projects:3dcats:wp200_intercomp_cloud []

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==== MYSTIC results including cloud for model intercomparison ====

This data includes the molecular optical thickness provided by Huan (moltau_400_500_u76_EuropeNO2.nc):

{{:projects:3dcats:wp_200:mystic_400_500_v2.nc|Results for 400-500 nm}}

{{:projects:3dcats:wp_200:mystic_400_500_v20200625.nc|Results for 400-500 nm, including more sza and albedo values}}

This data includes the molecular optical thickness provided by Huan (HITRAN2016_moltau_755_775_u76.nc)

{{:projects:3dcats:wp_200:mystic_o2a_v2.nc|Results for 755-775 nm, Heney-Greenstein phase function}}

{{:projects:3dcats:wp_200:mystic_o2a_v3.nc|Results for 755-775 nm, Mie optical properties}}

{{:projects:3dcats:wp_200:mystic_o2a_v20200625.nc|Results for 755-775 nm, Mie optical properties, including more sza and albedo values}}

{{:projects:3dcats:wp_200:mystic_o2a_reptran_orig_geom.nc|Results for 755-775 nm, Mie optical properties, REPTRAN band averages.}}

Here I have included different geometry settings to better understand the non-isotropic scattering by the cloud layer:\\ szas=[60], vzas=arange(0,81,5),vaas=[0,180], all simulations with Mie phase function.

All viewing directions are in the solar principal plane. 

{{:projects:3dcats:wp_200:mystic_400_500_v3.nc|Results for 400-500 nm, results in solar principal plane}}

{{:projects:3dcats:wp_200:mystic_o2a_reptran_bands.nc|Results averaged over three wavelength bands, solar principal plane.}}

{{:projects:3dcats:wp_200:mystic_o2a_pp.nc|Line-by-line simulation for O2A-band, solar principal plane.}}

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