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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| Formato: | Capítulo de libro |
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Pleiades Publishing
2018
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
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| LEADER | 08018caa a22008057a 4500 | ||
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| 001 | PAPER-25211 | ||
| 003 | AR-BaUEN | ||
| 005 | 20250725124914.0 | ||
| 008 | 190410s2018 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-85049307192 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Cirilo-Lombardo, D.J. | |
| 245 | 1 | 6 | |a About Superrotation in Venus |
| 260 | |b Pleiades Publishing |c 2018 | ||
| 270 | 1 | 0 | |m Cirilo-Lombardo, D.J.; Instituto de Física del Plasma (INFIP), CONICET–Universidad de Buenos AiresArgentina; email: diego777jcl@gmail.com |
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| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a 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. |l eng | |
| 536 | |a Detalles de la financiación: Consejo Nacional de Investigaciones Científicas y Técnicas | ||
| 536 | |a Detalles de la financiación: VII. ACKNOWLEDGMENTS We gratefully acknowledge to the Departamento de Física (FCEyN, UBA) and Instituto de Física del Plasma (CONICET-UBA), FM and DC are also grateful to the Consejo Nacional de Investigaciones Científicas y Técnicas, CV is also grateful to the Insti-tuto de Ciencias (UNGS) and DC is also grateful to the Bogoliubov Laboratory of Theoretical Physics for their institutional support. | ||
| 593 | |a Instituto de Física del Plasma (INFIP), CONICET–Universidad de Buenos Aires, Buenos Aires, Argentina | ||
| 593 | |a Facultad de Ciencias Exactas y Naturales, Departamento de Física, Universidad de Buenos Aires, Buenos Aires, Argentina | ||
| 593 | |a Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Dubna, 141980, Russian Federation | ||
| 593 | |a Instituto de Ciencias, Universidad Nacional de General Sarmiento, Los Polvorines, Argentina | ||
| 700 | 1 | |a Mayochi, M. | |
| 700 | 1 | |a Minotti, Fernando Oscar | |
| 700 | 1 | |a Vigh, Carlos Donato | |
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