Simulations
SE dycore
ID | Casename | Case Description | Diagnostics | Details/Comments |
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AA0 | b.e11.B1850C5CN.f09_g16.005 | Large-ensemble |
timeseries (1-200) |
Comments: |
AA1 | b.e12.B1850C5CN.ne30_g16.init.ch.001 | Coupled run with CESM1.2.0 out of the box + hybrid from b.e12.B1850C5CN.ne30_g16.control.022 at yr 145 |
timeseries w/ obs |
Comments: |
AA2 | b.e12.B1850C5CN.ne30_g16.init.ch.002 | Same as AA1 + ocean coupling frequency set to 2 hours |
timeseries w/ obs w/ AA1 |
Comments: ./xmlchange -file env_run.xml -id OCN_NCPL -val 12 ./xmlchange -file env_run.xml -id ROF_NCPL -val 12 Gokhan hopes this configuration will produce a slight warming of the SSTs (by adding a diurnal cycle) This doesn't have the expected effect. SSTS are slightly warmer but the TOA balance is off by almost 0.5 Wm/2. |
AA3 | b.e12.B1850C5CN.ne30_g16.init.ch.003 | Same as AA1 |
Comments: Retuning to balance TOA |
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AA4 | b.e12.B1850C5CN.ne30_g16.init.ch.004 | Same as AA3 + the wind stress seen by the ocean is reduced by 30% south of 35S. |
timeseries w/ obs w/ AA3 |
Comments: the wind stress seen by the ocean is reduced by 30% south of 35S. |
AA5 | b.e12.B1850C5CN.ne30_g16.init.ch.005 | Same as AA3 + start from Levitus |
Comments: None |
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AA6 | b.e12.B1850C5CN.ne30_g16.init.ch.006 | Same as AA3 + start from Large ensemble at year 400 |
Comments: None |
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AA9 | b.e12.B1850C5CN.ne30_g16.init.ch.009 | Same as AA5 start from Levitus + rhminl = 0.8935D0->0.8895D0 + rhminl = 0.8895D0->0.884D0 (at year 49) |
Comments: None |
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AA12 | b.e12.B1850C5CN.ne30_g16.init.ch.012 | Same as AA9 start using spunup ocean at year 402 + rhminl = 0.8935D0->0.885D0 |
timeseries |
Comments: None |
AA13 | b.e12.B1850C5CN.ne30_g16.init.ch.013 | Same as AA9 start from core + rhminl = 0.8935D0->0.885D0 |
Comments: None |
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AA14 | b.e12.B1850C5CN.ne30_g16.init.ch.014 | Same as AA3 hybrid from AA3 + using spunup ocean at year 402 + rhminl = 0.8935D0->0.885D0 |
Comments: None |
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AA15 | b.e12.B1850C5CN.ne30_g16.init.ch.015 | Same as AA9 + the wind stress seen by the ocean is reduced by 30% south of 35S. |
timeseries
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Comments: None |
AA16 | b.e12.B1850C5CN.ne30_g16.init.ch.016 | Start from Levitus in SE + spunup land from AA3 at year 147 + rhimnl = 0.884 (value from AA9) + extra output from ocean |
Comments: None |
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AA17 | b.e12.B1850C5CN.ne30_g16.init.ch.017 | Start from Levitus in FV + extra output from ocean |
Comments: I forgot to change the casename to "f09" |
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AA19 | b.e12.B1850C5CN.ne30_g16.init.ch.019 | Start from Levitus in SE + attempt to change vertical mixing |
Comments:
1) Add the following to user_nl_pop2 vmix_choice = 'const' 2) Copy the following files from /glade/p/work/mlevy/cases/C.const_mixing.cesm1_2_0/SourceMods/src.pop2 to your SourceMods/src.pop2 directory i) gx1v6_tavg_contents -- this is the list of all variables output by POP, and I removed the ones that are specific to KPP ii) ocn.base.tavg.csh -- this file controls how many stream functions POP should output... by default there are 3, but I think the 3rd file only contains KPP-specific variables, so I changed it to 2 streams. For the experiment you described (changing the kappa term in the diffusion equation), add the following two lines to user_nl_pop2: const_vdc = [new value; old value is 0.25] I was able to run for 5 days with the default (0.25) values as well as dropping down to 0.2; that's all the testing I did to make sure these code-mods wouldn't break anything.
