Fast-rotating Earth-like planets should show larger equator-to-pole temperature contrasts when they spin faster or have thinner atmospheres, with bulk lapse rate peaking at baroclinic criticality.
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Scaling Relations for Terrestrial Exoplanet Atmospheres from Baroclinic Criticality
Fast-rotating Earth-like planets should show larger equator-to-pole temperature contrasts when they spin faster or have thinner atmospheres, with bulk lapse rate peaking at baroclinic criticality.