Differences
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| Both sides previous revisionPrevious revision | Next revisionBoth sides next revision | ||
| planets_rt [2012/02/28 18:37] – statia | planets_rt [2012/02/28 18:40] – [28 Feb 2012] statia | ||
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| - 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. | ||
| - make tau_gas work with structure input and output | - make tau_gas work with structure input and output | ||
| + | |||
| + | **tau_haze.pro** | ||
| + | - make into a structure | ||
| + | - allow for particle size distribution for calculating mie scattering | ||
| + | - Lots of questions to answer: how do we specify things? Where are the calculations done? Do we want to fit for g,w, and asym and back out particle properties, or the other way around? | ||
| **spectrum fitting:** | **spectrum fitting:** | ||
