Role of ocean heat transport in climates of tidally locked exoplanets around M dwarf stars

The distinctive feature of tidally locked exoplanets is the very uneven heating by stellar radiation between the dayside and nightside. Previous work has focused on the role of atmospheric heat transport in preventing atmospheric collapse on the nightside for terrestrial exoplanets in the habitable...

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Vydané v:	Proceedings of the National Academy of Sciences - PNAS Ročník 111; číslo 2; s. 629
Hlavní autori:	Hu, Yongyun, Yang, Jun
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	United States 14.01.2014
Predmet:	Atmosphere Climate Computer Simulation Hot Temperature Models, Theoretical Oceans and Seas Planets Stars, Celestial planetary climate exoplanet habitability superEarth
ISSN:	1091-6490, 1091-6490
On-line prístup:	Zistit podrobnosti o prístupe
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