MPAS-Dev/MPAS-Model: MPAS Version 7.2
Authors/Creators
- Michael Duda1
- Doug Jacobsen2
- Mark Petersen3
- Matt Hoffman3
- Adrian K. Turner
- ldfowler58
- Xylar Asay-Davis3
- Todd Ringler
- Phillip J. Wolfram
- Luke Van Roekel4
- William Lipscomb1
- stephenprice
- skamaroc
- Nicole Jeffery
- Dom Heinzeller5
- Jon Woodring4
- maltrud
- Juan Saenz
- Miles Curry6
- Nick7
- weiwangncar
- mperego
- Kelly Werner1
- Jon Wolfe4
- Azamat Mametjanov
- Phil Jones3
- Bill Arndt8
- JJ Guerrette9
- Soyoung Ha10
- Tong Zhang
- 1. National Center for Atmospheric Research
- 2. @Google
- 3. Los Alamos National Laboratory
- 4. LANL
- 5. National Oceanic and Atmospheric Administration, Earth System Research Laboratory, Global Systems Division
- 6. UCAR/NCAR - MMM
- 7. OU
- 8. Berkeley National Laboratory
- 9. NCAR/MMM
- 10. NCAR
Description
This minor release addresses several issues in the MPAS-Atmosphere model.
MPAS-Atmosphere: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.
Files
MPAS-Dev/MPAS-Model-v7.2.zip
Files
(4.4 MB)
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Additional details
Related works
- Is supplement to
- https://github.com/MPAS-Dev/MPAS-Model/tree/v7.2 (URL)