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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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| Main Authors: | , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
National Academy of Sciences
2014
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| Acceso en liña: | https://ncbi.nlm.nih.gov/pmc/articles/PMC3896211/ https://ncbi.nlm.nih.gov/pubmed/24379386 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.1315215111 |
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