[4773] | 1 | *** BASIC TEST *** |
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| 2 | |
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| 3 | This file contains |
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| 4 | "ckdmip_evaluation1_concentrations_present_reduced.nc", the 50 |
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| 5 | clear-sky atmospheric profiles of the CKDMIP "Evaluation-1" dataset |
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| 6 | described by Hogan and Matricard (GMDD 2020), and the corresponding |
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| 7 | line-by-line fluxes in |
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| 8 | "ckdmip_evaluation1_lw_fluxes_present_reduced.nc" and |
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| 9 | "ckdmip_evaluation1_sw_fluxes_present_reduced.nc". |
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| 10 | |
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| 11 | Type "make" in this directory to run ecRad on these profiles. You |
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| 12 | will need the nco tools, because the shortwave calculation is |
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| 13 | performed five times for different solar zenith angles and the results |
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| 14 | are concatenated into one file. |
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| 15 | |
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| 16 | Then run the Matlab script "do_evaluate_ecrad.m" to evaluate the ecRad |
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| 17 | calculations against line-by-line, producing plots in the same style |
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| 18 | as Figs. 5 and 7 of Hogan and Matricardi (2020). |
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| 19 | |
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| 20 | By default the ecCKD gas optics is used: to use RRTMG, use instead |
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| 21 | "make GASMODEL=rrtmg", which uses the namelist file config-rrtmg.nam |
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| 22 | instead of config-ecckd.nam. To use a different spectral |
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| 23 | configuration file with ecCKD, edit config-ecckd.nam. |
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| 24 | |
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| 25 | |
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| 26 | *** CKDMIP SCENARIOS *** |
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| 27 | |
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| 28 | To run ecRad on a wider range of CKDMIP scenarios, first download a |
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| 29 | selection of concentration files from the CKDMIP FTP site to the |
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| 30 | "concentrations" directory: |
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| 31 | |
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| 32 | make download |
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| 33 | |
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| 34 | This also downloads the line-by-line reference fluxes to "lbl_fluxes". |
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| 35 | Then run ecRad on them using ecCKD gas optics with: |
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| 36 | |
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| 37 | make scenarios |
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| 38 | |
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| 39 | This generates *_lw_fluxes_* and *_sw_fluxes_* files in the "fluxes" |
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| 40 | directory. |
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| 41 | |
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| 42 | Or with the following you can use RRTMG gas optics: |
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| 43 | |
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| 44 | make GASMODEL=rrtmg scenarios |
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| 45 | |
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| 46 | You can clean up with "make clean" or delete any downloaded files with |
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| 47 | "make distclean". |
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