Modeling the surface temperature of earth-like planets
The Astrophysical Journal, 2015•iopscience.iop.org
We introduce a novel Earth-like planet surface temperature model (ESTM) for habitability
studies based on the spatial–temporal distribution of planetary surface temperatures. The
ESTM adopts a surface energy balance model (EBM) complemented by: radiative–
convective atmospheric column calculations, a set of physically based parameterizations of
meridional transport, and descriptions of surface and cloud properties more refined than in
standard EBMs. The parameterization is valid for rotating terrestrial planets with shallow …
studies based on the spatial–temporal distribution of planetary surface temperatures. The
ESTM adopts a surface energy balance model (EBM) complemented by: radiative–
convective atmospheric column calculations, a set of physically based parameterizations of
meridional transport, and descriptions of surface and cloud properties more refined than in
standard EBMs. The parameterization is valid for rotating terrestrial planets with shallow …
Abstract
We introduce a novel Earth-like planet surface temperature model (ESTM) for habitability studies based on the spatial–temporal distribution of planetary surface temperatures. The ESTM adopts a surface energy balance model (EBM) complemented by: radiative–convective atmospheric column calculations, a set of physically based parameterizations of meridional transport, and descriptions of surface and cloud properties more refined than in standard EBMs. The parameterization is valid for rotating terrestrial planets with shallow atmospheres and moderate values of axis obliquity (
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