Roles of Atmospheric Waves in Venus' Superrotation : Results of a Venus-Like GCM for a 3D Thermal Forcing
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- YAMAMOTO Masaru
- Faculty of Education, Wakayama University
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- TAKAHASHI Masaaki
- Center for Climate System Research, University of Tokyo
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説明
Superrotation of more than 100 m s−1 is formed at 60 km in a Venus-like general circulation model (Venus-like GCM) driven by a three-dimensional (3D) heating with a 117-day period. Meridional circulation efficiently pumps up angular momentum from the surface to the cloud-top level (65-70km) as expected from the Gierasch mechanism. Thermally-forced or enhanced waves with zonal wavenumbers of 1 and 2 produce equatorward eddy momentum fluxes, being possible candidates for the equatorward momentum flux caused by large horizontal diffusion in the Gierasch mechanism.
収録刊行物
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- Theoretical and Applied Mechanics Japan
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Theoretical and Applied Mechanics Japan 51 (0), 225-230, 2002
日本学術会議 「機械工学委員会・土木工学・建築学委員会合同IUTAM分科会」
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詳細情報 詳細情報について
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- CRID
- 1390001205210267008
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- NII論文ID
- 130004463510
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- ISSN
- 13494244
- 13480693
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- 本文言語コード
- en
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- データソース種別
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- JaLC
- CiNii Articles
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- 抄録ライセンスフラグ
- 使用不可