Skip to content

Latest commit

 

History

History
38 lines (20 loc) · 1.41 KB

README.md

File metadata and controls

38 lines (20 loc) · 1.41 KB

STEP2_QUENCHING

In order to perform DM for CHLA you should

  1. STEP 1 : Estimate the DARK OFFSET of the CHLA
  1. STEP 2 : Correct the profile from the DARK and estimate the quenching correction (Xing 2018, Terrats 2020, Sackmann 2008)

You need :

=> A working directory containing Argo B files and C files (Be careful the program will write a new CHLA_ADJUSTED in your B files !!!)

=> WMO.DARK : a file containing the OFFSET of the CHLA (the CHLA will be corrected as CHLA - OFFSET ) of the WMO float of interest

=> coriolis_CHLA.list is the list of all the WMO floats you want to correct (for every entry, you need a WMO.DARK file)

-lance_STEP2 is my launching script :

  -It defines the pathway to the working directory
  
  -It reads the coriolis_CHLA.list to know the WMO 
  
  -It reads the working directory to build the list of the Bfiles : "liste_all_B" 

-MLD_calc.R is calculating the MLD

-IPAR_15_DEPTH.R is estimating the depth at which the PAR is equal to 15 (Limit under which there is no longer quenching)

-RunningFilter.R is used to filter (mean, median) the data

-Quenching_correction.R is the main program (you will need oce, stringR, ncdf4 library)

The outputs are files ready for STEP3 : estimation of the SLOPE