About Superrotation in Venus

In this work we study in a general view slow rotating planets as Venus or Titan which present superrotating winds in their atmospheres. We are interested in understanding what mechanisms are candidates to be sources of net angular momentum to generate this kind of dynamics. In particular, in the cas...

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Detalles Bibliográficos
Publicado: 2018
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380946_v52_n3_p223_CiriloLombardo
http://hdl.handle.net/20.500.12110/paper_00380946_v52_n3_p223_CiriloLombardo
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_00380946_v52_n3_p223_CiriloLombardo
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spelling paper:paper_00380946_v52_n3_p223_CiriloLombardo2023-06-08T15:02:58Z About Superrotation in Venus In this work we study in a general view slow rotating planets as Venus or Titan which present superrotating winds in their atmospheres. We are interested in understanding what mechanisms are candidates to be sources of net angular momentum to generate this kind of dynamics. In particular, in the case of Venus, in its atmosphere around an altitude of 100 km relative to the surface, there exists winds that perform a full rotation around the planet in four terrestrial days, whereas the venusian day is equivalent to 243 terrestrial ones. This phenomenon called superrotation is known since many decades. However, its origin and behaviour is not completely understood. In this article we analise and ponderate the importance of different effects to generate this dynamics. © 2018, Pleiades Publishing, Inc. 2018 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380946_v52_n3_p223_CiriloLombardo http://hdl.handle.net/20.500.12110/paper_00380946_v52_n3_p223_CiriloLombardo
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description In this work we study in a general view slow rotating planets as Venus or Titan which present superrotating winds in their atmospheres. We are interested in understanding what mechanisms are candidates to be sources of net angular momentum to generate this kind of dynamics. In particular, in the case of Venus, in its atmosphere around an altitude of 100 km relative to the surface, there exists winds that perform a full rotation around the planet in four terrestrial days, whereas the venusian day is equivalent to 243 terrestrial ones. This phenomenon called superrotation is known since many decades. However, its origin and behaviour is not completely understood. In this article we analise and ponderate the importance of different effects to generate this dynamics. © 2018, Pleiades Publishing, Inc.
title About Superrotation in Venus
spellingShingle About Superrotation in Venus
title_short About Superrotation in Venus
title_full About Superrotation in Venus
title_fullStr About Superrotation in Venus
title_full_unstemmed About Superrotation in Venus
title_sort about superrotation in venus
publishDate 2018
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380946_v52_n3_p223_CiriloLombardo
http://hdl.handle.net/20.500.12110/paper_00380946_v52_n3_p223_CiriloLombardo
_version_ 1768543125550137344

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