ASCL Code Record
[ascl:2210.008]
RADTRAN: General purpose planetary radiative transfer model
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.
- Code site:
- https://github.com/nemesiscode/radtrancode https://nemesiscode.github.io/nemesis.html
- Described in:
- https://ui.adsabs.harvard.edu/abs/1997AdSpR..19.1149I
- Bibcode:
- 2022ascl.soft10008I
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