Science Now","Solaris is a transformative Solar Polar Discovery-class mission concept to address crucial outstanding questions that can only be answered from a polar vantage. Solaris will image the Sun's poles from 75° latitude, providing new insight into the workings of the solar dynamo and the solar cycle, which are at the foundation of our understanding of space weather and space climate. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-10a14cf6fddf9e5bc6d4746de00a3b98_HasslerDonaldM.pdf"
"365","7 September 2022 6:31:58 pm","Roberto","Casini","0000-0001-6990-513X","National Center for Atmospheric Research","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-6214e2ed0a98347ee78effee6d7aff72_CasiniRobertoAuthors.xlsx","Basic Research","Solar Physics;Basic research that is driven by space weather user needs","","","","","","","","","Space-based","Solar Coronal Polarization Diagnostics with H I Ly-α","To advance heliophysics and space weather research we must investigate magnetic energy buildup in coronal eruption precursors and the heating mechanisms of the solar-wind plasma. Thus, we must measure the coronal magnetic field strength and the temperature anisotropy of the solar wind, quantities that are currently unobserved but essential to the dynamic evolution of the Sun's corona and heliosphere. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-0ac0de9447044db45105c117da20d66a_CasiniRoberto.pdf"
"366","7 September 2022 6:34:44 pm","Roger","Varney","0000-0002-5976-2638","University of California, Los Angeles","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-3b6bf6138b434019311d627f00b531fe_SSPH_White_Paper_Author_Information_Form_3.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Continued Multi-Instrument Studies at the Poker Flat Research Range","The Poker Flat Research Range (PFRR) hosts a unique collection of instruments. These instruments need additional investment, especially if PFISR is to continue operations into the GDC era. We estimate that a coordinated program to manufacture and replace components in all of the existing AMISRs would be comparable in expense to an NSF Mid-Scale 1 facility proposal.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-dd3eb0855d26e191ad932a761d915120_VarneyRogerH3.pdf"
"367","7 September 2022 6:37:47 pm","Nikolai V.","Pogorelov","0000-0002-6409-2392","The University of Alabama in Huntsville, Huntsville, USA","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-4ef175998324fe06082f60ec0fdd0b91_PogorelovNikolaiV_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","","Heliosphere in the Local Interstellar Medium","We outline the main challenges in the physics of the SW--LISM interaction. The physical processes that require a focused attention of the heliospheric community are discussed from the theoretical perspective and space missions necessary for their investigation. We emphasize the importance of data-driven simulations, which are necessary for the interpretation and explanation of spacecraft data.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-82b4569b716da98a49746fa1aef43cf4_PogorelovNikolaiV.pdf"
"368","7 September 2022 7:08:43 pm","Robert","Pfaff","0000-0002-4881-9715","NASA/Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-5b3429eaa3dcc58734e0a97f9fa4118b_PfaffRobertF1_author_info.xlsx","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations","","","","","","","Exploring the Earth’s Atmosphere-Space Transition Region with Direct Measurements","To understand the Earth's atmosphere-space transition region, direct, high-resolution measurements of several key parameters are required to reveal the characteristics and energy exchange within the lower ionosphere/thermosphere. This white paper discusses the science motivation for gathering this fundamental knowledge which motivates new missions with satellites and sounding rockets.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-b6e81ea1d45b0b6e0b680ae31e5595cc_PfaffRobertF1.pdf"
"369","7 September 2022 6:54:22 pm","Peter","Chi","0000-0002-3739-6956","University of California Los Angeles","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-1599779f7ad64e2decb0ffa6430cb4c3_SSPH_White_Paper_Author_Information_Form_-_ChiPeterJ.xlsx","Basic Research","Planetary Magnetospheres","","","","","","","","","Ground-based;Space-based","Magnetoseismology in a New Era of Magnetospheric Research","Magnetoseismology consists of field line resonance sounding and travel time inversion, two unconventional methods of investigating the plasma mass density and impulsive phenomena in the magnetosphere. This white paper summarizes major outstanding science questions and technical hurdles in magnetoseismology, and recommends strategies in observations, modeling, and data analysis approaches.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-43f0a3bdfd74a430ba454b442bd12cdd_ChiPeterJ.pdf"
"370","7 September 2022 6:54:09 pm","Naoki","Bessho","0000-0002-5431-174X","University of Maryland, College Park; NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-2dd271a4c4b996df07e9dd55f678d97f_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Planetary Magnetospheres;Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","","Kinetic Physics Investigation of Magnetic Reconnection in the Heliosphere: Requirements for Simulations and Comparison with Space Measurements","Simulation research based on PIC and Vlasov codes and comparison with space measurements are essential to understand kinetic physics in various space environments. We discuss five kinetic topics about magnetic reconnection: collisionless resistivity and the reconnection rate, particle motion, 3D turbulence, wave-particle interactions, and studies of the Vlasov-Maxwell system.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-3cbe67091beef165dc5308824ef74d6a_BesshoNaoki.pdf"
"371","7 September 2022 6:55:26 pm","Elizabeth","MacDonald","0000-0002-3946-297X","NASA GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-cdf704cc7e4aa6a752729493508a61bb_MacDonaldElizabethA_Citizen_Science.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability;Other topic relevant to solar and space physics/heliophysics","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Science for all: The case for Citizen Science in all NASA missions","Heliophysics has a strong history of benefiting from citizen science that dates back to the 18th century & continues. However, we have only scratched the surface. With sustained funding & strategic leadership from NASA & NSF, crowdsourced science can help return further scientific gains in conjunction with satellite mission opportunities while keeping science accessible to the general public. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-ed499df1a26ad6e0f4482257d6371f6f_MacDonaldElizabethA-CitizenScienceSatelliteMissions.pdf"
"372","7 September 2022 6:57:48 pm","Michael","Henderson","0000-0003-4975-9029","Los Alamos National Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Other topic relevant to solar and space physics/heliophysics","","","","","","","","","Space-based","The Need for More Capable Space-Based Global Auroral Imagers","Fundamental questions concerning how auroral features are related to one another and to processes in the magnetosphere remain unclear. Limitations with past global auroral imagers are discussed. Critical open questions are summarized and types of next-generation more-capable global auroral imagers that can be used to answer these questions are discussed","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-2b3652dea61050c987c9c21175ad5fb0_WhitePaperAurora.pdf"
"373","7 September 2022 7:01:54 pm","Serena","Criscuoli","0000-0002-4525-9038","National Solar Observatory","Friedrich","Tetsu","Gianna","Adam","Haosheng","Woeger","Anan","Cauzzi","Kowalski","Lin","","0000-0001-6824-1108","0000-0002-6116-7301","0000-0001-7458-1176","","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","National Solar Observatory","National Solar Observatory","National Solar Obervatory","University of Colorado Boulder/National Solar Observatory","UH Institute for Astronomy","","Basic Research;Infrastructure, Workforce, Other Programmatic","Solar Physics","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","A NEAR-UV SPECTROGRAPH TO INVESTIGATE THE SOLAR ATMOSPHERE. A SECOND GENERATION INSTRUMENT FOR DKIST.","With this White Paper we make the case for a DKIST second-generation spectro-polarimeter that operates in the 300-400 nm spectral range, and lay out its high level scientific requirements. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-2689814028c364e22d4d19100b528d38_CriscuoliSerena2.pdf"
"374","7 September 2022 7:03:30 pm","Xin","Cao","0000-0003-0247-3584","LASP, University of Colorado Boulder","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-5f13c1f5256f8868d49bb14f3a8b4d33_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","","Science Return of Probing Magnetospheric Systems of Ice Giants","We discuss the science return of probing magnetospheric systems of ice giants for the future missions, over different magnetospheric regions, across from the interaction with upstream solar wind to the downstream region of magnetotail. We emphasize the importance of detecting the magnetospheres of ice giants , which enables us to deeply understand ice giants' space environment and habitability.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-d5be0812d52d7062df1f5ea616723455_CaoXin.pdf"
"375","7 September 2022 7:04:58 pm","Jeff","Klenzing","0000-0001-8321-6074","NASA / GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-889fbf1585a32ad388eb35d9d3e66a63_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","A system science perspective of the drivers of equatorial plasma bubbles","The complex drivers of equatorial plasma bubbles and resulting scintillation requires a system science approach spanning the M-ITM disciplines. The current roadmap missions strongly support this approach, but gaps are identified in planned observations, with potential mission and solutions proposed.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-30471a2feeaf2ad2d86fefee0a703386_KlenzingJeff.pdf"
"376","7 September 2022 7:13:01 pm","Jerry","Manweiler","0000-0002-8800-2128","Fundamental Technologies, LLC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-0942e816d6767a5853c754abd863e16a_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Space Weather Applications","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","Space Weather Pipeline from Research to Application to Operations;Other Space Weather","","","","","","Space-based","The Lagrange Communication and Advanced Realtime Space-weather (LCARS) Array","We explore the need and utility of the development of an array of spacecraft deployed at the Earth-Sun Lagrange points to enable three-dimensional (3D) space weather monitoring. We show that the utilization of all five Lagrange points is possible if each of the spacecraft are instrumented with modern high-bandwidth terahertz communication systems. We designate this network as the SOL-Network","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-8efa6a5357185c08283f2acc90ad192c_ManweilerJerryW.pdf"
"377","7 September 2022 7:06:54 pm","Sarah","Gibson","0000-0001-9831-2640","NCAR/HAO","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-84017bda24d98135978eccffe9649188_GibsonSarahEAuthors.xlsx","Basic Research","Solar Physics;Basic research that is driven by space weather user needs","","","","","","","","","Ground-based;Space-based","Coronal Polarimetry: Determining the Magnetic Origins of Coronal Mass Ejections","The mechanism for the release of stored magnetic energy in solar eruptions remains a major unsolved problem of Heliophysics. Choosing between triggers requires knowledge of pre-eruptive magnetic fields. Current coronal observations are insufficient to diagnose 3D coronal magnetic fields in CME precursors, motivating recommendations for new capabilities in next-generation V/IR and UV telescopes.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-d1f811885119f00bf96407c0991e5e46_GibsonSarahE.pdf"
"378","7 September 2022 7:07:23 pm","Steven","Petrinec","0000-0002-0329-7087","Lockheed Martin Space","Joseph","","","","","Mobilia","","","","","","","","","","[email protected]","","","","","Lockheed Martin Space","","","","","","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","Space Weather Research to Operations to Research Loop","","","","","","Space-based","Auroral Imaging Suite (AIS)","The Auroral Instrument Suite comprises two satellites, providing continuous multiple wavelength measurements of the entire Earth's northern auroral region. Auroral emissions provide quantitative measures of energy and particle deposition into the ionosphere, associated with changes in conductivity and large-scale currents. Such knowledge of auroral activity changes provides actionable information.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-d5574ff996a569c8b45778fc41e2b5e3_PetrinecStevenM.pdf"
"379","7 September 2022 7:29:21 pm","Mark","Conde","https://orcid.org/0000-0003-4924-878X","Geophysical Institute, University of Alaska Fairbanks","Donald","Miguel","Stephen","","","Hampton","Larsen","Kaeppler","","","","","","","","[email protected]","[email protected]","[email protected]","","","Geophysical Institute, University of Alaska Fairbanks","Dept of Physics & Astronomy, Clemson University","Dept of Physics & Astronomy, Clemson University","","","","Basic Research","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Ground-based;Space-based","Absolute Measurements of Neutral Winds and Ion Drifts in Earth’s Mesosphere and Thermosphere","Weather above Earth's mesopause is observed to be more dynamic than expected from theory. To understand this will require measurements that are sampled locally and derived with absolute accuracy - which is best achieved by tracking chemical tracer clouds deployed using a sounding rocket. We encourage NASA to take steps to ensure that expertise with this technique is preserved, or even expanded.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-6b4e48e002fb192d8b962afa867aefdc_CondeMarkG2.pdf"
