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Venus atmosphere profile from a maximum entropy principle

Epele, Luis Nicolás et al · SEDICI UNLP · 2007

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Author / responsible party
Epele, Luis Nicolás et al
Publisher
SEDICI UNLP
Year
2007
Language
English

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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

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APA 7

Epele, L. N. E. A. (2007). Venus atmosphere profile from a maximum entropy principle. http://sedici.unlp.edu.ar/handle/10915/35585

MLA

Epele, Luis Nicolás et al. "Venus atmosphere profile from a maximum entropy principle." 2007. http://sedici.unlp.edu.ar/handle/10915/35585.

Chicago

Epele, Luis Nicolás et al. 2007. "Venus atmosphere profile from a maximum entropy principle.". http://sedici.unlp.edu.ar/handle/10915/35585.

Harvard

Epele, L. N. E. A. 2007, Venus atmosphere profile from a maximum entropy principle, SEDICI UNLP, available at: http://sedici.unlp.edu.ar/handle/10915/35585 [Accessed 5 Aug. 2026].

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Title
Venus atmosphere profile from a maximum entropy principle
Author / contributors
Epele, Luis Nicolás et al
Publisher
SEDICI UNLP
Publication year
2007
Language
English

Subjects

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Ciencias Exactas; Física; adiabatic process; entropy; planetary atmosphere; temperature profile; Venus
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