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Updates branch with changes from NOAA-EMC:develop #3
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dustinswales
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Updates branch with changes from NOAA-EMC:develop #3
dustinswales
wants to merge
15
commits into
grantfirl:feature/rad-fix_gjf
from
dustinswales:feature/rad-fix_djs
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…uid potential temperature in local mixing of GFSPBL NOAA-EMC#977 (NOAA-EMC#963) * 3D-TKE EMDF GFS PBL scheme related changes from FIU (Ping Zhu, [email protected]). * Update changes in 3d TKE scheme * Add an option to use liquid potential temperature in temperature equation of GFS PBL scheme. (from @WeiguoWang-NOAA) * Update sa3dtke variables standard names * Update submodule physics for sa3dtke nonlocal mixing and stylistic coding * Update SA3DTKE variables names * Update submodules physics for SA3DTKE nonlocal mass-flux transport
…ture/rad-fix_djs
* Add fv3_cap unit tests and general unit test modificaitons
…stationary GWD changes, other misc. physics changes) (NOAA-EMC#950) * modified two ecmwf ngwd related files * modify comment with ngwd algorithm * use FMS version of get_tracer_index in GFS_typedefs * fix get_tracer_index calls with MODEL_ATMOS * fix integer underflow in control_scavenging_initialize * add ccpp/physics submodule change due to need for CMakeLists.txt change for FMS usage in GFS_typedefs.F90 * add wrapper for FMS version of get_tracer_index to handle large negative NO_TRACER value --------- Co-authored-by: bo yang <[email protected]>
* removed gfdl mp v1 files from orginal directory and moved to newly aded v1 directory * add GFDLMP v3 * Update GFDLMPV3 based SDFs * Support for TEMPO aerosol-aware hail-aware in CCPP * Update TEMPO SDF --------- Co-authored-by: Ruiyu Sun <[email protected]> Co-authored-by: Anders Jensen <[email protected]> Co-authored-by: Grant Firl <[email protected]> Co-authored-by: dustinswales <[email protected]>
* Added do_canopy option. * Added canopy variables to GFS typdefs and diagnostic codes. * Removed ozphys_2015 in GFSv16 physics suite file. * Import 5 canopy arrays and 3 photdiag arrays from AQM
…ture/rad-fix_djs
… SFS) (NOAA-EMC#990) * MERRA2 3 hourly forcing * Ensure qv photochemistry diagnostics are only in runs with qv photochemistry. * activate dx threshold to use the prognostic closure in saSAS convection for resolutions coarser than 30km: SFSv1. --------- Co-authored-by: anning.cheng <[email protected]> Co-authored-by: Daniel Wesloh <[email protected]> Co-authored-by: Lisa Bengtsson <[email protected]>
…ture/rad-fix_djs
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All changes are to the physics. See description in physics PR.