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Add code changes for the implementation of the low-resolution B #1441
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Automated GW-GDASApp Testing Results:
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Did not test, but I reviewed all the code changes, they look good to me.
Automated GW-GDASApp Testing Results:
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Automated GW-GDASApp Testing Results:
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Automated GW-GDASApp Testing Results:
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Weird, it looks like it used the wrong commit of the g-w branch. I merged develop before resubmitting the ci but that;s not what was cloned here: /work2/noaa/da/role-da/CI/hercules/GDASApp/workflow/PR/1441/global-workflow |
Automated GW-GDASApp Testing Results:
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Automated GW-GDASApp Testing Results:
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GDASApp ctests including C48mx500_3DVarAOWCDA and C48mx500_hybAOWCDA pass on Hera, Hercules, and Orion.
Approve.
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looks ok
Here are the changes that I needed to do for the recenter task to succeed with a zero exit status: diff --git a/parm/soca/berror/soca_ensrecenter.yaml b/parm/soca/berror/soca_ensrecenter.yaml
index b700601..b7d8e20 100644
--- a/parm/soca/berror/soca_ensrecenter.yaml
+++ b/parm/soca/berror/soca_ensrecenter.yaml
@@ -60,5 +60,5 @@ output increment:
date: '{{ MARINE_WINDOW_END_ISO }}'
exp: trash
type: incr
- output file: 'ocn.recenter.incr.%mem%.nc'
+ output file: 'recenter.incr.%mem%.nc'
pattern: '%mem%' and diff --git a/utils/soca/gdas_ens_handler.h b/utils/soca/gdas_ens_handler.h
index 741055c..dd5fe9c 100644
--- a/utils/soca/gdas_ens_handler.h
+++ b/utils/soca/gdas_ens_handler.h
@@ -169,7 +171,30 @@ namespace gdasapp {
postProcIncr.setToZero(incr);
// Save the increments used to initialize the ensemble forecast
- result = postProcIncr.save(mom6_incr, i+1);
+ result = postProcIncr.save(mom6_incr, i+1, {"ocn"}); It fixes two issues: missing ice file (that we don't use in this usecase anyway) and wrong ocean file name. |
…3238) This PR mostly includes configuration changes to allow the use a B-matrix at a defined resolution that may or may not be the same as the background. - Addition of an interpolation step in the B-matrix job - version update for the fix files - **the `gdas.cd` update should be the correct one now.** Resolves #3230 Resolves NOAA-EMC/GDASApp/issues/1375 # Dependencies - NOAA-EMC/GDASApp/pull/1441 - NOAA-EMC/jcb-gdas/pull/66 --------- Co-authored-by: Anna Shlyaeva <[email protected]> Co-authored-by: RussTreadon-NOAA <[email protected]> Co-authored-by: Rahul Mahajan <[email protected]>
* develop: added original date (#1570) Update OCEAN_BASIN_FILE_ORION path for marine ctest (#1569) Fixing window_begin and end in yaml for redating ADT (#1565) Save LETKF mean analysis and mean increment for verification (#1566) Update JEDI hashes (20250324) (#1567) Removes obsolete json files from marine bufr2ioda (#1564) Add hybrid 4denvar as a phase3 validation configuration (#1552) Bugfix/ocn ecen (#1550) Bugfix SSS obs for LETKF (#1560) Bugfix ocean ensemble recentering (#1558) apply ci path patch only when running g-w ctests (#1554) Update JEDI hashes (20250317) (#1531) add option to create_experiment.py in create_exp.sh (#1546) Update jcb hashes and support initial IODA stats capability (#1547) Fix GW-CI CTest dependencies (#1534) Converts prepoceanobs to use JCB-style obs list and config files (#1527) JEDI-based ensemble recentering and analysis calculation (#1488) tools for phase3 validation (#1526) Update JEDI hashes (20250306) (#1520) New jcb-gdas # and insitu obs prep bug fix (#1523) Marine in situ obs update (SSS, moorings, drifters) (#1511) Save marine background and analysis spread (#1517) Minor build and install updates and ctest cleanup (#1512) correct logic for upper loop limit in chem_diagb (#1516) Incorporate multi-cycle concatination and separation of variables in post-BUFR observations (#1504) Update JEDI hashes (20250225) (#1475) Add a depth dependent e-fold scale (#1494) Update jcb and da-utils hashes to support land DA. (#1509) Add options to inflate the ensemble while recentering (#1501) Add components to use jcb yamls for marine letkf job (#1486) Add GNSSRO bufr2ioda and json files (#1448) Removal of the marine verification tools (#1499) update logic to identify MSU machine (#1498) IODA Converter with In-Situ Observations Concatenation and ObsError Inflation (#1472) Add sea ice recentering (#1478) marine vrfy bugfix (#1483) add LD_LIBRARY_PATH patch for wcoss2 build (#1484) Bugfix for ensemble recenter + add a test (#1477) Add code changes for the implementation of the low-resolution B (#1441) update spack-stack path in Hera modulefiles (#1471) fixed glider output filename (#1469) add gdas_waveinit to C48mx500_3DVarAOWCDA ctest suite (#1470) update jcb-gdas hash 20250128 (#1466) Time series of omb stats and html doc (#1463) Update marine vrfy HTML codes (#1464) Automate the verify tools to submit from start pdy to end pdy (#1458) Update an offline marine vrfy tool (#1447) Update JEDI hashes (20250127) (#1460)
…(#3238) This PR mostly includes configuration changes to allow the use a B-matrix at a defined resolution that may or may not be the same as the background. - Addition of an interpolation step in the B-matrix job - version update for the fix files - **the `gdas.cd` update should be the correct one now.** Resolves #3230 Resolves /issues/1375 # Dependencies - /pull/1441 - NOAA-EMC/jcb-gdas/pull/66 --------- Co-authored-by: Anna Shlyaeva <[email protected]> Co-authored-by: RussTreadon-NOAA <[email protected]> Co-authored-by: Rahul Mahajan <[email protected]>
As the title says.
Dependencies
Work done in this PR
Interp to low-resolution:
Testing
Visual check showing the variance explained by the steric height (30 members)

left is native resolution, right is on the 1/2 deg grid.
"Science" note: The explained variance above is almost the opposite to what I would have expected, and what we saw in the previous offline ensemble, or even what we see in tendencies. Check if there's a bug in the explained variance calculation.
Automated CI tests to run in Global Workflow