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This merge addresses several issues in the MPAS-Atmosphere model. Specifically, this merge introduces the following fixes: - Correct the use of uninitialized memory in the init_atm_case_squall_line routine by initializing the qvb array to zero before its first use. - Fix a bug in the vertical extrapolation of relative humidity and specific humidity to model levels below the lowest first-guess level when first-guess levels are given in top-to-bottom order in the input intermediate file. - Fix reproducibility issues in several fields within the Noah LSM over land-ice points when running with different MPI task counts; however, only one of these fields -- smstav, the surface moisture availability field -- persists outside of the physics driver and is written to MPAS-Atmosphere restart files. - Correct the units and description attributes for the GWDO fields var2d, con, oa1, oa2, oa3, oa4, ol1, ol2, ol3, and ol4 in both the init_atmosphere and atmosphere core Registry.xml files. - Add code that had inadvertently been omitted for computing dtheta_dt_mp, the potential temperature heating rate from microphysics. Prior to this change, the dtheta_dt_mp field would always contain a constant zero value when written to model output files. - Correct a check on the availability of the dtheta_dt_mix variable when computing depv_dt_mix in the PV diagnostics module. - Correct the parallel computation of iLev_DT (and other fields that depend on it, including u_pv, v_pv, theta_pv, vort_pv, depv_dt_diab_pv, and depv_dt_fric_pv) in the PV diagnostics module. * hotfix-v7.2: Correct units and descriptions for GWDO fields var2d, con, oa[1-4], ol[1-4] Halo exchange inTropo in flood fill to find DT. Fix parallel reproducibility error in 'smstav' field Correct check on availability of dtheta_dt_mix when computing depv_dt_mix Fix bug in vertical interp of r.h. and s.h. when levels are given top-to-bottom Initialize qvb to zero before its first use in init_atm_case_squall_line Remove redundant mpas_pool_get_array calls for dtheta_dt_mp computation Use dt_dyn rather than dt_microp when computing dtheta_dt_mp Remove trailing whitespace and adjust indentation of dtheta_dt_mp computation Obtain 'rvord' from mpas_constants for computation of dtheta_dt_mp Increment version number to 7.2 Calculate dtheta_dt_mp by finite difference around microphysics call.
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MPAS-v7.1 | ||
MPAS-v7.2 | ||
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The Model for Prediction Across Scales (MPAS) is a collaborative project for | ||
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