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pull request versão MPAS_GPU 8.2.2
…rsion 8.2.2. Modified files: modified: Makefile modified: README.md modified: src/core_atmosphere/Registry.xml modified: src/core_atmosphere/physics/mpas_atmphys_lsm_noahmpinit.F modified: src/core_init_atmosphere/Registry.xml modified: src/core_init_atmosphere/mpas_init_atm_cases.F modified: src/core_init_atmosphere/mpas_init_atm_thompson_aerosols.F modified: src/framework/mpas_block_creator.F modified: src/framework/mpas_bootstrapping.F modified: src/framework/mpas_io.F
deleted: load_monan_app_modules.sh deleted: make.output deleted: make.sh deleted: monan_readme.md
- Merge MPAS 8.3.0 - Change doc -> docs - Change test -> testing_and_setup - Add cmake/ folder - Physics scheme in the "physics_mmm" and "physics_noaa" (src/core_atmosphere/physics/) directory are now obtained from a separate, shared MMM-physics and NOAA-GSL repository at compile time using the manage_externals tool (configuration file: /src/core_atmosphere/Externals.cfg).
File changed: src/core_init_atmosphere/mpas_init_atm_cases.F
. This development contains further configuration for the pre-operational MONAN global 10km uniform resolution, adapted to run on the new CRAY supercomputer. It contains new tuning for the GF scheme and sets WSM6 as the default cloud microphysics parameterization. For this configuration, the namelist.atmosphere should be set to config_physics_suite = 'mesoscale_reference_monan'.
PR Feature 757 com a Release/1.3.0 rc_merge
PR Feature 757_130rc com a Release/1.3.1 rc_merge
PR Feature 757_131rc com a Release/1.4.0 rc_merge
PR Feature 757_140rc com a Release/1.4.1 rc_merge
PR Feature 757_141rc com a Release/1.4.2 rc_merge
PR Feature 757_142rc com a Release/1.4.3 rc_merge
…_c143rc_merge Feature/monan 757 nf c143rc merge com a develop_gpu
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Pull Request Description
_Describe what this Pull Request contains and the changes made.
This GF version includes a new formulation for the gross entrainment rate that depends on the model grid spacing. This may help a smoother transition from non-resolved to resolved scales (grey-zone for deep convection). Also, this formulation, together with the cold-pool parameterization, significantly improves the organization of convection over tropical regions.
So, I decided to use this version as the starting point to retuning MPAS/MONAN 2.0 for the next candidate for regional and global operation on a medium-range time scale.
to do
Version 2.0 should default to the new land surface (NOAH_MP) and Gravity Wave Drag (UGWP). In this way, the suites 'mesoscale_reference_monan' and 'convection_permitting_monan' must select (in mpas_atmphys_control.F)
config_lsm_scheme = 'sf_noahmp'
config_gwdo_scheme = 'bl_ugwp_gwdo'
Type of Change
Testing and Quality
Scientific Impact
This GF version includes a new formulation for the gross entrainment rate that depends on the model grid spacing (Zhao et al 2024, GRL https://doi.org/10.1029/2024GL110735). This may help a smoother transition from non-resolved to resolved scales (grey-zone for deep convection). Also, this formulation, together with the cold-pool parameterization, significantly improves the organization of convection over tropical regions (Freitas, 2024 JAMES and 2026 WCO5).