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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