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A forthcoming PR will do the following for MPAS-related applications:
For VIL, discontinue use of the local GRIB2 table
Add GSL's experimental ceiling fields to the GRIB2 output
Within "INITPOST_MPAS", remove instances of "if imp_physics...". These portions of the code initialize various arrays based upon the microphysics scheme. However, many of these "imp_physics" identifiers correspond to schemes in WRF-ARW. If they are again needed for MPAS, these codes can be re-introduced.
A forthcoming PR will do the following for MPAS-related applications:
This issue can be assigned to @jaymes-kenyon
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