"380","7 September 2022 7:32:41 pm","Lindsay","Goodwin","0000-0001-5302-7889","New Jersey Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-d0559eda74c8b4d5ab13da2d5c4f283b_GoodwinLindsayV2_co-authors.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Ground-based assets to support the GDC mission","A key element for the success of GDC is the preparation and coordination of our ground-base assets. This white paper presents an overview of some of these ground-based capabilities and recommends: 1) maintaining continuous support for our existing ground-based assets, 2) increasing coverage of inexpensive proven technologies, and 3) improving support for new remote sensing technologies.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-1e0116ae0194c37d1573192da5a209bd_GoodwinLindsayV2.pdf"
"381","7 September 2022 7:33:01 pm","Vladimir","Airapetian","0000-0003-4452-0588","NASA GSFC/SEEC and American University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-ab560f91f12f56436eb94eadfaa45d44_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics;Other topic relevant to solar and space physics/heliophysics","","","","","","","","","Ground-based;Space-based","Expanding The Frontiers: From The Solar Corona and The Wind to Evolving Space Weather of Planet Hosting Stars","We describe the knowledge gaps in understanding outputs of planet hosting stars in the space between host stars and their rocky exoplanets as a crucial component of habitability and provide recommendations for the development of heliophysics models and their extension to describe stellar environments.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-f4c973e8bc165475c010d0951349d347_AirapetianVladimirS.pdf"
"383","7 September 2022 7:40:38 pm","Michael","Plumaris","0000-0003-3260-9438","Sapienza University of Rome","Fabrizio","Cascioli","Iess","","","De Marchi","Gael","Luciano","","","","","","","","[email protected]","[email protected]","[email protected]","","","Sapienza University of Rome","University of Maryland Baltimore County","Sapienza University of Rome","","","","Basic Research","Other topic relevant to solar and space physics/heliophysics","","","","","","","","","Ground-based;Space-based","Testing theories of gravitation with the Interstellar Probe Radio Experiment","Simulating the radioscience experiment for the Interstellar Probe mission concept to test General Relativity at unprecedented scales","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-847b80c7f2a3ef60188dc3baa94879c9_PlumarisMichael.pdf"
"384","7 September 2022 8:07:40 pm","Lindsay","Goodwin","0000-0001-5302-7889","New Jersey Institute of Technology","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-a800493c0aa567c697ec8fad99ca4bd7_GoodwinLindsayV2_co-authors.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Ground-based assets to support the GDC mission","A key element for the success of GDC is the preparation and coordination of our ground-base assets. This white paper presents an overview of some of these ground-based capabilities and recommends: 1) maintaining continuous support for our existing ground-based assets, 2) increasing coverage of inexpensive proven technologies, and 3) improving support for new remote sensing technologies.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-24b743cfeef32c791b69bdced871bd4c_GoodwinLindsayV2.pdf"
"386","7 September 2022 7:54:08 pm","Philip","Fernandes","0000-0002-3432-8624","Los Alamos National Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-ac3ec8063d3b2340e55ac99c73dab7ef_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","","","","","","","","Heavy Ions: A Critical Measurement for Understanding the Solar Wind/Ionosphere/Magnetosphere System","The typical on-orbit mass spectrometer is limited in mass resolution capability, such that it cannot distinguish N+ from O+ by design. We propose a community goal of characterizing the full complement of plasma species (composition and charge state) within the Solar Wind/Magnetosphere/Ionosphere system to understand how these populations interact with one another and impact the system as a whole.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-b5f7d495001c7a9ab9aa048a2e2c9e89_FernandesPhilipA.pdf"
"387","7 September 2022 7:54:44 pm","Noé","Lugaz","0000-0002-1890-6156","University of New Hampshire","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-47cd3ab8a41f0205b1a95e068e810541_SSPH__WkLfBalance_author_list_full.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","Work-Life Balance Starts with Proper Deadlines and Exemplary Agencies","The entire Heliophysics research system hinders/ discourages proper work-life balance. A core issue stems from the culture of ""work-above-life"" associated with mission development and implementation but also the expectations that seem to originate from announcements by agencies. We are calling for work-life balance plans and implementation to be a criterion used for mission down-selection. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-1599b680a9c6d405531c9f29ca814ced_LugazNoe3.pdf"
"388","7 September 2022 7:59:27 pm","Megan N.","Kenny","0000-0002-2390-5932","University of Colorado, Boulder, Southwest Research Institute","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-7420987a1521b8474d452e355cffb183_SSPH_White_Paper_Author_Information_Form.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","Gender Diversity in Heliophysics","Gender diversity in the field of heliophysics is severely lacking, to the detriment of all members of the field. We describe the current state of the profession through a collective lens of trans and nonbinary heliophysicists. We make recommendations on ways to build resources, opportunities, and practices that seek to welcome, uplift, and retain gender-expansive persons in our field.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-ea24429b3f9fa1bfecbe9c9ae5ded2c1_KennyMeganN.pdf"
"389","7 September 2022 7:59:26 pm","Noé","Lugaz","0000-0002-1890-6156","University of New Hampshire","Rob","Nada","","","","Lillis","Al-Haddad","","","","0000-0003-0578-517X","0000-0002-0973-2027","","","","[email protected]","[email protected]","","","","University of California-Berkeley","University of New Hampshire","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Other Programmatic","","","Space-based","Importance of a Small, Innovative Missions for Heliophysics Exploration (SIMHEX) program and of continuation of the Explorer selection increase.","This WP argues that 1) that there is a need for a Small, Innovative Missions for Heliophysics Exploration (SIMHEX) program within the Heliophysics division which would be similar in spirit to the Planetary SIMPLEX program, and that 2) the Heliophysics division should continue its program of expanding and accelerating the Explorer selections, one of the top priorities of the 2012 Decadal survey. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-b9bdeb78f48feb31d4e3a86a59d78e70_LugazNoe4.pdf"
"390","7 September 2022 7:59:37 pm","Brett","Isham","0000-0002-9451-690X","Interamerican University of Puerto Rico, Bayamón, Puerto Rico","Christiano","Jason","","","","Brum","Kooi","","","","0000-0001-6515-7621","0000-0002-5595-2522","","","","[email protected]","[email protected]","","","","Arecibo Observatory, University of Central Florida, Arecibo, Puerto Rico","U.S. Naval Research Laboratory, Washington, DC","","","","","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Fundamental space plasma theory (not specific to a particular region)","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Design Concepts for a New Arecibo Radar and Radio Telescope","We present a plan for a new Arecibo instrument capable of observing all the layers of the atmosphere and geospace with multi-scale high-resolution vector measurements, extending measurements to the plasmapause and beyond, observing high-resolution interplanetary scintillation, and opening a new radar window on coronal mass ejections, the solar corona, and perhaps elsewhere in the heliosphere. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-f946396241e239f31c39e6ac4b7d4dd1_IshamBrettC1.pdf"
"391","7 September 2022 8:01:45 pm","Olusegun","Jonah","0000-0002-8280-8657","SRI International","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-9eb36006b089a8e33c7a03c7f1d0679e_SSPHWhitePaperAuthorInformationForm.xlsx","Space Weather Applications;Infrastructure, Workforce, Other Programmatic","","","","Space Weather Pipeline from Research to Application to Operations;Other Space Weather","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","Ground-based","Need for COntinuous Network of GNSS Receivers over North Africa (CONGA)","This paper stipulates the importance and benefit of improved continuous network GNSS receivers over North Africa region. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-45919af9d0e75bef54b95180227cbb2b_JonahOlusegunF.pdf"
"392","7 September 2022 8:02:05 pm","Stacey","Sueoka","0000-0003-0838-6588","National Solar Observatory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-ad24c487d5c45e82cd6a5c3b5dddd3b2_SSPHWhitePaperAuthorInformationForm_Sueoka.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","Investment in people is essential to sustain a diverse and engaged workforce","The field of heliophysics is a vibrant, multi-disciplinary endeavor that is dependent on the skills of a wide range of professionals. Supporting all employees across the entire field, not just those in scientific positions, is vital for the ongoing success and vibrancy of the field. In this paper, we have delineated a number of recommendations that can be pursued by Federal Agencies.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-44b2c7865893fefb1787fd0660c4f651_SueokaStaceyR.docx"
"393","7 September 2022 8:03:00 pm","Brett","Isham","0000-0002-9451-690X","Interamerican University of Puerto Rico, Bayamón, Puerto Rico","Christiano","Jason","","","","Brum","Kooi","","","","0000-0001-6515-7621","0000-0002-5595-2522","","","","[email protected]","[email protected]","","","","Arecibo Observatory, University of Central Florida, Arecibo, Puerto Rico","U.S. Naval Research Laboratory, Washington, DC","","","","","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Fundamental space plasma theory (not specific to a particular region)","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Science Goals for a New Arecibo Observatory","Science goals for a new and more capable Arecibo radar and radio telescope are presented, in aeronomy and geospace science, experimental plasma and radio physics, and heliospheric science. A new Arecibo could also provide support for a variety of scientific and technology development projects. A companion white paper focuses on the design of a new telescope.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-730af3d174fd88daf8003877416f7e21_IshamBrettC2.pdf"
"394","7 September 2022 8:15:22 pm","Brett","Isham","0000-0002-9451-690X","Interamerican University of Puerto Rico, Bayamón, Puerto Rico","Jason","Namir","Joseph","Wlodek","","Kooi","Kassim","Helmboldt","Kofman","","0000-0002-5595-2522","0000-0001-8035-4906","0000-0002-2123-0441","0000-0002-6744-8796","","[email protected]","[email protected]","[email protected]","[email protected]","","U.S. Naval Research Laboratory, Washington, DC","U.S. Naval Research Laboratory, Washington, DC","U.S. Naval Research Laboratory, Washington, DC","Institute of Planetology and Astrophysics of Grenoble, Grenoble, France, and Space Research Center of the Polish Academy of Sciences, Warsaw, Poland","","","Basic Research;Infrastructure, Workforce, Other Programmatic","Solar Physics;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","An Advanced Low-Band VHF Geospace and Heliospheric Radar: Design and Technology","The construction of a multistatic, imaging, low-band VHF (20-80 MHz) atmospheric, geospace, and heliospheric radar should include high continuous transmitter power, multiple large receiving arrays at widely-separated sites for 3-D velocity measurements and radar imaging, frequency agility for observations at multiple scale lengths, and wide bandwidth for high range resolution. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-6a7a2c021114ebadd8febc0cda361b70_IshamBrettC3.pdf"
"395","7 September 2022 8:05:53 pm","Friedrich","Woeger","0000-0001-6907-9739","National Solar Observatory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-df02bcff3850247bc2dda5c526ed0229_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","Solar Physics","","","","","","","","","Ground-based","Staying at the Forefront of Scientific Discovery with 2nd Generation DKIST Instrumentation","Long term delivery of high-quality data to the solar physics community requires a continuous effort of maintaining, enhancing, and upgrading DKIST's existing instruments, and eventually commissioning new instruments. We are advocating for operations funding for a program for maintenance and upgrades, and supplemental funded major new instruments selected with help of the solar physics community.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-6e294a60a1a6f7efd6c8c001cc153efb_WoegerFriedrich.docx"
"396","7 September 2022 8:07:28 pm","Hsiang-Wen","Hsu","0000-0002-5478-4168","University of Colorado Boulder","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-c879a046f9f7c720c0cf839cfd5d79b0_HsuHsiangWenCoAuthor.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","In Situ Cosmic Dust Detection for Heliophysics","We discuss a suite of instruments cable of carrying out the next generation of in situ cosmic dust measurements from the heliosphere into interstellar space to provide compositional and dynamical information of interstellar dust and interplanetary dust particle populations in support of the Interstellar Probe mission concept.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-d706ecfac38129d268db14abd9dc43cc_HsuHsiangWen.pdf"
"397","7 September 2022 8:08:14 pm","Sushanta C","Tripathy","0000-0002-4495-6180","National Solar Observatory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-a246dca6316fb7513829fb9f85e09371_TripathySushantaCauthorinformationForm.xlsx","Basic Research","Solar Physics","","","","","","","","","Ground-based","Improving the Understanding of Subsurface Structure and Dynamics of Solar Active Regions","Three-dimensional mapping of the structure and dynamics of sunspots and active regions below the photosphere are among the long standing and intriguing puzzles in solar physics. In order to make substantial progress in this field, we are advocating full disk, simultaneous Doppler and vector magnetic field observations at different heights of the solar atmosphere. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-d42c7225edc73108b1a50c525f1f4747_TripathySushantaC.pdf"
