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Experimental Clouds
nabajour edited this page Jul 9, 2020
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Clouds are defined by a global fcloud parameter, and a cloud file.
The cloud file is a table per wavelength bins, which means that the same parameters are applied to the whole atmosphere for each wavelength bin.
fcloud parameter could become a local parameter, which would need to be computed at the beginning of the loop.
cloud absorption, scattering, asymetry could be localised instead of using a single value per wavelength.
Here are the steps to follow to extend this:
- replace input table per wavelength by input lookup table per wavlength, pressure, temperature, etc…
- add a table of this value per volume element and wavelength bin.
- add an interpolation function similar to the ones used for gas properties.
- change code in
trans_iso
andtrans_noniso
to use per volume element table instead of direct lookup table access.