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Merge b4b-dev (2024-10-10) #2829

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merged 30 commits into from
Oct 11, 2024
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Commits on Jun 26, 2024

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Commits on Aug 8, 2024

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Commits on Aug 22, 2024

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Commits on Sep 27, 2024

  1. Merge tag 'ctsm5.3.002' into merge-master-20240927

    Same as ctsm5.3.001
    
    I made an accidental merge and reverted it.
    slevis-lmwg committed Sep 27, 2024
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  2. Merge pull request ESCOMP#2797 from slevis-lmwg/merge-master-20240927

    Merge ctsm5.3.002 to b4b-dev
    slevis-lmwg authored Sep 27, 2024
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  3. Fix clm-basic tests

    slevis-lmwg committed Sep 27, 2024
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Commits on Sep 28, 2024

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Commits on Sep 30, 2024

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Commits on Oct 1, 2024

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  3. Merge pull request ESCOMP#2799 from slevis-lmwg/change_t061_to_t232

    Change testlist_clm ne30pg3_t061 tests to ne30pg3_t232
    slevis-lmwg authored Oct 1, 2024
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  5. Merge pull request ESCOMP#2804 from slevis-lmwg/alloc_elevclass_o

    Remove unused variable elevclass_o in mkglcmecMod.F90
    slevis-lmwg authored Oct 1, 2024
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  8. Correct the name of the hash to use in the checks that hash values ar…

    …e all set in fail, warn, and finidat tests
    ekluzek committed Oct 1, 2024
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  9. Merge pull request ESCOMP#2678 from mvdebolskiy/fix-namelist-tester

    Add check in build-namelist_test.pl
    ekluzek authored Oct 1, 2024
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Commits on Oct 4, 2024

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Commits on Oct 8, 2024

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  2. Fix issue ESCOMP#2793

    olyson committed Oct 8, 2024
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  3. Merge pull request ESCOMP#2627 from jedwards4b/shr_file_to_shr_log

    move from depricated shr_file to shr_log
    samsrabin authored Oct 8, 2024
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  4. Merge pull request ESCOMP#2806 from olyson/eflxbuild

    Set eflx_building_lun to spval properly
    olyson authored Oct 8, 2024
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Commits on Oct 10, 2024

  1. Merge tag 'ctsm5.3.005' into merge-b4bdev-20241010

    Hardcoded tuning adjustments for Leung_2024 dust emissions
    
    Changes to dust emissions when Leung_2024 method is being used.
    
    Tuning was needed since we saw some high biases in dust over semiarid
    regions given all the updates in CTSM and CAM. The biggest
    changes in CTSM that affects dust is an increase in friction velocity
    (ustar; fv in CTSM) over vegetated, semiarid regions, mainly
    due to a switch in the roughness scheme from 'ZengWang2007' to
    'Meier2022'. Since dust emission is very sensitive to ustar, the dust
    emission scheme magnifies this increase and caused strong high biases
    over semiarid regions, including Australia and Patagonia (see
    plots in issue ESCOMP#2732). To enhance the robustness of Leung_2023 and
    reduce the likelihood to see huge changes in answers in the
    future, we tried to limit the sensitivity of dust emissions to ustar. We
    also tried different methods (see specific notes below) to
    reduce dust emissions from semiarid regions given the high biases over
    there.
    samsrabin committed Oct 10, 2024
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Commits on Oct 11, 2024

  1. Update ChangeLog/ChangeSum.

    samsrabin committed Oct 11, 2024
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