{"payload":{"feedbackUrl":"https://github.com/orgs/community/discussions/53140","repo":{"id":78567085,"defaultBranch":"master","name":"MPAS-Model","ownerLogin":"jherwehe","currentUserCanPush":false,"isFork":true,"isEmpty":false,"createdAt":"2017-01-10T19:36:56.000Z","ownerAvatar":"https://avatars.githubusercontent.com/u/16904596?v=4","public":true,"private":false,"isOrgOwned":false},"refInfo":{"name":"","listCacheKey":"v0:1713383350.0","currentOid":""},"activityList":{"items":[{"before":"02ce76973c3c32bc4fbf0eeccaf63d55ad8d4770","after":"eb62cd1e4755ac18e5c7d3a1c6dbac86821f733c","ref":"refs/heads/develop","pushedAt":"2024-07-02T14:27:45.000Z","pushType":"push","commitsCount":143,"pusher":{"login":"jherwehe","name":"Jerry Herwehe","path":"/jherwehe","primaryAvatarUrl":"https://avatars.githubusercontent.com/u/16904596?s=80&v=4"},"commit":{"message":"Merge branch 'master' into develop\n\nThis merge introduces fixes from the release-v8.2.0 branch, and it connects the\nv8.2.0 tag to future commits on 'develop'.\n\n* master:\n  Fix instances of incorrect quotes in init_atmosphere and atmosphere registries\n  Add 'mp_thompson_aerosols' to list of possible_values for config_microp_scheme\n  Add 'sf_noahmp' to list of possible_values for config_lsm_scheme\n  Don't include FCINCLUDES in build options checked for build compatibility\n  Ignore the entire physics_mmm subdirectory of src/core_atmosphere/physics\n  Split physics source compilation from library updates for parallel builds\n  Add missing dependency among physics in MPAS-A main physics Makefile\n  Add 'sf_noahmp_in' package to Noah-MP static fields in atmosphere core registry\n  Add module search paths to support compilation of Noah-MP code with nvfortran\n  Update version number to 8.2.0\n  Improve check on deallocation of hash table in mpas_geotile_mgr_finalize\n  Add ONLY clause to USE statements for the 'mpi_f08' module\n  Add \"-check all\" to LDFLAGS_DEBUG for 'intel' build target","shortMessageHtmlLink":"Merge branch 'master' into develop"}},{"before":"f084b36f8ac82eb1e76c426d3572339c36523c77","after":"942d402417e2206353f4ec432fefd6b1ce5e3c96","ref":"refs/heads/master","pushedAt":"2024-07-02T14:11:25.000Z","pushType":"push","commitsCount":149,"pusher":{"login":"jherwehe","name":"Jerry Herwehe","path":"/jherwehe","primaryAvatarUrl":"https://avatars.githubusercontent.com/u/16904596?s=80&v=4"},"commit":{"message":"Merge branch 'release-v8.2.0'\n\nMPAS Version 8.2.0\n\nThis release of MPAS introduces several significant changes to MPAS-Atmosphere.\n\nNew physics\n\n * The Noah-MP v5.0.1 land-surface model is now available by setting\n   config_lsm_scheme = 'sf_noahmp' in the &physics namelist group.\n\n   - 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The PBL scheme includes the options needed to run the Eddy\n   Diffusivity Mass Flux (EDMF) scheme.\n\n * A separate driver for the parameterization of surface processes over sea-ice\n   points has been added.\n\n * The build system now tests for the availability of the modern 'mpi_f08'\n   module in the MPI library. If detected, the 'mpi_f08' module interface to\n   Fortran MPI routines will be used in favor of the older 'mpi' module\n   interface.\n\n * The atmosphere core now supports the storage and retrieval of time-invariant\n   fields in a separate I/O stream, offering significant disk space savings,\n   especially in cases where large ensembles or cycled simulations are being\n   run.\n\n * The top-level Makefile provides a new 'intel' build target for the Intel\n   oneAPI Fortran, C, and C++ compiler suite.\n\n * To support real-data simulations on meshes with grid distances approaching\n   1 km or less, the init_atmosphere core provides an option,\n   config_30s_supersample_factor, for super-sampling of the 30 arc-second\n   terrestrial fields (terrain, land use, soil category, and MODIS FPAR\n   monthly vegetation fraction).