"398","7 September 2022 8:19:12 pm","Asti","Bhatt","0000-0002-8881-5348","SRI International","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-cbeff45e1f0e040b3b28073c921ad389_SSPH_White_Paper_Author_Information_Form_multiscale.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","Research Tools and Infrastructure (that is not specific to one research area);Other Programmatic","","","Ground-based","Multi-scale geospace research with networks of distributed, homogeneous instruments","Understanding the effects of multiple scales in the dynamics of the mesosphere, ionosphere, and thermosphere (MIT) regions and their interactions remains a key challenge in geospace science. This white paper makes the case for building new and maintaining existing networks of homogeneous instruments in order to sample various scale sizes across large distances. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-85348d1f0bb1527a012bcf4aa431f03f_BhattAstiA1.pdf"
"399","7 September 2022 8:21:43 pm","Brett","Isham","0000-0002-9451-690X","Interamerican University of Puerto Rico, Bayamón, Puerto Rico","Jason","Namir","Joseph","Wlodek","","Kooi","Kassim","Helmboldt","Kofman","","0000-0002-5595-2522","0000-0001-8035-4906","0000-0002-2123-0441","0000-0002-6744-8796","","[email protected]","[email protected]","[email protected]","[email protected]","","U.S. Naval Research Laboratory, Washington, DC","U.S. Naval Research Laboratory, Washington, DC","U.S. Naval Research Laboratory, Washington, DC","Institute of Planetology and Astrophysics of Grenoble, Grenoble, France, and Space Research Center of the Polish Academy of Sciences, Warsaw, Poland","","","Basic Research;Infrastructure, Workforce, Other Programmatic","Solar Physics;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","An Advanced Low-Band VHF Radar for Atmospheric, Geospace, and Solar Research","The construction of a multistatic, imaging, low-band VHF (20-80 MHz) radar observatory would allow high-resolution vector measurements of incoherent scatter from the ionosphere and coherent scatter from the neutral atmosphere through the plasmasphere, and would change the nature of what can be observed. Paired with a powerful transmitter, radar measurements of the sun would also be possible. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-42fdad69c708fcb479368445732efaa7_IshamBrettC4.pdf"
"401","7 September 2022 8:30:47 pm","Brett","Isham","0000-0002-9451-690X","Interamerican University of Puerto Rico, Bayamón, Puerto Rico","Jason","Namir","Joseph","","","Kooi","Kassim","Helmboldt","","","0000-0002-5595-2522","0000-0001-8035-4906","0000-0002-2123-0441","","","[email protected]","[email protected]","[email protected]","","","U.S. Naval Research Laboratory, Washington, DC","U.S. Naval Research Laboratory, Washington, DC","U.S. Naval Research Laboratory, Washington, DC","","","","Basic Research;Infrastructure, Workforce, Other Programmatic","Solar Physics;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Solar Research Using an Advanced VHF Heliospheric Radar","A powerful low-band VHF (20-80 MHz) radar will enable renewed radar measurements of the sun. Solar radar will be a game changer for solar physics research, including studies of the micro and macrophysics of the corona, and would improve space weather prediction and monitoring, allowing early warning of earth-directed coronal mass ejections, which are important drivers of space weather. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-3cb9e9382a74c6b2ed9b43bdfa932de1_IshamBrettC5.pdf"
"403","7 September 2022 8:35:45 pm","Ayumi","Asai","0000-0002-5279-686X","Kyoto University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-ed6c5ba7d50ea9de2bc87498ac76c74d_SSPHWhitePaperAuthorInformationForm_NIRTF_Asai.xlsx","Basic Research;Space Weather Applications","Solar Physics","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Ground-based","Infrared Imaging Spectropolarimetry of the Solar Chromosphere and Corona with DKIST","We describe the importance of imaging spectroscopy, based on a tunable filter approach, for addressing key science goals of the solar physics community in studying the thermodynamics and magnetic field of the chromosphere and corona. We outline some basic requirements for such an instrument and identify some possible technical approaches.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-efbb87e9206de55187cd3add40fe2a7f_NIRTF.for.DKIST_WPHeliophysics2024.pdf"
"404","7 September 2022 8:39:28 pm","Brett","Isham","0000-0002-9451-690X","Interamerican University of Puerto Rico, Bayamón, Puerto Rico","Terence","Björn","Emil","Christiano","","Bullett","Gustavsson","Polisensky","Brum","","0000-0001-9256-6105","0000-0002-0868-7308","0000-0003-3272-9237","0000-0001-6515-7621","","[email protected]","[email protected]","[email protected]","[email protected]","","University of Colorado, Boulder, Colorado","University of Tromsø, Tromsø, Norway","U.S. Naval Research Laboratory, Washington, DC","Arecibo Observatory, University of Central Florida, Arecibo, Puerto Rico","","","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres;Fundamental space plasma theory (not specific to a particular region)","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Technical Design of a High-Frequency Antenna Array for Radar and Radio Imaging of the Ionosphere","We are developing a 2 to 25 MHz antenna array for radar and radio imaging of the ionosphere. The main array will be located near Arecibo in Puerto Rico, and will include 64 active crossed antenna elements within a 400-meter-diameter area. Relocatable antenna elements will also be included, with phase maintained through the use of GPS-disciplined rubidium clocks. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-90b87dee4beeb361a002da1134fa5db9_IshamBrettC6.pdf"
"405","7 September 2022 8:41:03 pm","Zhonghua","Xu","0000-0002-3800-2162","Virginia Tech","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-8c2a77d8fc962405995ae9f4124ed958_Interhemispheric_asymmetries_White_Paper_Authors.xlsx","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Ground-based;Space-based","A Strategic Vision for Understanding Inter-Hemispheric Asymmetries","Models for space weather forecasting will never be complete/valid without accounting for inter-hemispheric asymmetries in Earth's magnetosphere, ionosphere and thermosphere. This whitepaper is a strategic vision for understanding these asymmetries from a global perspective of geospace research and space weather monitoring, including current states, future challenges, and potential solutions.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-80ecf8613753f74fa0c2f40b67a39e54_XuZhonghua.pdf"
"406","7 September 2022 8:44:04 pm","Brett","Isham","0000-0002-9451-690X","Interamerican University of Puerto Rico, Bayamón, Puerto Rico","Terence","Björn","Emil","Christiano","","Bullett","Gustavsson","Polisensky","Brum","","0000-0001-9256-6105","0000-0002-0868-7308","0000-0003-3272-9237","0000-0001-6515-7621","","[email protected]","[email protected]","[email protected]","[email protected]","","University of Colorado, Boulder, Colorado","University of Tromsø, Tromsø, Norway","U.S. Naval Research Laboratory, Washington, DC","Arecibo Observatory, University of Central Florida, Arecibo, Puerto Rico","","","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres;Fundamental space plasma theory (not specific to a particular region)","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Science Goals for a High-Frequency Radar and Radio Imaging Array","Science goals for a large 2 to 25-MHz radio and radar imaging array include the study of space weather, ionospheric structure and dynamics, meteors, lightning, radio propagation, and plasma physics, including stimulated ionospheric radio emissions, such as those induced by the Arecibo Observatory high-power HF radio transmitter, which is likely to be restored to operation in the near future. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-e4e1c285b06f78d8c875145ebb31e5bd_IshamBrettC7.pdf"
"407","7 September 2022 8:44:34 pm","Joan","Burkepile","0000-0002-9959-6048","National Center for Atmospheric Research","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-56443125a7290e6a87daba77f6b71574_BurkepileJoan_SSPH_White_Paper_Author_Information_Form.xlsx","Space Weather Applications","","","","Other Space Weather","","","","","","Ground-based;Space-based","Observations for Improving SEP Forecasts and Warnings","This paper demonstrates the importance of having near-real-time low corona CME observations, 0.05 to 0.4 nm solar flare emission, low frequency radio emissions, relativistic electron intensities from L4, and high-quality energetic proton measurements from the SEL line and L4. The availability of these data in near-real-time can increase SEP warning times and improve SEP predictions. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-e4637c303c1b15d333362072d6ff0779_BurkepileJoan.pdf"
"408","7 September 2022 8:46:46 pm","Adam","Kobelski","0000-0002-4691-1729","NASA Marshall Space Flight Center","Alfred","Laurel","Bart","David","Valentin","De Wijn","Rachmeler","De Pontieu","McKenzie","Martinez-Pillet","0000-0002-5084-4661","0000-0002-3770-009X","0000-0002-8370-952X","0000-0002-9921-7757","0000-0001-7764-6895","[email protected]","[email protected]","[email protected]","Decadal Survey for Solar and Space Physics (Heliophysics) 2024-2033: White Paper Author Information Form Please fill in as much information as you have available about the authors of your submission. If you are viewing a read-only copy of this spreadsheet online, click ""File"" then ""Save As"" to save and edit a local copy. Leave unknown or inapplicable cells blank — do not use ""N/A"", ""Unknown"", etc. For ""authors"" that are collaborations or other non-persons, please fill the entire name in the ""Family name(s)"" field. Use as many columns as needed to provide affiliations for each author. Do not delete the example or otherwise rearrange the cells. Resizing is OK. Example Given name(s) Family name(s) ORCID iD Email Affiliation 1 Affiliation 2 More affiliations ... Author 1 J. R. R. Tolkien 0000-0000-0000-0000 [email protected] University of Leeds Author 2 Daphne du Maurier 0000-0000-0000-0000 [email protected] University of Exeter Manderley Estate Author 3 The LIGO Collaboration Author 4 Martin Luther King, Jr. 0000-0000-0000-0000 Boston University Southern Christian Leadership Conference Your Submission Given name(s) Family name(s) ORCID iD Email Affiliation 1 Affiliation 2 More affiliations ... Author 1 Adam Kobelski 0000-0002-4691-1729 [email protected] NASA Marshall Space Flight Center (no need to fill this column) Alfred De Wijn 0000-0002-5084-4661 [email protected] National Center for Atmospheric Research, High Altitude Observatory Laurel Rachmeler 0000-0002-3770-009X [email protected] National Oceanic and Atmospheric Administration Bart De Pontieu 0000-0002-8370-952X [email protected] Lockheed Martin Solar and Astrophysics Laboratory David McKenzie 0000-0002-9921-7757 [email protected] NASA Marshall Space Flight Center Valentin Martinez-Pillet 0000-0001-7764-6895 [email protected] National Solar Observatory [email protected]","[email protected]","[email protected]","National Oceanic and Atmospheric Administration","Lockheed Martin Solar and Astrophysics Laboratory","NASA Marshall Space Flight Center","National Solar Observatory","","Basic Research;Space Weather Applications","Solar Physics;Other topic relevant to solar and space physics/heliophysics","","","Other Space Weather","","","","","","Ground-based;Space-based","Needed Measurements of Chromospheric Magnetic Fields","Regular multi-height measurements of the magnetic field of the chromosphere are crucial for understanding the solar atmosphere and the flow of energy between the photosphere and corona. We recommend a continued focus on the study of chromospheric magnetism through modeling and an increased investment in instrumentation as well as tools to interpret those observations","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-debed8851c99cf99371649d5d5565da7_KobelskiAdamR.pdf"
"409","7 September 2022 8:47:26 pm","Michael","Liemohn","0000-0002-7039-2631","University of Michigan","Jörg-Micha","Raluca","Natalia","Daniel","","Jahn","Ilie","Ganushkina","Welling","","","","","","","[email protected]","[email protected]","[email protected]","[email protected]","","Southwest Research Institute","University of Illinois","University of Michigan","University of Michigan","","","Basic Research","Planetary Magnetospheres;Planetary ionospheres/upper atmospheres","","","","","","","","","Space-based","Science Case for a Global Ionospheric Outflow Mission","A mission is needed to observe the spatial pattern of ionospheric outflow and its relation to geospace driving conditions. Initial cost estimates suggest that such a mission could be achieved within the constraints of the Small Explorer mission line with minimal instrumentation (i.e., only low-energy ions), or at the Mid-sized Explorer line with additional contextual measurements.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-b1d82836668144b2131c9a67afaf243b_Science_Case_for_a_Global_Ionospheric_Outflow_Mission_v3.pdf"
"410","7 September 2022 8:49:52 pm","Errol","Summerlin","","NASA, GSFC","Marta","Antti","Brent","","","Shelton","Pulkkinen","Randol","","","","","","","","[email protected]","[email protected]","[email protected]","","","NASA, GSFC","NASA, GSFC","NASA, GSFC","","","","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Space-based","CATSCaNS: Co-Axial Tomography of the Solar Corona and Near Sun environment","CATSCaNS is a mission concept that seeks to revolutionize our understanding of CMES by resolving the internal structure of CMEs with tomographic imaging taken from multiple deep space small sats. Advances in miniature coronagraphs and other instruments as well as advances in small sat laser communications systems make this concept eminently feasible in the coming decade.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-50e0b111c29d7b2682e7685762be2657_CATSCANS_White_paper_final_v2.pdf"
