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Analysis code for paper: Changes in clouds and thermodynamics under solar geoengineering and implications for required solar reduction

Russotto, Rick

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    <dct:description>&lt;p&gt;Analysis and plotting scripts&amp;nbsp;for paper by R.D. Russotto and T.P. Ackerman in&amp;nbsp;&lt;em&gt;Atmos. Chem. Phys.&lt;/em&gt;&amp;nbsp;special issue on the Geoengineering Model Intercomparison Project.&lt;/p&gt; &lt;p&gt;DOI for paper:&amp;nbsp;&lt;a href="https://doi.org/10.5194/acp-2018-345"&gt;10.5194/acp-2018-345&lt;/a&gt;&lt;/p&gt; &lt;p&gt;Python code was written by Rick Russotto. The APRP.py module was based in part on Matlab scripts provided by Yen-Ting Hwang. The vertical regridding code was based in part on the &amp;quot;convert_sigma_to_pres&amp;quot;&amp;nbsp;algorithm by Dan Vimont, available at&amp;nbsp;&lt;a href="http://www.aos.wisc.edu/~dvimont/matlab/"&gt;http://www.aos.wisc.edu/~dvimont/matlab/&lt;/a&gt;.&lt;/p&gt; &lt;p&gt;If you use any of this code, please acknowledge where it came from.&lt;/p&gt; &lt;p&gt;Python scripts were run using Python 2.7.9. Versions of packages used:&amp;nbsp;&lt;br&gt; -Matplotlib 1.5.1&amp;nbsp;&lt;br&gt; -NumPy 1.8.2&amp;nbsp;&lt;br&gt; -NetCDF4 1.1.0&lt;/p&gt; &lt;p&gt;&amp;nbsp;&lt;/p&gt; &lt;p&gt;Which scripts make which figures in the paper:&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Figure 1:&amp;nbsp;&lt;/strong&gt;&lt;br&gt; isG1ReductionCorrelatedWithECS.py&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Figure 2:&amp;nbsp;&lt;/strong&gt;&lt;br&gt; taZonalMeanProfiles.py&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Figure 3:&amp;nbsp;&lt;/strong&gt;&lt;br&gt; husZonalMeanProfiles.py&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Figure 4:&amp;nbsp;&lt;/strong&gt;&lt;br&gt; cloudFractionZonalMeanProfiles.py&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Figure 5:&amp;nbsp;&lt;/strong&gt;&lt;br&gt; multiModelMeanCloudsV2.py&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Figure 6:&amp;nbsp;&lt;/strong&gt;&lt;br&gt; multiModelMeanPredictorsV2.py&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Figure 7:&amp;nbsp;&lt;/strong&gt;&lt;br&gt; multiModelMeanAPRP.py&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Figures 8, S9, S10, S11:&amp;nbsp;&lt;/strong&gt;&lt;br&gt; analyzeKernelResults.py&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Figures 9, S12:&amp;nbsp;&lt;/strong&gt;&lt;br&gt; mapLWCRE.py&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Figures 10, 11:&amp;nbsp;&lt;/strong&gt;&lt;br&gt; barGraphsV2.py&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Figures S1, S2, S3:&amp;nbsp;&lt;/strong&gt;&lt;br&gt; cloudFractionMaps.py&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Figures S4, S5:&amp;nbsp;&lt;/strong&gt;&lt;br&gt; lowCloudPredictorMaps.py&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Figures S6, S7, S8:&amp;nbsp;&lt;/strong&gt;&lt;br&gt; scriptUsingAPRPonGeoMIP.py&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Figure S13:&lt;/strong&gt;&lt;br&gt; rapidVsFeedbackAPRP.py&lt;/p&gt; &lt;p&gt;&lt;strong&gt;Other scripts and modules that the above scripts depend on:&amp;nbsp;&lt;/strong&gt;&lt;br&gt; APRP.py&amp;nbsp;&lt;br&gt; calculateClimatologiesForRadiativeKernels.py&amp;nbsp;&lt;br&gt; correctCESM_rlut.py&amp;nbsp;&lt;br&gt; find_rlut_correction.py&amp;nbsp;&lt;br&gt; geomipFunctions.py&amp;nbsp;&lt;br&gt; saveModelLatsLons.py&amp;nbsp;&lt;br&gt; zonalMeanCloudFraction_CSIRO.py&amp;nbsp;&lt;br&gt; zonalMeanCloudFraction_HadGEM2-ES.py&amp;nbsp;&lt;/p&gt; &lt;p&gt;&amp;nbsp;&lt;/p&gt; &lt;p&gt;A standalone version of the APRP code can be found at&amp;nbsp;&lt;a href="https://github.com/rdrussotto/pyAPRP"&gt;https://github.com/rdrussotto/pyAPRP&lt;/a&gt;, with further documentation.&lt;/p&gt;</dct:description>
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