\n\n * When compiling, PRECISION=single is now the default, and double-precision\n   builds must be specified with PRECISION=double.","shortMessageHtmlLink":"Merge branch 'release-v8.1.0'"}},{"before":"cbbbb88f125b0469a63f343b460621c3e9c521c4","after":"90ab3ed8fa65f058600563fec95e87be42e9a2e0","ref":"refs/heads/atmosphere/develop-EPA_ACM2","pushedAt":"2024-04-17T20:32:02.000Z","pushType":"force_push","commitsCount":0,"pusher":{"login":"ldfowler58","name":null,"path":"/ldfowler58","primaryAvatarUrl":"https://avatars.githubusercontent.com/u/4108894?s=80&v=4"},"commit":{"message":"Add the ACM2 PBL scheme to MPAS-A\n\nThis EPA_ACM2 commit will add the ACM2 planetary boundary layer scheme\n(Pleim, 2007a; Pleim, 2007b) to MPAS-A as a new \"config_pbl_scheme\"\noption called \"bl_acm\".  The ACM2 PBL scheme code (module_bl_acm.F) was\nmigrated from WRFV4.4.1 with only minor changes and has been generalized\nto work with either MPAS or WRF.  Also refer to the ACM2 description in\nthe WRF-ARW technical document available at\nhttps://opensky.ucar.edu/islandora/object/opensky:2898 for an overview\nof the physics behind this option.\n\nNew file:\n  src/core_atmosphere/physics/physics_wrf/module_bl_acm.F\n\nModified files:\n  Makefile\n  src/core_atmosphere/Registry.xml\n  src/core_atmosphere/physics/mpas_atmphys_control.F\n  src/core_atmosphere/physics/mpas_atmphys_driver.F\n  src/core_atmosphere/physics/mpas_atmphys_driver_pbl.F\n  src/core_atmosphere/physics/mpas_atmphys_interface.F\n  src/core_atmosphere/physics/mpas_atmphys_packages.F\n  src/core_atmosphere/physics/mpas_atmphys_vars.F\n  src/core_atmosphere/physics/physics_wrf/Makefile\n\nThese EPA_ACM2 code changes to MPAS-A are based on the 22 August 2022\n\"develop\" branch of MPAS v7.3.\n\nReferences:\nPleim, J. E., 2007a:  A combined local and nonlocal closure model for\n  the atmospheric boundary layer. part I: Model description and testing.\n  J. Appl. Meteor. Climatol., 46, 13831395.\n  https://doi.org/10.1175/jam2539.1\nPleim, J. E., 2007b:  A combined local and nonlocal closure model for\n  the atmospheric boundary layer. part II: Application and evaluation in\n  a mesoscale meteorological model.  J. Appl. Meteor. 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The Pleim surface layer scheme code\n(module_sf_pxsfclay.F) was migrated from WRFV4.4.1 with only minor\nchanges and has been generalized to work with either MPAS or WRF.  Note\nthat this implementation of the Pleim surface layer in MPAS-A does not\nyet support fractional sea ice, in contrast to the other available\nsurface layer schemes.  The Pleim surface layer works with any LSM or\nPBL scheme, but is normally used in conjunction with the PX LSM and the\nACM2 PBL.  Refer to the description in the WRF-ARW technical document\navailable at https://opensky.ucar.edu/islandora/object/opensky:2898 for\nan overview of the physics behind this option.\n\nNew file:\n  src/core_atmosphere/physics/physics_wrf/module_sf_pxsfclay.F\n\nModified files:\n  Makefile\n  src/core_atmosphere/Registry.xml\n  src/core_atmosphere/physics/mpas_atmphys_control.F\n  src/core_atmosphere/physics/mpas_atmphys_driver_sfclayer.F\n  src/core_atmosphere/physics/physics_wrf/Makefile\n\nThese EPA_PXsfclay code changes to MPAS-A are based on the 22 August\n2022 \"develop\" branch of MPAS v7.3.\n\nReference:\nPleim, J. E., 2006: A simple, efficient solution of flux-profile\n  relationships in the atmospheric surface layer, J. Appl. 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The Pleim surface layer scheme code\n(module_sf_pxsfclay.F) was migrated from WRFV4.4.1 with only minor\nchanges and has been generalized to work with either MPAS or WRF.  Note\nthat this implementation of the Pleim surface layer in MPAS-A does not\nyet support fractional sea ice, in contrast to the other available\nsurface layer schemes.  The Pleim surface layer works with any LSM or\nPBL scheme, but is normally used in conjunction with the PX LSM and the\nACM2 PBL.  Refer to the description in the WRF-ARW technical document\navailable at https://opensky.ucar.edu/islandora/object/opensky:2898 for\nan overview of the physics behind this option.