"411","7 September 2022 8:52:58 pm","Larisa","Goncharenko","0000-0001-9031-7439","MIT Haystack Observatory","Han-Li","Jorge","Gunter","Eswaraiah","Nikolay","Liu","Chau","Stober","Sunkara","Zabotin","0000-0002-6370-0704","0000-0002-2364-8892","0000-0002-7909-6345","0000-0002-0419-6755","0000-0003-0715-1082","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","HAO NCAR","Leibniz Institute of Atmospheric Physics at the University of Rostock","University of Bern","Madanapalle Institute of Technology and Science","University of Colorado Boulder","","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Importance of the semidiurnal tide, and future measurements needed to improve its characterization","Observations of semidiurnal tides are critically needed to advance understanding of interactions between the lower and upper atmosphere. Many factors about these interactions remain unknown due to the lack of observations at altitudes between 90-200 km. We propose to invest in ground-based infrastructure, implement DYNAMIC-like mission, and strengthen inter-division and inter-agency links","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-3e594f8c11c76e735bd47918e693b8ba_GoncharenkoLarisaP.pdf"
"413","7 September 2022 9:04:11 pm","Zishun","Qiao","0000-0001-6900-7313","Embry-Riddle Aeronautical University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-da036e729425023f50448e5968f6a983_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Infrastructure needs on latitudinal and longitudinal chains of co-located ground-based observations","This white paper discusses the significance and potential of coordinating a chain of ground-based instruments with the current large facilities to extend the latitudinal and longitudinal observational coverage in the American sector. We further discuss the benefits of co-locating heterogeneous instruments with different techniques and different temporal/spatial resolution/coverage.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-ad8e47976d7ea0fe3abe2229a10dd01e_QiaoZishun.pdf"
"414","7 September 2022 9:05:25 pm","Robert","Arritt","","Electric Power Research Institute","Jennifer","","","","","Gannon","","","","","","","","","","[email protected]","","","","","Computational Physics, Inc","","","","","","Space Weather Applications","","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Ground-based","GICs from the End User Perspective","The opinion of the technical community is that there are not enough magnetometers in the CONUS to properly inform GIC hazard analyses and industry reliability standards (e.g. NERC TPL-007). ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-d3973d2d21b48bdfba34138f9054fd9b_GICs_from_the_End_User_Perspective_5-12-2022.docx"
"415","7 September 2022 9:09:43 pm","Leslie","Lamarche","0000-0001-7098-0524","SRI International","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-ddcdcd7ea46ca4cf79bca1c7cbe7ca21_AuthorInformationForm.xlsx","Basic Research","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","","Polar Cap Science: Plasma Structuring","Discuss plasma structuring in the polar cap, the mechanisms that contribute to it, and open questions.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-1e4a83bf7c685283c7dc90ee802949ae_LamarcheLeslieJ1.pdf"
"416","7 September 2022 9:12:20 pm","Veerle","Sterken","0000-0003-0843-7912","ETH Zürich","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-6a1317abf7e245f3d054ec5f82fe44c5_SSPH_White_Paper_Author_Information_Form_Sterken_ISP.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Outer Heliosphere;Other topic relevant to solar and space physics/heliophysics","","","","","","Other Programmatic","","","Ground-based;Space-based","Synergies between interstellar dust and heliospheric science with an Interstellar Probe","We focus on the synergies between heliosphere and dust science and illustrate how to use interstellar dust (ISD) in the solar system as a tracer for the (dynamic) heliosphere properties. We discuss the potential role of cosmic dust in heliospheric physics. An Interstellar Probe with dust suite would bring great advances to ISD research, and can contribute, through the dust, to heliosphere science.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-f67110be0aefc1c031687fc862ad1584_SterkenVeerleJ.pdf"
"417","7 September 2022 9:22:01 pm","Jaye L.","Verniero","0000-0003-1138-652X","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-1469aaa4f2369b7a0ef5a0e71339c647_SSPH_White_Paper_Author_Information_Form_%25281%2529.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Guiding Heliophysics Toward an Enhanced Transdisciplinary Framework","The inherent interdisciplinary nature of heliophysics attracts minds of diverse skill sets. However, the current funding infrastructure is built for siloed research groups and incremental projects. We review the present landscape and make recommendations toward a transdisciplinary framework enabling enhanced creativity and increased likelihood of scientific breakthroughs. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-de6cc7024bb79b823bcd56b79f9ef9ec_VernieroJayeL.pdf"
"418","7 September 2022 9:24:42 pm","John","Cooper","0000-0003-4832-7320","NASA GSFC Emeritus Code 672 Heliospheric Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-6589c83e6c95e6462f146b447780725d_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","Space-based","Heliophysics from, by, and of the Moon in the Age of Artemis: Lunar Solar Occultation Explorer (LunaSOX)","The present decade and beyond of the NASA Artemis human exploration program will offer abundant opportunities for heliophysics investigations from the vantage points of lunar orbit and the surface. The Lunar Solar Occultation Explorer concept uses the lunar limb to occult the solar disk for high-resolution coronal observations at hourly to daily to monthly cadence from orbit or the lunar surface.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-65ec6236e9bdcfe78de8b5f9c347e8c2_CooperJohnF.pdf"
"419","7 September 2022 9:26:47 pm","Kyung-Suk","Cho","0000-0003-2161-9606","Korea Astronomy & Space Science Institute","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-00558d64c8495fc52449a547b59d372d_KASItoAuthors_09.06.xlsx","Space Weather Applications","","","","Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","Space-based","Open New Horizon with L4 Mission","The L4 mission will significantly contribute advancing heliophysics science, improving the capability of space weather forecasting, and extending space weather studies far beyond near-Earth space. This white paper outlines the importance of L4 observations and advocates comprehensive and coordinated observations of the heliosphere at multi-points including other planned L1 and L5 missions. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-51b526e9d7d16f8bd6d2f4eaad537cd1_white_paper_Korea_final.pdf"
"420","7 September 2022 9:33:45 pm","Juliana","Vievering","0000-0002-7407-6740","Johns Hopkins Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-1a40d27ccb2b918c3ce05fc6e7f12a00_Solar-Stellar_Connection_White_Paper_Author_Information_Form_final.xlsx","Basic Research","Solar Physics;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","","High-Energy Aspects of the Solar-Stellar Connection","In this white paper, we demonstrate the scientific value of interdisciplinary research on high-energy solar/stellar activity. Such interdisciplinary research leverages the combination of spatially-resolved solar measurements with the variety of sources and extreme conditions from stellar observations to provide a more complete picture than either discipline could present on its own.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-90a320a90130f9b7254dfe986e2964b9_VieveringJulianaT2.pdf"
"421","7 September 2022 9:42:57 pm","Tibor","Torok","0000-0003-3843-3242","Predictive Science Inc.","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-45883bb21d87663fd22cf9f1fa532c2f_TorokTibor_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics","","","","","","","","","","Learn to Walk Before You Run: A Case for Fundamental CME Research Utilizing Idealized MHD Models","We discuss the importance of fundamental CME research, and the usefulness of idealized MHD models for it. To support such research, we recommend to (1) generally encourage/support fundamental research and simple modeling approaches, (2) establish a new, focused funding opportunity for such research in the field of heliophysics, and (3) foster collaboration with the plasma & stellar communities.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-5c86a9d07b70734e20cc6c51fc7f63c6_TorokTibor.pdf"
"422","7 September 2022 9:51:54 pm","Nicholeen","Viall","0000-0003-1692-1704","NASA Goddard Space Flight Center","Mihir","Raphael","Samantha","","","Desai","Attie","Wallace","","","0000-0002-7318-6008","0000-0003-4312-6298","0000-0002-1091-4688","","","[email protected]","[email protected]","[email protected]","","","Southwest Research Institute","NASA Goddard Space Flight Center/George Mason University","NASA Goddard Space Flight Center/NASA Postdoctoral Program","","","","Basic Research","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","","","","Space-based","Huygens Probes at the Sun","In order to solve the coronal heating problem and understand the formation of the solar wind, in situ, ground truth measurements must be made in the magnetically closed-corona. We envision Huygens Probes at the Sun: a series of expendable, small satellites that take in situ measurements in the closed-field corona, which are released from a parent spacecraft orbiting near to the Sun. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-fc17cf411dc8c20042d5d85a091ba50a_Huygens_Probes_at_the_Sun_V3.pdf"
"423","7 September 2022 9:53:35 pm","Li-Jen","Chen","0000-0002-4768-189X","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-00b8ff724615bc45b9187242ad415f0e_HelioSwarm_White_Paper_Author_Information_Form-final.xlsx","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Fundamental space plasma theory (not specific to a particular region)","","","Other Space Weather","","","","","","Space-based","Plasma turbulence: Challenges and next transformative steps from the perspective of multi-spacecraft measurements","We recommend to bring into reality the following within the next decade: 1. Measurements from multiple spacecraft covering a 3D volume and simultaneously spanning the MHD to kinetic scales (such as HelioSwarm). 2. Coordination of the new multi-scale mission(s) with existing multi-spacecraft missions such as MMS to maximize the power of cross-scale ion and electron measurements.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-46829ecd72c5991eca10a0de47b82183_ChenLiJen.pdf"
"424","7 September 2022 9:57:59 pm","Matthew E.","Hill","0000-0002-5674-4936","Johns Hopkins University Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-af43fb5b109a484c24b20319fa8d8284_Hill_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","Cosmic Rays Measurements on an Interstellar Probe: A Bold Approach to Concluding the Second Century of Space Aged Science","Flying a capable galactic cosmic ray (GCR) experiment on an Interstellar Probe (ISP) mission that launches around 2036 will provide the measurements needed to resolve the GCR puzzles by the end of the current century, cap-stoning ~200 years of cosmic ray science. The GCR experiment needs to be in the local interstellar medium, the one place where the uniquely revealing low-energy GCRs are found.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-905ac663385b35c568c75e240cbdd9fe_MatthewEHill.docx"
"425","7 September 2022 9:58:57 pm","Mary","Knapp","0000-0002-5318-7660","MIT Haystack Observatory, 99 Millstone Rd. Westford, MA 01886","John","Frank","Lenny","Erika","Allan","Swoboda","Lind","Paritsky","Palmerio","Weatherwax","0000-0003-2627-2031","0000-0002-9097-4380","","0000-0001-6590-3479","","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","MIT Haystack Observatory, 99 Millstone Rd. Westford, MA 01886","MIT Haystack Observatory, 99 Millstone Rd. Westford, MA 01886","MIT Haystack Observatory, 99 Millstone Rd. Westford, MA 01886","Predictive Science Inc., San Diego, CA 92121, USA","MIT Haystack Observatory, 99 Millstone Rd. Westford, MA 01886","","Basic Research;Space Weather Applications","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Planetary Magnetospheres","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","Space-based","SmallSat Constellations for Active and Passive Sensing in the Heliosphere","Constellations of spacecraft provide multi-point measurements that are valuable to heliophysics. Small spacecraft enable focused science investigations and are the basis for larger constellation missions at lower cost than traditional architectures. We describe the uniqueness of multi-spacecraft measurements enabled by small, inexpensive spacecraft and present three case study missions. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-ebbec994c351d29c972e96983329c4f4_KnappMaryE.pdf"
"426","7 September 2022 9:59:40 pm","Cesar","Valladares","0000-0001-6609-3236","University of Texas at Dallas","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop","","","","","","Ground-based;Space-based","Investigations of the initiation, lifetime, and effects of Equatorial Spread F","This document describes a comprehensive plan to investigate all different facets of the Equatorial Spread F (ESF) phenomena, formulate a series of questions, and devise a forecasting plan for ESF. It is indicated the need to understand the underlying physics of the low-latitude ionosphere and various instability mechanisms that operate near the equator. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-c68bc35b3337f1a09c6e943f0e0a202f_ValladaresCesarE.docx"
"427","7 September 2022 10:02:24 pm","Erich","Becker","0000-0001-7883-3254","NorthWest Research Associates","Rolando","Nicholas","Sharon","Valery","","Garcia","Pedatella","Vadas","Yudin","","0000-0002-6963-4592","0000-0002-8878-5126","0000-0002-6459-005X","0000-0002-9839-0750","","[email protected]","[email protected]","[email protected]","[email protected]","","NCAR","NCAR","NWRA","NASA/GSFC","","","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres","","","Space Weather Pipeline from Research to Application to Operations","","","","","","","Explicit simulation of gravity waves in whole atmosphere models","Current whole atmosphere models are limited regarding their ability to predict space weather disturbances caused by waves from below. This is largely because of insufficient representation of gravity waves (GWs). We describe some major requirements necessary for the explicit simulation of GWs and the associated multi-step vertical coupling in high-resolution whole-atmosphere models.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-6fd65040515715d03534615c8e8b4188_BeckerErich.pdf"
