GFDLMP-v3 and TEMPO MP microphysics#823
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@dustinswales I'd like to test this version. How do I check this code? Thanks! |
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git clone --recursive --branch feature/gfdlmpv3 https://github.com/dustinswales/ufs-weather-model.git |
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Dependency: ufs-community/ccpp-physics#195 |
… into feature/gfdlmpv3
dustinswales
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BrianCurtis-NOAA
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Jul 14, 2025
DusanJovic-NOAA
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Jul 14, 2025
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Description (*updated on 7/2/2025)
This PR contains host side changes to accommodate TWO new cloud microphysics parameterization in the CCPP physics.
GFDLMP v3:
@RuiyuSun
For the refactoring, all of the configuration/namelist info is moved into a common module that is referenced by both MP versions and a shared fv_sat_adj.F90. There are default values for the scheme configurations defined within this module, and overwritten by the namelist, if provided. Both the v1 and v3 rely on some of the same parameters, but with different default values. This is handled by introducing a pre-processor directive into the new configuration module.
Note. The "initialization bug" results in itsy-bitsy changes to the results, and is not addressed in these changes. A complete solution would require the GFDL MP scheme namelist to be read in during the dycore initialization.
TEMPO MP:
@AndersJensen-NOAA
TEMPO stand for Thompson-Eidhammer Microphysics Parameterization for Operations.
The use of a submodule will enable centralized community development (and testing) of the microphysics scheme for various applications and dynamical cores. This submodule will eventually replace the Thompson parameterization currently in the CCPP after approval from all parties involved and significant testing.
This implementation is done in a way that will allow parallel testing of both TEMPO and the original Thompson microphysics.
The PR also adds the "hail-aware" component, which is 2-moment, predicted density graupel and a namelist flag for use (lthailaware).
Testing
Tested on Hera using Intel/GNU
No changes to baselines