\n\nNew file:\n  src/core_atmosphere/physics/physics_wrf/module_sf_pxsfclay.F\n\nModified files:\n  Makefile\n  src/core_atmosphere/Registry.xml\n  src/core_atmosphere/physics/mpas_atmphys_control.F\n  src/core_atmosphere/physics/mpas_atmphys_driver_sfclayer.F\n  src/core_atmosphere/physics/physics_wrf/Makefile\n\nThese EPA_PXsfclay code changes to MPAS-A are based on the 22 August\n2022 \"develop\" branch of MPAS v7.3.\n\nReference:\nPleim, J. E., 2006: A simple, efficient solution of flux-profile\n  relationships in the atmospheric surface layer, J. Appl. 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Other KF\nenhancements include extending the KF look-up table (to prevent \"OUT OF\nBOUNDS\" errors being written to fort.98 file) and improving the DQEVAP\nand QICE calculations.  This version of module_cu_kfeta.F has also been\ngeneralized to work with either MPAS or WRF.\n\nModified files:\n  Makefile\n  src/core_atmosphere/Registry.xml\n  src/core_atmosphere/physics/mpas_atmphys_driver.F\n  src/core_atmosphere/physics/mpas_atmphys_driver_cloudiness.F\n  src/core_atmosphere/physics/mpas_atmphys_driver_convection.F\n  src/core_atmosphere/physics/mpas_atmphys_driver_radiation_lw.F\n  src/core_atmosphere/physics/mpas_atmphys_driver_radiation_sw.F\n  src/core_atmosphere/physics/mpas_atmphys_vars.F\n  src/core_atmosphere/physics/physics_wrf/module_cu_kfeta.F\n  src/core_atmosphere/physics/physics_wrf/module_ra_rrtmg_sw.F\nThese EPA_KF code changes to MPAS-A are based on the 22 August 2022\n\"develop\" branch of MPAS v7.3.\n\nReferences:\nBullock, O. R., K. Alapaty, J. A. Herwehe, and J. S. Kain, 2015:  A\n  dynamically computed convective time scale for the KainFritsch\n  convective parameterization scheme.  Monthly Weather Review, 143,\n  2105-2120.  https://doi.org/10.1175/MWR-D-14-00251.1\nHerwehe, J. A., K. Alapaty, T. L. Spero, and C. G. Nolte, 2014:\n  Increasing the credibility of regional climate simulations by\n  introducing subgrid-scale cloud-radiation interactions.  Journal of\n  Geophysical Research: Atmospheres, 119, 5317-5330.\n  https://doi.org/10.1002/2014JD021504\nAlapaty, K., J. A. Herwehe, T. L. Otte, C. G. Nolte, O. R. Bullock, M.\n  S. Mallard, J. S. Kain, and J. Dudhia, 2012:  Introducing subgrid-\n  scale cloud feedbacks to radiation for regional meteorological and\n  climate modeling.  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Other KF\nenhancements include extending the KF look-up table (to prevent \"OUT OF\nBOUNDS\" errors being written to fort.98 file) and improving the DQEVAP\nand QICE calculations.  This version of module_cu_kfeta.F has also been\ngeneralized to work with either MPAS or WRF.\n\nModified files:\n  Makefile\n  src/core_atmosphere/Registry.xml\n  src/core_atmosphere/physics/mpas_atmphys_driver.F\n  src/core_atmosphere/physics/mpas_atmphys_driver_cloudiness.F\n  src/core_atmosphere/physics/mpas_atmphys_driver_convection.F\n  src/core_atmosphere/physics/mpas_atmphys_driver_radiation_lw.F\n  src/core_atmosphere/physics/mpas_atmphys_driver_radiation_sw.F\n  src/core_atmosphere/physics/mpas_atmphys_vars.F\n  src/core_atmosphere/physics/physics_wrf/module_cu_kfeta.F\n  src/core_atmosphere/physics/physics_wrf/module_ra_rrtmg_sw.F\nThese EPA_KF code changes to MPAS-A are based on the 22 August 2022\n\"develop\" branch of MPAS v7.3.\n\nReferences:\nBullock, O. R., K. Alapaty, J. A. Herwehe, and J. S. Kain, 2015:  A\n  dynamically computed convective time scale for the KainFritsch\n  convective parameterization scheme.  Monthly Weather Review, 143,\n  2105-2120.  https://doi.org/10.1175/MWR-D-14-00251.1\nHerwehe, J. A., K. Alapaty, T. L. Spero, and C. G. Nolte, 2014:\n  Increasing the credibility of regional climate simulations by\n  introducing subgrid-scale cloud-radiation interactions.  Journal of\n  Geophysical Research: Atmospheres, 119, 5317-5330.\n  https://doi.org/10.1002/2014JD021504\nAlapaty, K., J. A. Herwehe, T. L. Otte, C. G. Nolte, O. R. Bullock, M.\n  S. Mallard, J. S. Kain, and J. Dudhia, 2012:  Introducing subgrid-\n  scale cloud feedbacks to radiation for regional meteorological and\n  climate modeling.  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