The rotational and divergent components of atmospheric circulation on tidally locked planets
Tidally locked exoplanets likely host global atmospheric circulations with a superrotating equatorial jet, planetary-scale stationary waves, and thermally driven overturning circulation. In this work, we show that each of these features can be separated from the total circulation by using a Helmholt...
Auteurs principaux: | Hammond, M, Lewis, NT |
---|---|
Format: | Journal article |
Langue: | English |
Publié: |
National Academy of Sciences
2021
|
Documents similaires
-
Data for 'Hammond and Lewis: The rotational and divergent components of atmospheric circulation on tidally locked planets, Proc. Nat. Acad. Sci., 2021'
par: Hammond, M, et autres
Publié: (2021) -
Wave-mean flow interactions in the atmospheric circulation of tidally locked planets
par: Hammond, M, et autres
Publié: (2018) -
The atmospheric circulation of tidally locked terrestrial exoplanets
par: Hammond, M
Publié: (2019) -
Atmospheric circulation on slowly rotating planets in the Solar System, and beyond
par: Lewis, NT
Publié: (2022) -
The equatorial jet speed on tidally locked planets. I. Terrestrial planets
par: Hammond, M, et autres
Publié: (2020)