Hello, I would like to do some radiative transfer modeling for Venus. I want to see about what percentage of photons emitted from the surface of Venus get scattered/absorbed at various altitudes. The wavelengths I'm interested in are NIR, 0.7-1.5 microns. Would ART provide reasonable estimates at these wavelengths?
Thanks, -- Joshua Knicely (he/him/his) Ph.D. Candidate, University of Alaska Fairbanks
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