Atmospheric dynamics of temperate sub-neptunes. I. Dry dynamics

Sub-Neptunes (planets with radii between 2 and 4 R⊕) are abundant around M-dwarf stars, yet the atmospheric dynamics of these planets is relatively unexplored. In this paper, we aim to provide a basic underpinning of the dry dynamics of general low-mean-molecular-weight, temperate sub-Neptune atmosp...

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Hlavní autoři: Innes, H, Pierrehumbert, RT
Médium: Journal article
Jazyk:English
Vydáno: IOP Publishing 2022