The circulation pattern and day-night heat transport in the atmosphere of a synchronously rotating aquaplanet: Dependence on planetary rotation rate
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- 作者：S. Noda ; a ; 1 ; noda@gfd-dennou.org" class="auth_mail" title="E-mail the corresponding author ; M. Ishiwatarib ; c ; K. Nakajimad ; Y.O. Takahashia ; c ; S. Takehiroe ; M. Onishia ; 2 ; G.L. Hashimotof ; K. Kuramotob ; c ; Y.-Y. Hayashia ; c
- 关键词：Astrobiology ; Atmospheres ; dynamics ; Atmospheres structure ; Extra-solar ; planets ; Meteorology
- 刊名：Icarus
- 出版年：2017
- 出版时间：15 January 2017
- 年：2017
- 卷：282
- 期：Complete
- 页码：1-18
- 全文大小：9702 K
文摘
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Atmospheric circulation of a synchronously rotating aquaplanet is examined by a GCM.
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Its dependence on the planetary rotation rate is focused.
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Four types of circulation structures are identified.
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Net day-night energy transport is almost insensitive to the circulation structure.
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The insensitivity originates from the radiation limit of the moist atmosphere.