About Superrotation in Venus

Autores
Cirilo, Diego Julio; Mayochi, Mariano Gustavo; Minotti, Fernando Oscar; Vigh, Carlos Donato
Año de publicación
2018
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
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.
Fil: Cirilo, Diego Julio. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física del Plasma. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física del Plasma; Argentina
Fil: Mayochi, Mariano Gustavo. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina
Fil: Minotti, Fernando Oscar. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física del Plasma. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física del Plasma; Argentina
Fil: Vigh, Carlos Donato. Universidad Nacional de General Sarmiento. Instituto de Ciencias; Argentina
Materia
SUPERROTATION
PLANETARY PHYSICS
PHYSICS OF FLUIDS AND ATMOSPHERES
GRAVITY WAVES
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/86850
Acceder
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network_name_str CONICET Digital (CONICET)
spelling About Superrotation in VenusCirilo, Diego JulioMayochi, Mariano GustavoMinotti, Fernando OscarVigh, Carlos DonatoSUPERROTATIONPLANETARY PHYSICSPHYSICS OF FLUIDS AND ATMOSPHERESGRAVITY WAVEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1https://purl.org/becyt/ford/1.1https://purl.org/becyt/ford/1In 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.Fil: Cirilo, Diego Julio. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física del Plasma. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física del Plasma; ArgentinaFil: Mayochi, Mariano Gustavo. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; ArgentinaFil: Minotti, Fernando Oscar. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física del Plasma. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física del Plasma; ArgentinaFil: Vigh, Carlos Donato. Universidad Nacional de General Sarmiento. Instituto de Ciencias; ArgentinaSP MAIK Nauka/Interperiodica2018-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/86850Cirilo, Diego Julio; Mayochi, Mariano Gustavo; Minotti, Fernando Oscar; Vigh, Carlos Donato; About Superrotation in Venus; SP MAIK Nauka/Interperiodica; Solar System Research; 52; 3; 6-2018; 223-2330038-0946CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1134/S003809461803005Xinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T10:10:08Zoai:ri.conicet.gov.ar:11336/86850instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-03 10:10:09.165CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv About Superrotation in Venus
title About Superrotation in Venus
spellingShingle About Superrotation in Venus
Cirilo, Diego Julio
SUPERROTATION
PLANETARY PHYSICS
PHYSICS OF FLUIDS AND ATMOSPHERES
GRAVITY WAVES
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
dc.creator.none.fl_str_mv Cirilo, Diego Julio
Mayochi, Mariano Gustavo
Minotti, Fernando Oscar
Vigh, Carlos Donato
author Cirilo, Diego Julio
author_facet Cirilo, Diego Julio
Mayochi, Mariano Gustavo
Minotti, Fernando Oscar
Vigh, Carlos Donato
author_role author
author2 Mayochi, Mariano Gustavo
Minotti, Fernando Oscar
Vigh, Carlos Donato
author2_role author
author
author
dc.subject.none.fl_str_mv SUPERROTATION
PLANETARY PHYSICS
PHYSICS OF FLUIDS AND ATMOSPHERES
GRAVITY WAVES
topic SUPERROTATION
PLANETARY PHYSICS
PHYSICS OF FLUIDS AND ATMOSPHERES
GRAVITY WAVES
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
https://purl.org/becyt/ford/1.1
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv 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.
Fil: Cirilo, Diego Julio. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física del Plasma. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física del Plasma; Argentina
Fil: Mayochi, Mariano Gustavo. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina
Fil: Minotti, Fernando Oscar. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física del Plasma. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física del Plasma; Argentina
Fil: Vigh, Carlos Donato. Universidad Nacional de General Sarmiento. Instituto de Ciencias; Argentina
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.
publishDate 2018
dc.date.none.fl_str_mv 2018-06
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/86850
Cirilo, Diego Julio; Mayochi, Mariano Gustavo; Minotti, Fernando Oscar; Vigh, Carlos Donato; About Superrotation in Venus; SP MAIK Nauka/Interperiodica; Solar System Research; 52; 3; 6-2018; 223-233
0038-0946
CONICET Digital
CONICET
url http://hdl.handle.net/11336/86850
identifier_str_mv Cirilo, Diego Julio; Mayochi, Mariano Gustavo; Minotti, Fernando Oscar; Vigh, Carlos Donato; About Superrotation in Venus; SP MAIK Nauka/Interperiodica; Solar System Research; 52; 3; 6-2018; 223-233
0038-0946
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1134/S003809461803005X
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv SP MAIK Nauka/Interperiodica
publisher.none.fl_str_mv SP MAIK Nauka/Interperiodica
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.13397

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