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With those in coupled run 37 (#367). That is, we don't want to use the above "non-CLUBB parameters". I expect this run to be out to lunch, but I want to see the impact of just the tau's code, on top of our existing coupled runs.
Case directory:
Locally (if still available):
/glade/p/cesmdata/cseg/runs/cesm2_0/$CASE
Description:
Same as #394, but replacing the non-clubb tunings:
!----non-CLUBB parameters
dust_emis_fact = 0.80D0
seasalt_emis_scale=1.5
micro_mg_dcs=0.00065
micro_mg_vtrmi_factor=1.25
microp_aero_wsubi_scale=1.0
microp_aero_wsub_scale = 0.01
zmconv_dmpdz=-0.0005
cldfrc_dp2=750
With those in coupled run 37 (#367). That is, we don't want to use the above "non-CLUBB parameters". I expect this run to be out to lunch, but I want to see the impact of just the tau's code, on top of our existing coupled runs.
Case directory:
Locally (if still available):
/glade/p/cesmdata/cseg/runs/cesm2_0/$CASE
On github:
https://github.com/NCAR/amwg_dev/tree/$CASE
Sandbox:
Locally (if still available):
/glade/work/hannay/cesm_tags/cesm2_3_alpha16b
On github: https://github.com/ESCOMP/cesm/tree/cesm2_3_alpha16b
Diagnostics:
Diags (if available)
https://webext.cgd.ucar.edu/BLT1850/$CASE/
Output:
Output (if still available):
/glade/derecho/scratch/hannay/archive/$CASE/
Contacts:
@cecilehannay @bstephens82
Extra details:
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