"428","7 September 2022 10:03:46 pm","Romina","Nikoukar","0000-0002-8608-2822","The Johns Hopkins University Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-738f5410090f1f3f23a88b8e4e2e3345_RominaNikoukar2-_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Other Space Weather","","","","","","","Novel Measurement Architectures Addressing Unresolved Issues Concerning Radio Wave Scintillation and Ionospheric Irregularities","Scintillation is a major space weather hazard that hinders radio communication and navigation. Despite this importance, critical questions concerning scintillation in relation to larger-scale ionospheric phenomena remain. We advocate for coordinated and simultaneous space and ground-based measurements of plasma and multi-frequency scintillation to determine the underlying physical processes. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-b6f2332252f206be02da74bdaa7a97d6_RominaNikoukar2.pdf"
"429","7 September 2022 10:06:27 pm","Matthew","Argall","0000-0001-6315-1613","University of New Hamsphire","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-b44532fb547ec05ffbb4403e9dc6edb9_ArgallMatthewR_Authorship.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Other topic relevant to solar and space physics/heliophysics","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Intelligent Missions in the Living Heliospheric System Observatory","This white paper outlines how we would like to see ML rise to the same level as Theory, Experiment, and Modeling within Heliophysics, particularly when it comes to PI-led mission design. We provide a vision of how the Heliophysics System Observatory can achieve these needs with suggestions of how to incorporate ML into ground and in-flight operations and to utilize past mission data. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-d3c581532c1e53ce20f34744a9cdbba3_ArgallMatthewR.pdf"
"430","7 September 2022 10:15:29 pm","Romina","Nikoukar","0000-0002-8608-2822","The Johns Hopkins University Applied Physics Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-cd44dd71c9a5b62d994596c2937e87b7_RominaNikoukar3-SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Other Space Weather","","","","","","","Next-Generation Ionosphere Radio Sensors Based on the Software-Defined Radio Platform","The advent of software-defined radio (SDR) platforms has opened new avenues for the easy-to-configure, low-SWaP beacon systems design suitable for small satellites and ground arrays. Next-generation SDR-based radio sensors with the deployment of a large constellation of small satellites allows for ionosphere imaging necessary for ionosphere specification and multi-frequency scintillation studies. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-9bda602e0225e91321e40cbce34deb23_RominaNikoukar3.pdf"
"431","7 September 2022 10:18:12 pm","Craig","DeForest","0000-0002-7164-2786","SwRI","Nicholeen","Yuhong","Sarah","Daniel","","Viall-Kepko","Fan","Gibson","Seaton","","0000-0003-1692-1704","0000-0003-1027-0795","0000-0001-9831-2640","0000-0002-0494-2025","","[email protected]","[email protected]","[email protected]","[email protected]","","NASA","UCAR","UCAR","SwRI","","","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop","","","","","","Space-based","CME Origins and Propagation: Importance of the Polar Perspective","Near-polar perspective imaging is critical to understanding CMEs, their onset, their interaction with the solar corona, and their propagation across the inner heliosphere. We highlight several areas that require polar imaging for advancement, and recommend measurements needed from a polar vantage to advance CME physics and the applied physics of space weather forecasting. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-240f83c8d6c86f65b445c9ea0f1ad758_Polar_CME_Imaging-2.pdf"
"432","7 September 2022 10:18:27 pm","Lisa","Upton","0000-0003-0621-4803","Southwest Research Institute","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-15b4a316b13fa68125d7082c840488c6_PolarFields_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Other Space Weather","","","","","","Space-based","Revealing the Sun’s Polar Magnetic Fields: The Key to Unlocking the Solar Activity Cycle","Solar polar missions to obtain precise, accurate, and comprehensive measurements of the polar magnetic fields are the essential next step for improving understanding of the dynamo and for advancing predictive capabilities on both short (Active Region evolution, flares, CMEs) and long (solar cycle) time scales.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-e5244155b64045b95e60748d0ce680d6_PolarFluxWhitePaper_Final.pdf"
"433","7 September 2022 10:19:01 pm","Edward","Thiemann","0000-0002-5305-9466","Laboratory for Atmospheric and Space Physics, University of Colorado at Boulder","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-b7fa361700c518d69e2ce2d34b0317d2_SSPH_White_Paper_Author_Information_Form_occultations.xlsx","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres","","","Space Weather Pipeline from Research to Application to Operations","","","","","","","Ultraviolet Occultations: An Essential Technique for Bridging the Thermospheric Gap","Solar and stellar ultraviolet occultations provide a capability essential for advancing our understanding of the thermosphere. Advances over the past decade have demonstrated the power of occultations for measuring density, temperature and waves. Additionally, occultation instruments are readily miniaturized, making them ideal candidates for space weather monitoring sensors. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-07e3095d78ccc2c6704ef8715986d881_ThiemannEdwardM.pdf"
"434","7 September 2022 10:19:06 pm","Douglas","Rowland","0000-0003-0948-6257","NASA GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Space-based","“Resolve” – leveraging commercial constellations with a mission to measure the global weather in the middle and upper atmosphere","""Resolve"" is a dense observation network of spaceborne sensors leveraging the commercial constellations of spacecraft to fully characterize the global-scale lower atmosphere forcing with spatial resolutions of 1000 km and timescales of one day or less. This will provide the first comprehensive picture of the complex and nonlinear interactions in this region.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-6b3cd5263ee88b1a9ed66935bf34cca6_RowlandDouglasE4.pdf"
"435","7 September 2022 10:19:52 pm","Ekaterina","Verner","","NASA/HQ/Heliophysics","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research;Infrastructure, Workforce, Other Programmatic","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Other topic relevant to solar and space physics/heliophysics","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion;Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Non Traditional Ways to Advance Science and Technology in Heliophysics","Can we advance research in Heliophysics, Space Weather, and technology in new ways? What is the best way to do it? Do we have the resources and infrastructure to do that? Open Innovation or Crowdsourcing platforms are very beneficial to bringing together a large number of people with all types of backgrounds, skills, and expertise. They provide unique opportunities, valuable products, and services. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-856a013e25a47cc0ffd144714ecdb6ea_VernerEkaterinaM.pdf"
"436","7 September 2022 10:24:47 pm","Raphael","Attie","0000-0003-4312-6298","NASA GSFC / George Mason University","Benoit","Michael","Pete","William, Dean","Lisa","Tremblay","Kirk","Schuck","Pesnell","Upton","0000-0002-5181-7913","0000-0001-9874-1429","","0000-0002-8306-2500","0000-0003-0621-4803","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","NSO","NASA GSFC","NASA GSFC","NASA GSFC","SWRI","","Basic Research","Solar Physics","","","","","","","","","Space-based","Quantifying the sun’s magnetic stress with the photospheric flows","This white paper presents research avenues to accurately quantify the magnetic stress that builds up free energy in the photosphere, and which heats up the corona. In particular, these capacities relate to our ability to track the photospheric flows accurately enough to resolve rotating motions that stress the magnetic field. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-024e4d121f329d8e817bbed6d0b5053c_AttieRaphael.pdf"
"438","7 September 2022 10:26:08 pm","Kiran","Jain","0000-0002-1905-1639","National Solar Observatory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-881f6a1d46dffdce29fa8e8c43772846_JainKiran_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop","","","","","","Ground-based;Space-based","Seismic Monitoring of the Sun’s Far Hemisphere: A Crucial Component in Future Space Weather Forecasting","We present a coherent vision for the role of helioseismic monitoring of magnetic activity in the Sun's far hemisphere that will contribute to improving space weather forecasting as well as fundamental research. These require reliable, continuous synoptic monitoring of the far hemisphere as an integral component of our science and technology infrastructure over the coming decade.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-69e4fb9c82ea46f1574c2b2eceed83be_JainKiran.pdf"
"439","7 September 2022 10:29:00 pm","William","Longley","0000-0002-8518-8633","Rice University","Lindsay","","","","","Goodwin","","","","","0000-0001-5302-7889","","","","","[email protected]","","","","","New Jersey Institute of Technology","","","","","","Basic Research","Fundamental space plasma theory (not specific to a particular region)","","","","","","","","","","Geospace: The naturally occurring plasma laboratory","This white paper argues for the merit in addressing space physics problems that are core to plasma physics, regardless of discipline or application. We recommend: 1) Consider plasma physics to be a fundamental science topic within space physics and therefore relevant to NASA investigations, and 2) annual solicitation of the NASA B.3 Heliophysics Theory, Modeling, and Simulations (HTMS) program.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-698e7b3139d2bf64b7890d18455986d3_LongleyWilliamJ.pdf"
"440","7 September 2022 10:33:05 pm","Mausumi","Dikpati","0000-0002-2227-0488","NCAR/HAO","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-b923e5c1183f768e471fde102a35be1b_Intermediate-scale_SW_--_SSPH_White_Paper_Author_Information_Form_Sept_7%252C2022.xlsx","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop;Other Space Weather","","","","","","Ground-based;Space-based","Space Weather Modeling and Prediction for Intermediate Time-scales","Enhanced solar activity bursts, or quasi-annual ""seasons"" of activity, followed by a quiet period, lead to similar quasi-periodic ""seasons"" of space weather. Forecasting space weather on time-scales of hours-to-days and decades-to-centuries received great attention. Recent discovery of solar Rossby waves reveal a golden opportunity to simulate space weather on weeks-to-months in advance.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-3d13bac3769b660e962ec0110405ee62_DikpatiMausumi.pdf"
"441","7 September 2022 10:37:00 pm","W. Kent","Tobiska","0000-0002-0415-8484","Space Environment Technologies","Shaylah","Marcin","Piyush","Richard","","Mutschler","Pilinski","Mehta","Licata","","","","","","","[email protected]","[email protected]","[email protected]","[email protected]","","Space Environment Technologies","Freestream, LLC","West Virginia University","West Virginia University","","","Space Weather Applications","","","","Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","Ground-based;Space-based","Critical needs for thermospheric density specification to aid operational systems","The number of LEO objects is TRIPLING in two years, directly increasing unintentional collisions between objects. Recommendations for reducing risks include creating an operationally viable uncertainty solution for the global thermosphere, methods to remediate the small size debris in LEO, and better understanding physical processes to reduce the global thermosphere density uncertainty.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-cec9f244bc6765c610a59dc68a747092_TobiskaWKentA1.pdf"
"442","7 September 2022 10:41:46 pm","Asti","Bhatt","0000-0002-8881-5348","SRI International","Leslie","Pablo","Todd","","","Lamarche","Reyes","Valentic","","","0000-0002-8881-5348","0000-0002-8433-5072","0000-0002-1940-3040","","","[email protected]","[email protected]","[email protected]","","","SRI International","SRI International","SRI International","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Data infrastructure needs for ground-based geospace science","Geospace science studies the entire coupled sun-earth system. In order to understand all parts of the system, a diverse set of observations from disparate instruments obtained at various locations in the geospace system are needed. Many are ground-based. This white paper outlines the current challenges and provides recommendations on best practices for ground-based geospace data infrastructure.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-17940b4f797932968cd292c48220602f_BhattAstiA2.pdf"
"443","7 September 2022 10:45:11 pm","Anthony","van Eyken","0000-0003-4160-3724","SRI International","John","Eric","","","","Kelly","Donovan","","","","","0000-0002-8557-4155","","","","[email protected]","[email protected]","","","","University of Central Florida","University of Calgary","","","","","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Ground-based;Space-based","A Well-Managed Planet?","The Well-Managed Planet requires reliable data covering all of geospace. Data availability must be evaluated for evolving scientific and societal need. New and existing instrumentation must be maintained and operated continuously. Data must be validated, citable, and widely and easily discoverable. Creating this infrastructure is an overwhelming technical challenge worthy of National attention.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-735e945e85a9d4bbd12491f26e4be933_vanEykenAnthonyP.pdf"
