Stage atmospheric backgrounds and UFS cubed-sphere history files#19
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| npy: {{atmosphere_npy_ges}} | ||
| npz: {{atmosphere_npz_ges}} | ||
| field metadata override: "{{atmosphere_fv3jedi_files_path}}/fv3jedi_fieldmetadata_restart.yaml" | ||
| field metadata override: "{{atmosphere_fv3jedi_files_path}}/fv3jedi_fieldmetadata_history.yaml" No newline at end of file |
CoryMartin-NOAA
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Jul 30, 2024
CoryMartin-NOAA
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This PR changes the GDASApp so that backgrounds for the atmospheric analyses are staged as UFS cubed-sphere history files rather than FMS restarts. jjob tests and test data are also updated to accommodate these changes. The motivation being that FMS restarts include many data we don't need for the analyses and thus take up too much disk space/bandwidth. This is a companion PR to Global Workflow [#2792](NOAA-EMC/global-workflow#2792) and JCB-GDAS [#19](NOAA-EMC/jcb-gdas#19).
DavidNew-NOAA
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This PR changes the GDASApp so that backgrounds for the atmospheric analyses are staged as UFS cubed-sphere history files rather than FMS restarts. jjob tests and test data are also updated to accommodate these changes. The motivation being that FMS restarts include many data we don't need for the analyses and thus take up too much disk space/bandwidth. This is a companion PR to Global Workflow [#2792](NOAA-EMC/global-workflow#2792) and JCB-GDAS [#19](NOAA-EMC/jcb-gdas#19).
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This PR changes the G-W so that backgrounds for the atmospheric analyses are staged as UFS cubed-sphere history files rather than FMS restarts. The motivation being that FMS restarts include many data we don't need for the analyses and thus take up too much disk space/bandwidth.
This is a companion PR to Global Workflow #2791 and GDASApp #1236.