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Only 30 members should be used for the early cycle #1588
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Only 30 members should be used for the early cycle #1588
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@CatherineThomas-NOAA Is there a set of 80-member low-res ICs I can use to test? |
Not that I know of @AndrewEichmann-NOAA . |
Sorry @AndrewEichmann-NOAA, we have 30 member low res, or 80 member full res. You can fake the 80 members by just copying/linking to the existing members though. |
@CatherineThomas-NOAA Where are those on Hera? I forget if there is a reason not to use what's under |
That should "work" @AndrewEichmann-NOAA . |
@AndrewEichmann-NOAA : I agree, I think those C48 ones would work. In case you want to poke around the higher res ICs, there are some dates for the full res on Hera here: |
@CatherineThomas-NOAA Does the following experiment cover what's needed? Edits in config.base:
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@AndrewEichmann-NOAA : Sorry for missing this earlier, but |
So when |
@AndrewEichmann-NOAA : The recentering in the early cycle should be performed on and copied to the |
From @CatherineThomas-NOAA :
The early cycle EnKF will only consist of 30 members (NMEM_ENS_GFS in config.base). Those 30 members are chosen as a subset of the previous cycle's 80 members on a cyclical basis. 00z uses members 1-30, 06z uses 21-50, 12z uses 41-70, 18z uses 61-80 and 1-10. The shift in members per cycle is defined by NMEM_ENS_GFS_OFFSET in config.base:
In the atmospheric EnKF scripts, we first compute the offset for the cycle (mem_offset). From exgdas_enkf_update.sh:
Then we point to the appropriate member when defining the background:
This feature was added in this PR. There were a couple bugfixes since then, but it should give you an idea to what's generally needed.
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