"444","7 September 2022 10:46:34 pm","W. Kent","Tobiska","0000-0002-0415-8484","Space Environment Technologies","","","","","","","","","","","","","","","","","","","","","","","","","","","Space Weather Applications","","","","Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","Ground-based;Space-based","Critical needs for radiation monitoring from the surface to LEO to aid operational systems","Radiation exposure is a natural hazard for flights from the atmosphere to space. Multiple sources of ionizing radiation contribute dose exposure. Mature measurement capabilities exist for providing radiation monitoring, but none are continuous within the atmosphere. A new, dedicated vehicle needs to be built for continuous radiation monitoring.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-faaf6273b250e2f580128057b9bcc61d_TobiskaWKentA2.pdf"
"445","7 September 2022 10:49:37 pm","Ercha","Aa","0000-0002-5228-4119","MIT Haystack Observatory","Shun-Rong","Wenbin","Anthea","Bill","","Zhang","Wang","Coster","Rideout","","0000-0002-1946-3166","0000-0002-6287-4542","0000-0001-8980- 6550","","","[email protected]","[email protected]","[email protected]","[email protected]","","MIT Haystack Observatory","NCAR High Altitude Observatory","MIT Haystack Observatory","MIT Haystack Observatory","","","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop","","","","","","Ground-based","Next-Decade Needs for Ionospheric 3-D imaging","Accurately imaging the 3-D spatial variation and temporal evolution of Earth's ionosphere has always been a challenging task for space weather community. We recommend advancing ionospheric 3-D imaging with finer resolution and precision, improved ionospheric driver estimation, better uncertainty quantification, support space weather nowcast/forecast, and sustained effort to increase data coverage","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-cfe23b2116a5662eab87b93dde83ac35_ErchaAa.pdf"
"446","7 September 2022 10:57:34 pm","Matthew","Zettergren","0000-0002-9837-059X","Embry-Riddle Aeronautical University","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-3288cddc87733ac516773f8883e66ccc_Author_Form_ZettergrenMatthewD.xlsx","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","","Physics-based Ionosphere-Thermosphere-Mesosphere Modeling: Status and Future Needs","This paper reviews the current state of first-principles (i.e. physics-based) ionosphere-thermosphere-mesosphere (ITM) models that use numerical solutions to systems of underlying differential or algebraic equations. We identify compelling future directions and urgent needs, and make near-term recommendations for investments in several different aspects of physics-based modeling and simulation. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-c19641e6ccd09c98a254edfa16a1d8cf_ZettergrenMatthewD.pdf"
"447","7 September 2022 10:55:13 pm","Daniel","Seaton","0000-0002-0494-2025","Southwest Research Institute, Boulder, CO","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F242-f58b0cdc05406dc0b6235d37b4d8399b_COMPLETE_Data_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Solar Physics","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Improving Multi-Dimensional Data Formats, Access, and Assimilation Tools for the Twenty-First Century","We discuss the need for new strategies for data products and data assimilation techniques to support complex contemporary observations. We present a case study that highlights this need, and make recommendations including investments in approaches for data assimilation and multi-observations products and developing new data use paradigms and modernized data formats.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-91bffa8f2fb1c8797c623f6d5d20f271_COMPLETE_Data_Strategy.pdf"
"448","7 September 2022 10:55:33 pm","Marta","Shelton","","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-9bb1ac0cabbd6badaaa0ee6d93440cf0_SSPH_White_Paper_Author_Information_Form_Shelton_at_al.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Infrastructure Strategy to Enable Optical Communications for Next-Generation Heliophysics Missions","For end-to-end support of decadal research strategies, a communications infrastructure is needed to improve data returned from deep space. Optical communications must be a part of a comprehensive solution as it provides 20x the data rate of RF frequencies. Based on data, maintaining or accelerating the build-out to form an Optical Ground Station Network for deep space is recommended.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-8e89976de087d489843fd2a4659402f0_SheltonMartaB.pdf"
"449","7 September 2022 10:57:41 pm","Carlos","Maldonado","0000-0002-1130-5067","Los Alamos National Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-c9347ce3be3a915d1c61fc5d3776ea44_SSPH_White_Paper_Author_Information_Form_20220907.xlsx","Basic Research;Space Weather Applications","Planetary Magnetospheres;Planetary ionospheres/upper atmospheres","","","Other Space Weather","","","","","","Space-based","The Critical Need for Innovations in Instruments and Techniques to Enable In-Situ Cold Ion and Cold Electron Measurements within the Magnetosphere","The lack of accurate measurements of the cold ion and cold electron populations through the magnetosphere makes closure of long-standing science questions extremely difficult if not impossible. This will require innovations in plasma spectrometers and associated techniques required to obtain high-fidelity in-situ measurements of the cold ion and cold electron populations in the magnetosphere. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-8345ebf9de98d5538efdd01e80fb6f3c_MaldonadoCarlosA.pdf"
"450","7 September 2022 11:06:54 pm","Eric","Donovan","0000-0002-8557-4155","University of Calgary","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Ground-based","A Long-Term North American Ground-Based Observing Program: Scaffolding for Geospace Research at the System Level and Space Weather Research","Long-term ground-based observations from across the US and Canada play a key role in informing our understanding of the multi-scale processes by which fundamental processes are spun up to have system-level consequences. I am recommending a 'scaffolding program' wherein key networks would provide long-term multi-scale observations that inform our fundamental science and our space weather goals. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F62-0e4f545e79fdd3357a4362bb80b92433_Donovan_GB_Scaffolding.pdf"
"451","7 September 2022 11:11:12 pm","Kevin","Reardon","0000-0001-8016-0001","National Solar Observatory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-ca6d48bded774a9319b859fc31ec39a7_Spectropolarimetric.Inversion.Techniques.WP.Author.Information.xlsx","Basic Research;Space Weather Applications","Solar Physics","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Ground-based;Space-based","Spectropolarimetric inversions: Our key to unlocking the secrets of the solar atmosphere","The physical conditions on the Sun can be inferred from the shapes of solar spectral lines by solving a complicated, ill-posed inverse problem. Powerful codes are being developed that treat complex aspects of the solar atmosphere. To unlock their full potential, the community must make a concerted, sizable effort to improve the physical veracity and computational tractability of these techniques. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-b77ce3823186919e6271908ab8295e2e_ReardonKevinP.pdf"
"452","7 September 2022 11:30:20 pm","Leslie","Lamarche","0000-0001-7098-0524","SRI International","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-7de4151d2a66eb482a6c06e821f0e443_AuthorInformationForm.xlsx","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Coordinating Science Between NASA Space-Based Missions and NSF Facilities","The funding structures of NSF and NASA create a situation where coordinated measurements from NSF large facilities and NASA missions is excessively challenging. This paper discusses how coordinated measurements are critical for system science, and explains why the issue is challenging.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-952e7283342bba9fdd4e92a52054d194_LamarcheLeslieJ3.pdf"
"453","7 September 2022 11:27:28 pm","James","Ryan","0000-0003-3534-5968","University of New Hampshire","John","Paul","Pierre-Simon","Veronica","Surujhdeo","Clem","Evenson","Mangeard","Bindi","Seunarine","0000-0001-5681-6883","","0000-0003-4865-6968","","","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","University of Delaware","University of Delaware","University of Delaware","University of Hawaii","University of Wisconsin, River Falls","","Basic Research;Space Weather Applications","Solar Physics;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","","The U.S. and Global Neutron Monitor Network for
Heliophysics and Space Weather","We review the status of the US neutron monitor network, the science activities that utilize the network, the long-standing and permanent need for the network, its key role in the national Space Weather Strategy, future scientific and space weather activities and objectives and, lastly, plans for expanding the public profile and improving the security and scientific function of the network","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-dae9489b8fc6d32a41aa913a62033a70_RyanJamesM.pdf"
"454","7 September 2022 11:28:24 pm","John","Leibacher","0000-0001-7605-3684","National Solar Observatory, LPL/University of Arizona, IAS/Université Paris-Saclay","Thierry","Gaël","Rafael A.","Laurent","Philip","Appourchaux","Buldgen","García","Gizon","Scherrer","0000-0002-1790-1951","","0000-0002-8854-3776","0000-0001-7696-8665","0000-0002-6937-6968","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","Institut d'Astrophysique Spatiale, Université Paris–Saclay","Département d'Astronomie, Université de Genève","Université Paris–Saclay. Université Paris–Cité, CEA, CNRS, AIM: ORCID 0000-0002-8854-3776","Max Planck Institute for Solar System Research: ORCID 0000-0001-7696-8665","Stanford University","","Basic Research","Solar Physics","","","","","","","","","","Probing the Structure and Dynamics of the Solar Core with Gravity Modes","The rotation and mixing of the core of the Sun, which control solar evolution and the present-day Sun, remain poorly constrained in spite of their crucial importance. The detection of a few gravity (g)-modes should enable the helioseismic probing of the solar core much like that already achieved for the outer radiative zone and convection zone with pressure (p)-modes","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-159c5f01605b9810cb737ec034a3f7a5_LeibacherJohnW.pdf"
"455","7 September 2022 11:34:49 pm","Benjamin","Lynch","0000-0001-6886-855X","University of California--Berkeley","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-952fbbf2ff059c30f1649e467e9ff8c7_Connecting_Solar_and_Stellar_Flares_CMEs_AuthorList.xlsx","Basic Research","Solar Physics;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","","Connecting Solar and Stellar Flares/CMEs: Expanding Heliophysics to Encompass Exoplanetary Space Weather","The maturity of data-inspired and data-constrained modeling of the Sun-to-Earth space weather chain provides a natural starting point for the development of new, multidisciplinary research and applications to other stars and their exoplanetary systems. Here we present recommendations for future solar CME research to further advance stellar flare and CME studies. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-f6956b7993d4b663eb4a50922b107226_LynchBenjaminJ.pdf"
"456","7 September 2022 11:42:30 pm","Mark","Conde","https://orcid.org/0000-0003-4924-878X","Geophysical Institute, University of Alaska Fairbanks","Donald","Aaron","","","","Haampton","Ridley","","","","","","","","","[email protected]","[email protected]","","","","Geophysical Institute, University of Alaska Fairbanks","University of Michigan","","","","","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Ground-based","4D-Imaging of Earth’s Space-Atmosphere Interaction Region","This White Paper describes a new array of three geophysical observatories currently being readied for deployment to northern Scandinavia, in support of the EISCAT-3D initiative. Multiple parameters of Earth's ionosphere and thermosphere will be measured, with the flagship product being 4D (lon, lat, alt, time) imaging of 3-component vector winds throughout the EISCAT-3D study volume. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-7ef857b2cf5d0ece4f2f3430c3f64e0d_CondeMarkG3.pdf"
"457","7 September 2022 11:39:04 pm","Clayton","Cantrall","0000-0002-9943-0566","JHU/APL","Larry","","","","","Paxton","","","","","0000-0002-2597-347X","","","","","[email protected]","","","","","JHUAPL","","","","","","Basic Research","Planetary ionospheres/upper atmospheres;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","Discovering the extent of terrestrial atmospheres: Mapping hydrogen and atomic oxygen in the thermosphere and exosphere","We propose utilizing space-based far ultraviolet (FUV) remote sensing to explore Earth's H and O distributions in support of cross-disciplinary, high-impact research goals. Thorough quantification of these distributions on Earth requires a dedicated, long-term, space-based FUV observational campaign.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-d2c40efbef8913813e536c9a77c0a0c8_CantrallClaytonE.pdf"
"458","7 September 2022 11:39:09 pm","Ryan","Volz","0000-0002-7504-0336","MIT Haystack Observatory","Jorge","Julio","","","","Chau","Urbina","","","","0000-0002-2364-8892","0000-0001-6281-4905","","","","[email protected]","[email protected]","","","","Leibniz Institute of Atmospheric Physics at the University of Rostock","The Pennsylvania State University","","","","","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based","Next-generation meteor radar networks for MLT science","Networks of meteor radars provide unique measurements that are necessary for advancing science of the mesosphere-lower thermosphere (MLT) region in the coming decade. We recommend deploying next-generation meteor radar networks to observe MLT wind fields and meteoric input over large regions with dense spatiotemporal sampling where scientifically necessary to achieve Decadal survey goals.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-fc9805c352ad19f3fdf75b83a5f3b6c4_VolzRyanA.pdf"
