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Thermal structure and major ion composition of the Venus ionosphere - First RPA results from Venus orbiterPioneer Venus in situ measurements of thermal plasma quantities were obtained by a retarding potential analyzer. Evidence for significant solar wind heating of the ionosphere and indications that the ionosphere is close to diffusive equilibrium are reported. Information on ionopause height, the ionospheric particle pressures at the ionopause, and the measured ratio of ionospheric scale height to ionopause ratio is presented.
Document ID
19790040145
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Knudsen, W. C.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Miller, K. L.
(Lockheed Research Laboratories Palo Alto, Calif., United States)
Spenner, K.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Novak, V.
(Fraunhofer-Gesellschaft zur Foerderung der angewandten Forschung Institut fuer physikalische Weltraumforschung, Freiburg im Breisgau, Germany)
Whitten, R. C.
(NASA Ames Research Center Moffett Field, Calif., United States)
Spreiter, J. R.
(Stanford University Stanford, Calif., United States)
Date Acquired
August 9, 2013
Publication Date
February 23, 1979
Publication Information
Publication: Science
Volume: 203
Subject Category
Lunar And Planetary Exploration
Accession Number
79A24158
Funding Number(s)
CONTRACT_GRANT: NAS2-9481
CONTRACT_GRANT: BMFT-01-DO-238/RV14-B-28/73
Distribution Limits
Public
Copyright
Other

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