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Simple models of the thermal structure of the Venusian ionosphereAnalytical and numerical models of plasma temperatures in the Venusian ionosphere are proposed. The magnitudes of plasma thermal parameters are calculated using thermal-structure data obtained by the Pioneer Venus Orbiter. The simple models are found to be in good agreement with the more detailed models of thermal balance. Daytime and nighttime temperature data along with corresponding temperature profiles are provided.
Document ID
19810041858
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Whitten, R. C.
(NASA Ames Research Center Space Sciences Div., Moffett Field, Calif., United States)
Knudsen, W. C.
(Lockheed Research Laboratories Palo Alto, Calif., United States)
Date Acquired
August 11, 2013
Publication Date
October 1, 1980
Publication Information
Publication: Icarus
Volume: 44
Subject Category
Lunar And Planetary Exploration
Accession Number
81A26262
Funding Number(s)
CONTRACT_GRANT: NAS2-9481
Distribution Limits
Public
Copyright
Other

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