"459","7 September 2022 11:40:07 pm","Xin","Cao","0000-0003-0247-3584","LASP, University of Colorado Boulder","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-a2f892d936a02b70329edcc135784987_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","","Science Return of Probing Magnetospheric Systems of Ice Giants","We discuss the science return of probing magnetospheric systems of ice giants for the future missions, over different magnetospheric regions, across from the interaction with upstream solar wind to the downstream region of magnetotail. We emphasize the importance of detecting the magnetospheres of ice giants , which enables us to deeply understand ice giants' space environment and habitability.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-38ecb2f80482dce64f04b93b1e5fa8ba_CaoXin.pdf"
"460","7 September 2022 11:42:04 pm","Amir","Caspi","0000-0001-8702-8273","Southwest Research Institute","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F181-99bfbad7e45b5c287fb9ed91faad74a7_COMPLETE_Science_White_Paper_Author_Information_Form_sorted.xlsx","Basic Research","Solar Physics","","","","","","","","","Space-based","COMPLETE: a flagship mission for complete understanding of 3D coronal magnetic energy release","COMPLETE is a flagship mission concept that combines comprehensive magnetography with broadband spectroscopic imaging from multiple viewpoints around the Sun to enable tomographic reconstruction of 3D coronal magnetic fields and associated dynamic plasma properties that provide direct diagnostics of energy release.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-7f34009bf7a247be660c51c0b03a5c48_CaspiAmir1.pdf"
"461","7 September 2022 11:43:11 pm","Dimitrios","Vassiliadis","","NOAA/NESDIS/OPPA","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-0a6332780ddc15d8b7c3a3f69114feea_SSPHWhitePaperAuthorInformationForm_vassiliadis.xlsx","Basic Research;Space Weather Applications","Planetary Magnetospheres;Planetary ionospheres/upper atmospheres","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Ground-based","Advancing Space Weather Research and Mission Planning: OSEs, OSSEs, and Related Methods","The effective utilization of data in geospace models is essential for scientific understanding, developing specifications & forecasts and prioritizing observing-system procurements. Powerful methods leveraging high-resolution data are increasingly used in space physics: OSEs quantifying the impact of observing systems on model accuracy and OSSEs quantifying the value of new systems. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-a2b23e3eeb2de77eba341228862c6662_VassiliadisDimitrios.docx"
"462","7 September 2022 11:44:04 pm","Albert","Shih","0000-0001-6874-2594","NASA Goddard Space Flight Center","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-e60a9cf01501017b5f0ecc33b8c7e316_Shih_-_Ion_acceleration_in_SEEs_-_author_information.xlsx","Basic Research","Solar Physics;Basic research that is driven by space weather user needs","","","","","","","","","Space-based","Ion Acceleration in Solar Eruptive Events","How ions are accelerated to extreme energies during solar eruptive events – solar flares and associated coronal mass ejections (CMEs) – is still not well understood. We recommend prioritizing new observations of ion-associated signatures through the funding of next-generation measurements primarily in gamma rays, as well as in energetic neutral atoms (ENAs), neutrons, and EUV.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-63785ddfc6b66e32e4d8f50d29877c88_ShihAlbertY3.pdf"
"463","7 September 2022 11:45:59 pm","Hyunju","Connor","0000-0002-1327-1809","NASA GSFC","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-b2aa58a65c725b052a6941ec403b6ecf_SSPH_White_Paper_Author_Information_Form_-_exosphere.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","The Earth’s exosphere and its response to space weather","In the coming decade, we advocate that our community needs to increase our exploration of the neutral populations in the outermost reaches of the Earth's atmosphere. It is imperative that we improve both in-situ and remote-sensing technologies for measuring key neutral species in our exosphere. We also encourage dedicated exosphere missions and to stimulate model developments of our exosphere.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F101-c8c08b1d8938434638ef4cbb6daa71a7_ConnorHyunjuK.pdf"
"467","7 September 2022 11:53:50 pm","Leslie","Lamarche","0000-0001-7098-0524","SRI International","Matthew","Katrina","","","","Zettergren","Bossert","","","","","","","","","[email protected]","[email protected]","","","","ERAU","ASU","","","","","Basic Research","Planetary ionospheres/upper atmospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","","Polar Cap Science: MIT Coupling and Energy Deposition","This is a review of MIT coupling that occurs in the polar cap, and how these process deposit energy in the ionosphere.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-448fb4acebe3a93a42293854d3d27edc_LamarcheLeslieJ2.pdf"
"468","7 September 2022 11:55:11 pm","Christina","Lee","0000-0002-1604-3326","University of California, Berkeley","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-156d4a5f14d3861642627df6eecda92a_SSPH__LeeChristina_MarsSWxWP_Author_Info_Form.xlsx","Basic Research;Space Weather Applications","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Basic research that is driven by space weather user needs","","","Space Weather Research to Operations to Research Loop;Space Weather Applications related to robotic and human exploration in and beyond low-Earth orbit and the lunar environment","","","","","","Space-based","Heliophysics and Space Weather Science at ~1.5 AU: Knowledge Gaps and Need for Solar and Solar Wind Monitors at Mars","Discussion of knowledge gaps & open questions about the solar-interplanetary drivers of the space weather at Mars during active/quiescent solar periods, and the need for continuous, routine observations to address them. For advancing science & strategic planning for human exploration at Mars by the 2030s, now is the time to consider a network of upstream solar and solar wind monitors at Mars.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-88de3dd1281fdfca369c745281a9a808_LeeChristinaO.pdf"
"469","7 September 2022 11:55:24 pm","Philip","Horzempa","prescott44","LeMoyne College","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","Rigel Exoplanet Geologist","The Rigel probe will be sent to explore the surface of an exoplanet in a neighboring star system. It will be a robotic geologist. This paper outlines the challenges and promise of such a project.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F140-e6e750a43c342bec028aa9b9b16c76b1_RIGEL_INTERSTELLAR_PROBE__-__PF__-__A2.pdf"
"470","7 September 2022 11:56:18 pm","Cherilynn","Morrow","0000-0002-0898-7482","Consultant, Southwest Research Institute","Craig","Sanlyn","Sarah","","","DeForest","Buxner","Gibson","","","0000-0002-7164-2786","0000-0002-8504-252X","0000-0001-9831-2640","","","[email protected]","[email protected]","[email protected]","","","Southwest Research Institute","Planetary Science Institute","High Altitude Observatory, National Center for Atmospheric Research","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","Support for a New and Improved Approach for NASA Mission-Embedded Outreach","Former NASA policy required PI's of proposed missions to allocate 1-2% of their budget for education & public outreach (EPO). This policy was endorsed by the previous Decadal Survey. However, the ""mandate"" approach was not fully successful and was discontinued. We describe a new, optional approach to mission-embedded outreach being enacted by the PUNCH mission as the basis for a new endorsement. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F190-e0b88dbc2a8d1c1b9beb967ebfd9c395_MorrowCherilynnA.pdf"
"471","7 September 2022 11:56:41 pm","Nour E.","Raouafi","0000-0003-2409-3742","Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-265e70083c823c72c50ae43098085b30_2024-2033_SSPH_Decadal_White_Paper_Firefly-Author_Information_Form.xlsx","Basic Research;Space Weather Applications","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Space-based","Firefly: The Case for a Holistic Understanding of the Global Structure and Dynamics of the Sun and the Heliosphere","This white paper is on the HMCS Firefly mission concept study. Firefly focuses on the global structure and dynamics of the Sun's interior, the generation of solar magnetic fields, the deciphering of the solar cycle, the conditions leading to the explosive activity, and the structure and dynamics of the corona as it drives the heliosphere.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F68-16030f9cb9d69d20ef782b4de10a8012_2024-2033_SSPH_Decadal_White_Paper_Firefly-HMCS_Mission_Concept.pdf"
"472","7 September 2022 11:58:55 pm","Xinzhao","Chu","0000-0001-6147-1963","University of Colorado Boulder","Guotao","Zhibin","Chester","Sharon","Shikha","Yang","Yu","Gardner","Vadas","Raizada","","","0000-0001-9765-8973","","","","","","","","","","","","","","Basic Research;Infrastructure, Workforce, Other Programmatic","Basic research that is driven by space weather user needs","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Ground-based;Space-based","Future Lidars for Cutting-Edge Sciences in the ITM Physics and Space-Atmosphere Coupling","In the last 15 years, lidar observations have evolved to the significantly extended altitude ranges. The recent results demonstrate the huge potentials that lidars and their future generations will bring to the ionosphere-thermosphere-mesosphere (ITM) physics and space-atmosphere interactions. This paper will focus on the future of ground-based lidar studies in enabling cutting-edge sciences. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F69-6cf06bf4b0cdbff6dc87192eeffea582_Chu_FutureLidars_WhitePaper.pdf"
"473","7 September 2022 11:57:43 pm","Hadi","Madanian","0000-0002-2234-5312","University of Colorado Boulder","","","","","","","","","","","","","","","","","","","","","","","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Dynamic Characterization of Plasma Boundaries with Soft X-Ray Imagers","This paper describes the need and make recommendations for a new type of measurement.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-ae004a9f42670ff68ed11d4edde43d2c_MadanianHadi2.pdf"
"475","7 September 2022 11:58:03 pm","Russell","Stoneback","0000-0001-7216-4336","Stoneris","","","","","","","","","","","","","","","","","","","","","","","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Sustainable Funding for Scientific Software","Long term continuous funding is required for effective scientific software development and the maintenance of vibrant development communities. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-5e347ed65059f3fca0bb57419c5089f4_StonebackRussellA.pdf"
"476","8 September 2022 12:01:50 am","Robert","Pfaff","0000-0002-4881-9715","NASA/Goddard Space Flight Centewe","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-70b66937b81ff512a63e2580cd23aaa1_PfaffRobertF2_author_info.xlsx","Basic Research","Planetary ionospheres/upper atmospheres","","","","","","","","","","Measuring the Vector Electric Field in the Ionosphere","This white paper discusses the importance of electric field measurements on low Earth orbiting satellites in the Earth's ionosphere at all latitudes. Such observations are critical to learning how the Earth's coupled ion-neutral gases interact among themselves and with energy and momentum sources originating from the magnetosphere above and the troposphere below. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F79-39d6663d3238e36b6b61e223c229605e_PfaffRobertF2.pdf"
"477","8 September 2022 12:00:35 am","Sarah A.","Spitzer","0000-0001-9607-1492","University of Michigan","Susan T.","Jason A.","Jim M.","","","Lepri","Gilbert","Raines","","","0000-0003-1611-227X","0000-0002-3182-7014","0000-0001-5956-9523","","","[email protected]","[email protected]","[email protected]","","","University of Michigan","University of Michigan","University of Michigan","","","","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","Complementary Interstellar Detections from the Heliotail","What is the global shape of the Heliosphere, especially in the Heliotail, and how does the ISM interact with, penetrate, and affect the composition of the Heliosphere? * Better PUI measurements * GCR measurements & ENAs in the Heliotail * Measurements of interstellar ions that penetrate the Heliosphere * A possible Interstellar Probe Component in the Heliotail ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-436c8cf0a5e423b15d886ee6003e1c6f_SpitzerSarahA.pdf"
"478","8 September 2022 12:01:12 am","Marcin","Pilinski","0000-0002-1509-3268","University of Colorado Boulder","Eric","Jeffrey","Timothy","Kent","","Sutton","Thayer","Minton","Tobiska","","0000-0003-1424-7189","0000-0001-7127-8251","0000-0003-4577-7879","0000-0002-0415-8484","","[email protected]","[email protected]","[email protected]","[email protected]","","Space Weather Technology, Research, and Education Center","Space Weather Technology, Research, and Education Center","Ann and H.J. Smead Aerospace Engineering Sciences","Space Environment Technologies","","","Basic Research;Space Weather Applications","Planetary ionospheres/upper atmospheres;Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations","","","","","","","Relevance of Gas-Surface Interactions for Thermospheric Science and Monitoring","Drag-derived neutral density datasets are valuable to the scientific exploration of the thermosphere as well as to monitoring of the low Earth orbit environment. We discuss challenges in developing and utilizing these datasets stemming from uncertainties in satellite aerodynamic parameters. We then present potential research pathways for addressing these challenges.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F19-666d0129cb6831378fbf3aea32f6cd74_PilinskiMarcinD.pdf"
"479","8 September 2022 12:08:47 am","Amir","Caspi","0000-0001-8702-8273","Southwest Research Institute","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-98c066ddf18fa1ef43a4c2605330a57d_Science_White_Paper_Author_Information_Form_sorted.xlsx","Basic Research","Solar Physics","","","","","","","","","","Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release","The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. We advocate for new and multi-point co-optimized measurements, sensitive to magnetic field and other plasma parameters, spanning from optical to gamma-ray wavelengths, to bring closure to long-standing and fundamental questions.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-a8412fd475ebc471f4176a1410de0eeb_CaspiAmir2.pdf"
