The puzzling Venusian polar atmospheric structure reproduced by a general circulation model

Unlike some planets, the Venusian polar vortex is warmer than the mid-latitudes at cloud-top level, but the mechanism behind this is unknown. Here, the authors use a general circulation model and suggest the cold collar and warm polar regions are due to residual mean meridional circulation intensifi...

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Autores principales:	Hiroki Ando, Norihiko Sugimoto, Masahiro Takagi, Hiroki Kashimura, Takeshi Imamura, Yoshihisa Matsuda
Formato:	article
Lenguaje:	EN
Publicado:	Nature Portfolio 2016
Materias:	Science Q
Acceso en línea:	https://doaj.org/article/37ad107018ae4859a78220c20d4c54ef
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spelling	oai:doaj.org-article:37ad107018ae4859a78220c20d4c54ef2021-12-02T17:32:21ZThe puzzling Venusian polar atmospheric structure reproduced by a general circulation model10.1038/ncomms103982041-1723https://doaj.org/article/37ad107018ae4859a78220c20d4c54ef2016-02-01T00:00:00Zhttps://doi.org/10.1038/ncomms10398https://doaj.org/toc/2041-1723Unlike some planets, the Venusian polar vortex is warmer than the mid-latitudes at cloud-top level, but the mechanism behind this is unknown. Here, the authors use a general circulation model and suggest the cold collar and warm polar regions are due to residual mean meridional circulation intensified by thermal tides.Hiroki AndoNorihiko SugimotoMasahiro TakagiHiroki KashimuraTakeshi ImamuraYoshihisa MatsudaNature PortfolioarticleScienceQENNature Communications, Vol 7, Iss 1, Pp 1-8 (2016)
institution	DOAJ
collection	DOAJ
language	EN
topic	Science Q
spellingShingle	Science Q Hiroki Ando Norihiko Sugimoto Masahiro Takagi Hiroki Kashimura Takeshi Imamura Yoshihisa Matsuda The puzzling Venusian polar atmospheric structure reproduced by a general circulation model
description	Unlike some planets, the Venusian polar vortex is warmer than the mid-latitudes at cloud-top level, but the mechanism behind this is unknown. Here, the authors use a general circulation model and suggest the cold collar and warm polar regions are due to residual mean meridional circulation intensified by thermal tides.
format	article
author	Hiroki Ando Norihiko Sugimoto Masahiro Takagi Hiroki Kashimura Takeshi Imamura Yoshihisa Matsuda
author_facet	Hiroki Ando Norihiko Sugimoto Masahiro Takagi Hiroki Kashimura Takeshi Imamura Yoshihisa Matsuda
author_sort	Hiroki Ando
title	The puzzling Venusian polar atmospheric structure reproduced by a general circulation model
title_short	The puzzling Venusian polar atmospheric structure reproduced by a general circulation model
title_full	The puzzling Venusian polar atmospheric structure reproduced by a general circulation model
title_fullStr	The puzzling Venusian polar atmospheric structure reproduced by a general circulation model
title_full_unstemmed	The puzzling Venusian polar atmospheric structure reproduced by a general circulation model
title_sort	puzzling venusian polar atmospheric structure reproduced by a general circulation model
publisher	Nature Portfolio
publishDate	2016
url	https://doaj.org/article/37ad107018ae4859a78220c20d4c54ef
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The puzzling Venusian polar atmospheric structure reproduced by a general circulation model

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