RADTRAN: General purpose planetary radiative transfer model
Abstract
RADTRAN calculates the transmission, absorption or emission spectra emitted by planetary atmospheres using either line-by-line integration, spectral band models, or 'correlated-K' approaches. Part of the NEMESIS project (ascl:2210.009), the code also incorporates both multiple scattering and single scattering calculations. RADTRAN is general purpose and not hard-wired to any specific planet.
- Publication:
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Astrophysics Source Code Library
- Pub Date:
- October 2022
- Bibcode:
- 2022ascl.soft10008I
- Keywords:
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- Software