Hot hydrogen and oxygen atoms in the upper atmospheres of Venus and Mars: Distribution of hot hydrogen and oxygen calculated by a theoretical model

Andrew Nagy; Jhoon Kim; Tom Cravens

Hot hydrogen and oxygen atoms in the upper atmospheres of Venus and Mars: Distribution of hot hydrogen and oxygen calculated by a theoretical model

Andrew Nagy, Jhoon Kim, Tom Cravens

Department of Atmospheric Sciences

Research output: Contribution to journal › Article › peer-review

Abstract

Optical observations of hot atoms in the atmospheres of Venus and Mars are briefly reviewed. A summary of hot hydrogen and oxygen production and loss processes is given. Results of some recent model calculations as well as a number of new results of the hot hydrogen and oxygen populations are presented and their implication in terms of solar wind interaction processes is discussed.

Original language	English
Article number	1990AnGeo...8..251N
Pages (from-to)	251
Number of pages	256
Journal	Annales Geophysicae
Volume	8
Publication status	Published - 1990 Apr

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title = "Hot hydrogen and oxygen atoms in the upper atmospheres of Venus and Mars: Distribution of hot hydrogen and oxygen calculated by a theoretical model",

abstract = "Optical observations of hot atoms in the atmospheres of Venus and Mars are briefly reviewed. A summary of hot hydrogen and oxygen production and loss processes is given. Results of some recent model calculations as well as a number of new results of the hot hydrogen and oxygen populations are presented and their implication in terms of solar wind interaction processes is discussed.",

author = "Andrew Nagy and Jhoon Kim and Tom Cravens",

year = "1990",

month = apr,

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T2 - Distribution of hot hydrogen and oxygen calculated by a theoretical model

AU - Nagy, Andrew

AU - Kim, Jhoon

AU - Cravens, Tom

PY - 1990/4

Y1 - 1990/4

N2 - Optical observations of hot atoms in the atmospheres of Venus and Mars are briefly reviewed. A summary of hot hydrogen and oxygen production and loss processes is given. Results of some recent model calculations as well as a number of new results of the hot hydrogen and oxygen populations are presented and their implication in terms of solar wind interaction processes is discussed.

AB - Optical observations of hot atoms in the atmospheres of Venus and Mars are briefly reviewed. A summary of hot hydrogen and oxygen production and loss processes is given. Results of some recent model calculations as well as a number of new results of the hot hydrogen and oxygen populations are presented and their implication in terms of solar wind interaction processes is discussed.

UR - http://adsabs.harvard.edu/abs/1990AnGeo...8..251N

M3 - Article

VL - 8

SP - 251

JO - Annales Geophysicae

JF - Annales Geophysicae

SN - 0992-7689

M1 - 1990AnGeo...8..251N

ER -

Hot hydrogen and oxygen atoms in the upper atmospheres of Venus and Mars: Distribution of hot hydrogen and oxygen calculated by a theoretical model

Abstract

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