Simulating gas giant exoplanet atmospheres with Exo-FMS: comparing semigrey, picket fence, and correlated-k radiative-transfer schemes

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:...

Detaylı Bibliyografya
Asıl Yazarlar:	Lee, EKH, Parmentier, V, Hammond, M, Grimm, SL, Kitzmann, D, Tan, X, Tsai, S-M, Pierrehumbert, RT
Materyal Türü:	Journal article
Dil:	English
Baskı/Yayın Bilgisi:	Royal Astronomical Society 2021

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