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AA20 | b.e12.B1850C5CN.ne30_g16.init.ch.020 | Start from Levitus in SE + spunup land from AA3 at year 147 + rhimnl = 0.884 (value from AA9) + dust_emis_fact = 0.35D0 (same as in FV) + extra output from ocean |
Comments: None |
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AA21 | b.e12.B1850C5CN.ne30_g16.init.ch.021 | Start from Levitus in SE + mapping files (see details) |
Comments: atm2ocn_fmapname = '/glade/p/cesmdata/cseg/inputdata/cpl/gridmaps/ne30np4/map_ne30np4_TO_gx1v6_aave.130522.nc' atm2ocn_smapname = '/glade/p/cesmdata/cseg/inputdata/cpl/gridmaps/ne30np4/map_ne30np4_TO_gx1v6_blin.130522.nc' atm2ocn_vmapname = '/glade/p/cesmdata/cseg/inputdata/cpl/gridmaps/ne30np4/map_ne30np4_TO_gx1v6_patc.130522.nc' ocn2atm_fmapname = '/glade/p/cesmdata/cseg/inputdata/cpl/gridmaps/gx1v6/map_gx1v6_TO_ne30np4_aave.130522.nc' ocn2atm_smapname = '/glade/p/cesmdata/cseg/inputdata/cpl/gridmaps/gx1v6/map_gx1v6_TO_ne30np4_aave.130522.nc' |
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AA22 | b.e12.B1850C5CN.ne30_g16.init.ch.022 | Start from Levitus in SE + changes from gohkan to modify TAUX seen by ocean |
Comments: doesn't work properly |
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AA23 | b.e12.B1850C5CN.ne30_g16.init.ch.023 | Start from Levitus in SE + turn TMS off |
Comments: |
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AA24 | b.e12.B1850C5CN.ne30_g16.init.ch.024 | Start from Levitus in SE + tms_orocnst = 1.0->2.0D0 |
Comments: |
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AA25 | b.e12.B1850C5CN.ne30_g16.init.ch.025 | Start from Levitus in SE + old SE topo (smooth): |
Comments: |
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AA26 | b.e12.B1850C5CN.ne30_g16.init.ch.026 | Start from Levitus in SE + hdsp(i) = 4.0_r8 * sgh(i) |
Comments: |
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AA27 | b.e12.B1850C5CN.ne30_g16.init.ch.027 | Start from Levitus in SE |
Comments: |
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AA28 | b.e12.B1850C5CN.ne30_g16.init.ch.028 | Start from Levitus in SE |
Comments: |
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AA29 | b.e12.B1850C5CN.ne30_g16.init.ch.029 | Start from Levitus in SE |
Comments: |
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AA31 | b.e12.B1850C5CN.poles_30x4_g16.init.ch.031 | Start from Levitus in SE |
Comments: |
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AA32 | b.e12.B1850C5CN.ne30_g16.init.ch.032 | Start from Levitus in SE |
Comments: |
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AA34 | b.e12.B1850C5CN.poles_30x4_g16.init.ch.034 | Same as AA16: + min(kappa_{iso,thic}) = 600 m^2/s |
timeseries |
Comments: |
AA35 | b.e12.B1850C5CN.poles_30x4_g16.init.ch.035 | Same as AA16: + min(kappa_thic) = 600 m^2/s, min(kappa_iso) = 1200 m^2/s |
timeseries |
Comments: |
AA36 | b.e12.B1850C5CN.poles_30x4_g16.init.ch.036 | Same as AA16: + min(kappa_{iso,thic}) = 600 m^2/s and KPP modification (stability-dependent surface layer depth) |
timeseries |
Comments: |