Venus atmosphere profile from a maximum entropy principle

Autores
Epele, Luis Nicolás; Fanchiotti, Huner; García Canal, Carlos Alberto; Pacheco, A. F.; Sañudo, J.
Año de publicación
2007
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The variational method with constraints recently developed by Verkley and Gerkema to describe maximum-entropy atmospheric profiles is generalized to ideal gases but with temperature-dependent specific heats. In so doing, an extended and non standard potential temperature is introduced that is well suited for tackling the problem under consideration. This new formalism is successfully applied to the atmosphere of Venus. Three well defined regions emerge in this atmosphere up to a height of 100 km from the surface: the lowest one up to about 35 km is adiabatic, a transition layer located at the height of the cloud deck and finally a third region which is practically isothermal.
Facultad de Ciencias Exactas
Materia
Ciencias Exactas
Física
adiabatic process
entropy
planetary atmosphere
temperature profile
Venus
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by/3.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/35585
Acceder
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oai_identifier_str oai:sedici.unlp.edu.ar:10915/35585
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Venus atmosphere profile from a maximum entropy principleEpele, Luis NicolásFanchiotti, HunerGarcía Canal, Carlos AlbertoPacheco, A. F.Sañudo, J.Ciencias ExactasFísicaadiabatic processentropyplanetary atmospheretemperature profileVenusThe variational method with constraints recently developed by Verkley and Gerkema to describe maximum-entropy atmospheric profiles is generalized to ideal gases but with temperature-dependent specific heats. In so doing, an extended and non standard potential temperature is introduced that is well suited for tackling the problem under consideration. This new formalism is successfully applied to the atmosphere of Venus. Three well defined regions emerge in this atmosphere up to a height of 100 km from the surface: the lowest one up to about 35 km is adiabatic, a transition layer located at the height of the cloud deck and finally a third region which is practically isothermal.Facultad de Ciencias Exactas2007-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf641-647http://sedici.unlp.edu.ar/handle/10915/35585enginfo:eu-repo/semantics/altIdentifier/url/http://www.nonlin-processes-geophys.net/14/641/2007/npg-14-641-2007.pdfinfo:eu-repo/semantics/altIdentifier/issn/1023-5809info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/3.0/Creative Commons Attribution 3.0 Unported (CC BY 3.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-03T10:29:55Zoai:sedici.unlp.edu.ar:10915/35585Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-03 10:29:55.673SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Venus atmosphere profile from a maximum entropy principle
title Venus atmosphere profile from a maximum entropy principle
spellingShingle Venus atmosphere profile from a maximum entropy principle
Epele, Luis Nicolás
Ciencias Exactas
Física
adiabatic process
entropy
planetary atmosphere
temperature profile
Venus
title_short Venus atmosphere profile from a maximum entropy principle
title_full Venus atmosphere profile from a maximum entropy principle
title_fullStr Venus atmosphere profile from a maximum entropy principle
title_full_unstemmed Venus atmosphere profile from a maximum entropy principle
title_sort Venus atmosphere profile from a maximum entropy principle
dc.creator.none.fl_str_mv Epele, Luis Nicolás
Fanchiotti, Huner
García Canal, Carlos Alberto
Pacheco, A. F.
Sañudo, J.
author Epele, Luis Nicolás
author_facet Epele, Luis Nicolás
Fanchiotti, Huner
García Canal, Carlos Alberto
Pacheco, A. F.
Sañudo, J.
author_role author
author2 Fanchiotti, Huner
García Canal, Carlos Alberto
Pacheco, A. F.
Sañudo, J.
author2_role author
author
author
author
dc.subject.none.fl_str_mv Ciencias Exactas
Física
adiabatic process
entropy
planetary atmosphere
temperature profile
Venus
topic Ciencias Exactas
Física
adiabatic process
entropy
planetary atmosphere
temperature profile
Venus
dc.description.none.fl_txt_mv The variational method with constraints recently developed by Verkley and Gerkema to describe maximum-entropy atmospheric profiles is generalized to ideal gases but with temperature-dependent specific heats. In so doing, an extended and non standard potential temperature is introduced that is well suited for tackling the problem under consideration. This new formalism is successfully applied to the atmosphere of Venus. Three well defined regions emerge in this atmosphere up to a height of 100 km from the surface: the lowest one up to about 35 km is adiabatic, a transition layer located at the height of the cloud deck and finally a third region which is practically isothermal.
Facultad de Ciencias Exactas
description The variational method with constraints recently developed by Verkley and Gerkema to describe maximum-entropy atmospheric profiles is generalized to ideal gases but with temperature-dependent specific heats. In so doing, an extended and non standard potential temperature is introduced that is well suited for tackling the problem under consideration. This new formalism is successfully applied to the atmosphere of Venus. Three well defined regions emerge in this atmosphere up to a height of 100 km from the surface: the lowest one up to about 35 km is adiabatic, a transition layer located at the height of the cloud deck and finally a third region which is practically isothermal.
publishDate 2007
dc.date.none.fl_str_mv 2007-10
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
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://sedici.unlp.edu.ar/handle/10915/35585
url http://sedici.unlp.edu.ar/handle/10915/35585
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://www.nonlin-processes-geophys.net/14/641/2007/npg-14-641-2007.pdf
info:eu-repo/semantics/altIdentifier/issn/1023-5809
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/3.0/
Creative Commons Attribution 3.0 Unported (CC BY 3.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by/3.0/
Creative Commons Attribution 3.0 Unported (CC BY 3.0)
dc.format.none.fl_str_mv application/pdf
641-647
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 13.13397

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