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...
Autors principals: | Lefevre, M, Turbet, M, Pierrehumbert, R |
---|---|
Format: | Journal article |
Idioma: | English |
Publicat: |
American Astronomical Society
2021
|
Ítems similars
-
The phase-curve signature of condensible water-rich atmospheres on slowly rotating tidally locked exoplanets
per: Ding, F, et al.
Publicat: (2020) -
Atmospheric circulation of tide-locked exoplanets
per: Pierrehumbert, R, et al.
Publicat: (2018) -
The atmospheric circulation of tidally locked terrestrial exoplanets
per: Hammond, M
Publicat: (2019) -
A Laboratory Model of the Large-Scale Atmospheric Circulation of Tidally Locked Exoplanets
per: Bálint Vass, et al.
Publicat: (2024-08-01) -
How Landmass Distribution Influences the Atmospheric Dynamics of Tidally Locked Terrestrial Exoplanets
per: F. Sainsbury-Martinez, et al.
Publicat: (2024-01-01)