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Do Chemistry
Most steps follow the same instructions as regular rrfs-workflow with some steps have some special options or configurations.
which git-lfs 2>/dev/null || module load git-lfs
GIT_LFS_SKIP_SMUDGE=1 git clone -b rrfs-mpas-jedi --recursive https://github.com/NOAA-EMC/rrfs-workflow
cd rrfs-workflow/sorc
./build.all chem noda
NOTE: If doing chemistry data assimilation, one needs to build as ./build.all chem
Example:
cd workflow
cp exp/exp.conus12km exp.conus12km
vi exp.conus12km # set DO_CHEMISTRY=true; modify EXP_NAME, OPSROOT, RETRO_PERIOD and others as needed.
vi config_resources/config.chemistry # double check chemistry related variables are set correctly
./setup_rocotpy.py exp.conus12km
NOTE:
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Lots of variables should be modified in
config_resources/config.chemistry, such asCYC_INTERVAL, CYCLEDEF_IC_STEP_HRS, LBC_CYCS, COLDSTART_CYCS, FCST_LEN_HRS_CYCLES, LBC_LENGTH, etc. The settings in config.chemistry will override the corresponding settings in the exp file.
We adopt this strategy so that one can run the chemistry workflow out-of-the-box with minimum changes. -
The default setting does NOT do data assimilation.
AlthoughDO_IODA,DO_JEDI,DO_CYCare set totrueby default in exp files, they are overrode tofalseinconfig_resources/config.chemistry. So if one wants to chemistry DA, one needs to change them back totruein config.chemistry.
The other procedures/steps are the same as running regular RRFS experiments in this documentation link
When RAVE emission file is not available, rrfs-workflow will try to find a RAVE_dummy file from ${COMINrrfs}/RAVE_dummy.nc; if the dummy file is not available, the workflow will stop with an error.
One can link an existing RAVE_dummy file from other staged area; or one may create a new dummy file from an RAVE emission file under the prep_chem run directory using the utility workflow/ush/chem_create_rave_dummy.sh.
Usually, one mesh only needs a corresponding RAVE_dummy file and most times it may be found at ${CHME_INPUT}/emissions/RAVE/processed/RAVE.dummy.${MESH_NAME}.nc.