Simulating gas giant exoplanet atmospheres with Exo-FMS: comparing semigrey, picket fence, and correlated-k radiative-transfer schemes
Radiative-transfer (RT) is a fundamental part of modelling exoplanet atmospheres with general circulation models (GCMs). An accurate RT scheme is required for estimates of the atmospheric energy transport and for gaining physical insight from model spectra. We implement three RT schemes for Exo-FMS:...
| Prif Awduron: | , , , , , , , |
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| Fformat: | Journal article |
| Iaith: | English |
| Cyhoeddwyd: |
Royal Astronomical Society
2021
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