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planets_rt [2012/02/28 18:40] – [28 Feb 2012] statiaplanets_rt [2012/02/28 19:37] – [28 Feb 2012] statia
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 **tau_gas.pro:** **tau_gas.pro:**
       - test katherine's new code for ch4 coefficients       - test katherine's new code for ch4 coefficients
-      - update tau gas to take any combination of input param files as strings? This would allow use of new param files, and multiple wavelength ranges to be specified. It would make code more transparent to outside user.+      - update makeparfile take any combination of input param files as strings? This would allow use of new param files, and multiple wavelength ranges to be specified. It would make code more transparent to outside user.
       - incorporate all needed functions/files into one program (e.g. all rayleigh scattering, nh3 absorption, h2h2, etc coefficients covering relevent T and frequency)       - incorporate all needed functions/files into one program (e.g. all rayleigh scattering, nh3 absorption, h2h2, etc coefficients covering relevent T and frequency)
       - NH3 absorption: need to figure out why we'd want to use band models to get k coefficients. Is there a difference between the band model answer and the sromovsky answer? Why? Code in best choice.        - NH3 absorption: need to figure out why we'd want to use band models to get k coefficients. Is there a difference between the band model answer and the sromovsky answer? Why? Code in best choice. 

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