【摘 要】
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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 transpo
【机 构】
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Laboratory for Climate and Atmosphere-Ocean Studies, Dept.of Atmospheric and Oceanic Sciences, Schoo
【出 处】
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中国科学院大气物理研究所大气科学和地球流体力学数值模拟国家重点实验室2013年度LASG年会
论文部分内容阅读
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 zone (HZ) around M-dwarfs.
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