3D convection-resolving model of temperate, tidally locked exoplanets

3D convection-resolving model of temperate, tidally locked exoplanets

A large fraction of known terrestrial-size exoplanets located in the habitable zone of M-dwarfs are expected to be tidally locked. Numerous efforts have been conducted to study the climate of such planets, using in particular 3D global climate models (GCMs). One of the biggest challenges in simulati...

書誌詳細
主要な著者:	Lefevre, M, Turbet, M, Pierrehumbert, R
フォーマット:	Journal article
言語:	English
出版事項:	American Astronomical Society 2021

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