"480","8 September 2022 12:12:09 am","Xin","Cao","0000-0003-0247-3584","LASP, University of Colorado Boulder","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F107-274b45822e87b89b2d9189f0fb10d406_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Planetary Magnetospheres;System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","","Science Return of Probing Magnetospheric Systems of Ice Giants","We discuss the science return of probing magnetospheric systems of ice giants for the future missions, over different magnetospheric regions, across from the interaction with upstream solar wind to the downstream region of magnetotail. We emphasize the importance of detecting the magnetospheres of ice giants , which enables us to deeply understand ice giants' space environment and habitability.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-0f885e0be2c34ff00fb3477bc5817259_CaoXin.pdf"
"481","8 September 2022 12:29:50 am","Lindsay","Glesener","0000-0001-7092-2703","University of Minnesota","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-696042ffedad966262df9282a837ee8f_SSPHWhitePaperAuthorInformationForm.xlsx","Basic Research","Solar Physics","","","","","","","","","","The need for focused, hard X-ray investigations of the Sun","Understanding accelerated particles at the Sun is one of the most important problems in heliophysics. Flare-accelerated particles have huge energies; are an important source of particles in the heliosphere; and are the most important corollary to other areas of high-energy astrophysics. This paper describes the scientific motivation for X-ray studies of particle acceleration at the Sun.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F202-99a69346660dffa74e233a5563bf44b9_GlesenerLindsay.pdf"
"482","8 September 2022 12:33:56 am","Cora","Randall","0000-0002-4313-4397","University of Colorado","Lynn","Nicholas","Scott","Naomi","Thomas","Harvey","Pedatella","Bailey","Maruyama","Chen","0000-0002-7928-0804","0000-0002-8878-5126","0000-0001-7693-0966","","0000-0002-0294-3614","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","university of Colorado","NCAR","Virginia Tech","University of Colorado","Columbia U.","","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions)","","","","","","","","","Space-based","Sun-Earth Coupling via Energetic Particle Precipitation","The motivation behind this white paper is the need to improve our understanding of, and ability to simulate, energetic particle precipitation (EPP) effects on the atmosphere. Investigating coupling between the mesosphere / lower thermosphere and lower atmosphere will improve predictability of the atmospheric response to solar and magnetospheric forcing.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-fbf24a84b8b11fe7d960a3be36a88e11_RandallCoraE.pdf"
"483","8 September 2022 1:50:57 am","Dave","Brain","0000-0001-8932-368X","LASP / University of Colorado","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-51837a5f37a23eb0d8591bcc9f0db95e_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);","","","","","","","","","","The Influence of Planetary and Stellar Characteristics on Atmospheric Escape and Habitability","Atmospheric escape occurs at planets everywhere, and influences the evolution of planetary atmospheres and surface habitability. We argue for developing a common understanding of atmospheric escape that accounts for different star and planet characteristics. This requires comprehensive measurements at multiple planets, new models that cover the entire parameter space, and interdisciplinary effort.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F206-5c2d92d32fd4d4dc368151d8ea36aba1_BrainDaveA.pdf"
"484","8 September 2022 2:13:35 am","Gianna","Cauzzi","0000-0002-6116-7301","National Solar Observatory","","","","","","","","","","","","","","","","","","","","","","","","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","State of the Profession including workforce capabilities and current status, future needs to improve health and vitality of the community, diversity, equity, accessibility, and inclusion","","","","COMMUNITY EDUCATION TO FOSTER FACILITY ENGAGEMENT: Schools and Data Workshops to Enhance the Scientific Return of DKIST","The Daniel K. Inouye Telescope (DKIST) recently commenced operations, and data will soon be available to the US solar community. We advocate here for a continuing program aimed at informing and educating the US researchers on high-resolution solar imaging, spectroscopy, and polarimetry from the ground, in order to properly exploit the incredible scientific opportunities provided by this facility. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F196-bdb55dbe418dc0d9e4c69e9b7989d88f_CauzziGianna.pdf"
"485","8 September 2022 3:00:32 am","Artur","Davoyan","","University of California Los Angeles","Marco","Les","Henry","","","Velli","Johnson","Helvajian","","","","","","","","","","","","","University of California Los Angeles","Marshall Space Flight Center","The Aerospace Corporation","","","","Basic Research","Solar Physics;Inner Heliosphere and solar wind interaction with unmagnetized bodies","","","","","","","","","Space-based","ENABLING 4D MAPPING OF THE INNER CORONA AT HIGH LATITUDES AND POLES WITH EXTREME SOLAR SAILING","Understanding the profound complexity of solar interior is one of the most elusive long-standing grand open questions. Here, we propose a breakthrough space mission that will place a spacecraft in an extreme vicinity of the Sun and at a high solar latitude (>45 deg, including poles), with an orbit that is just 2-5 solar radii (R_☼) from its surface. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F76-8cedf975295b815c9bdd9c4732a2c65a_DavoyanArturA2.pdf"
"486","8 September 2022 3:02:19 am","Artur","Davoyan","","University of California Los Angeles","Marco","Henry","Les","Slava","","Velli","Helvajian","Johnson","Turyshev","","","","","","","","","","","","University of California Los Angeles","The Aerospace Corporation","Marshall Space Flight Center","Jet Propulsion Laboratory","","","Basic Research","Outer Heliosphere;Emerging Opportunities: interstellar medium, astrospheres (and their stars), exoplanets (and their magnetospheres/ionospheres/upper atmospheres), and planetary habitability","","","","","","","","","Space-based","SCALABLE AND LOW COST EXPLORATION OF THE INTERSTELLAR NEIGHBORHOOD WITH 50 AU/YEAR FAST TRANSIT SOLAR SAIL MISSIONS","The present white paper sets a goal of transforming in the next decade the way heliosphere and local interstellar medium are explored. We discuss that new technologies, with subcomponents proven feasible and flight tested, can allow fast (>25 AU/year and potentially up-to 50 AU/year) and scalable exploration of distant reaches of the outer solar system. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-f0e491793964762c24df20c7c79b6951_DavoyanArturA1.pdf"
"487","8 September 2022 10:52:53 am","Amber","Dubill","","Johns Hopkins Applied Physics Laboratory","Angelos","George","","","","Vourlidas","Ho","","","","","","","","","[email protected]","[email protected]","","","","Johns Hopkins Applied Physics Laboratory","Johns Hopkins Applied Physics Laboratory","","","","","Basic Research;Space Weather Applications","Solar Physics;Other topic relevant to solar and space physics/heliophysics","","","Space Weather Pipeline from Research to Application to Operations","","","","","","Space-based","Improving Solar Observing Capabilities with Diffractive Solar Sailing","Solar sails, and in particular diffractive sails are an enabling technology for pushing the boundaries of heliophysics forward by allowing unique measurements from obits unattainable otherwise. Specifically, diffractive solar sailing is beneficial to establish solar polar observational sailcraft. (Recommended resubmission as a .pdf file)","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F105-7c82759d15a583f258465ae17e6c50d3_DubillAmberL.pdf"
"488","8 September 2022 11:53:16 am","Nathalia","Alzate","0000-0001-5207-9628","NASA GSFC / ADNET Systems","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F36-3f47eccc57c5a717c84be7eb6123caae_AlzateNathaliaAuthors.xlsx","Basic Research;Infrastructure, Workforce, Other Programmatic","Solar Physics;Other topic relevant to solar and space physics/heliophysics","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","","Data Mining for Science of the Sun-Earth Connection as a Single System","Heliophysicists will have to manage the increasing amount of information from new missions and improved re-analysis of past missions. This is further complicated by different datasets/catalogs in different formats requiring different analysis tools, often available in different programming languages. There is need for venues of discussion and coordination of data management and interoperability.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F135-00c1e3c02da82cd251b0473ca076ed6c_AlzateNathalia.pdf"
"489","8 September 2022 1:38:48 pm","Qian","Wu","0000-0002-7508-3803","National Center for Atmospheric Research","Wenbin","Dong","Jan-Peter","Yongliang","Chaosong","Wang","Lin","Weiss","Zhang","Huang","0000-0002-6287-4542","0000-0003-2894-6677","0000-0003-4934-4966","0000-0003-4851-1662","0000-0002-2096-9340","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","NCAR","NCAR","UCAR/COSMIC","APL","AFRL","","Basic Research;Space Weather Applications","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","Space Weather Pipeline from Research to Application to Operations;Space Weather Research to Operations to Research Loop","","","","","","Space-based","Global Airglow Thermosphere Ionosphere Mission (GATI)","This white paper describes a concept of high-orbit limb-scan instrument: Global Airglow Thermosphere Ionosphere mission (GATI) which will measure the thermospheric winds (200 to 300 km altitude) by recording wind induced Doppler shift in the O 630 nm airglow emission day and night. ","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F121-6a978660594d7fd68757cf749ea30e37_submission.pdf"
"490","8 September 2022 7:58:33 pm","Philip","Fernandes","0000-0002-3432-8624","Los Alamos National Laboratory","","","","","","","","","","","","","","","","","","","","","","","","","","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F44-58e74f683d198f41efc024e8ab8dec59_SSPH_White_Paper_Author_Information_Form.xlsx","Basic Research","System Science (solar wind - magnetosphere - atmosphere - ionosphere interactions);Basic research that is driven by space weather user needs","","","","","","","","","","Heavy Ions: A Critical Measurement for Understanding the Solar Wind/Ionosphere/Magnetosphere","The typical on-orbit mass spectrometer is limited in mass resolution capability, such that it cannot distinguish N+ from O+ by design. We propose a community goal of characterizing the full complement of plasma species (composition and charge state) within the Solar Wind/Magnetosphere/Ionosphere system to understand how these populations interact with one another and impact the system as a whole.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F164-b0ac853c1d5e0272c84dc37f101d1324_FernandesPhilipA.pdf"
"491","9 September 2022 2:55:32 am","John","Leibacher","0000-0001-7605-3684","National Solar Observatory, LPL/University of Arizona, IAS/Université Paris-Saclay","Thierry","Gaël","Rafael A.","Laurent","Philip","Appourchaux","Buldgen","García","Gizon","Scherrer","0000-0002-1790-1951","","0000-0002-8854-3776","0000-0001-7696-8665","0000-0002-6937-6968","[email protected]","[email protected]","[email protected]","[email protected]","[email protected]","Institut d'Astrophysique Spatiale, Université Paris–Saclay","Département d'Astronomie, Université de Genève","Université Paris–Saclay. Université Paris–Cité, CEA, CNRS, AIM: ORCID 0000-0002-8854-3776","Max Planck Institute for Solar System Research: ORCID 0000-0001-7696-8665","Stanford University","","Basic Research","Solar Physics","","","","","","","","","","Probing the Structure and Dynamics of the Solar Core with Gravity Modes","The rotation and mixing of the core of the Sun, which control solar evolution and the present-day Sun, remain poorly constrained in spite of their crucial importance. The detection of a few gravity (g)-modes should enable the helioseismic probing of the solar core much like that already achieved for the outer radiative zone and convection zone with pressure (p)-modes.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F8-5a5111805a05db5b1fda4df50575e1d5_LeibacherJohnW1.pdf"
"492","9 September 2022 1:56:05 pm","Stephen","Omondi","","Student at E-JUST at Alexandria in Egypt","","","","","","","","","","","","","","","","","","","","","","","","","","","Basic Research","Inner Heliosphere and solar wind interaction with unmagnetized bodies;Outer Heliosphere","","","","","","","","","Space-based","Understanding Magnetic Field Inside/Outside Heliosphere and Connecting to Magnetopause","The study covers magnetic field profiles in both the interior and outer heliosphere. Measurements of magnetic fields and plasma across the heliopause and far into the VLISM are required to understand the complex topology and dynamics at the heliosphere's interface to the VLISM. The interstellar probe will be of great use in achieving this mission.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F81-5c677bd3cc244907958ef0f29d9a6633_Helio_Clean.docx"
"493","14 September 2022 1:37:32 pm","Hadi","Madanian","0000-0002-2234-5312","University of Colorado Boulder","Randal","Robert","Shotaro","","","Bryant","Lillis","Sakai","","","","","","","","","","","","","Carnegie Mellon University","University of California Berkeley","Tohoku University","","","","Infrastructure, Workforce, Other Programmatic","","","","","","","Research Tools and Infrastructure (that is not specific to one research area)","","","Space-based","Increased Science Return of Long Duration Missions Exploring Distant Environments through Autonomous Spacecraft Design","This document describes the need for new investments in enabling technologies in preparation for long duration missions exploring distant environments. It describes some of the main technological obstacles in designing exploration missions that can consistently produce science results even at extremely far distances from Earth. It recommends solutions to overcome those obstacles.","http://surveygizmoresponseuploads.s3.amazonaws.com/fileuploads%2F623127%2F6920789%2F127-0653446abca78d7b632c5042b59d57cc_MadanianHadi1.pdf"