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Absorption of whistler mode waves in the ionosphere of VenusIt is shown that whistler mode waves from the ionosheath of Venus are absorbed by Landau damping at the dayside ionosphere boundary. This process heats the ionospheric electrons and it may provide an important energy input into the dayside ionosphere. Cyclotron damping of the waves does not occur in the same region. However, Landau damping of ionosheath waves is apparently not an important energy source in the nightside ionosphere. Impulsive events in the nightside ionosphere seem to fall into two classes: (1) lightning signals (near periapsis) and (2) noise, which may be caused by gradient or current instabilities.
Document ID
19790056821
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Taylor, W. W. L.
(TRW Defense and Space Systems Group Redondo Beach, CA, United States)
Scarf, F. L.
(TRW Defense and Space Systems Group Redondo Beach, Calif., United States)
Russell, C. T.
(California, University Los Angeles, Calif., United States)
Brace, L. H.
(NASA Goddard Space Flight Center Greenbelt, Md., United States)
Date Acquired
August 9, 2013
Publication Date
July 6, 1979
Publication Information
Publication: Science
Volume: 205
Subject Category
Lunar And Planetary Exploration
Accession Number
79A40834
Funding Number(s)
CONTRACT_GRANT: NAS2-8088
CONTRACT_GRANT: NAS2-9842
CONTRACT_GRANT: NAS2-9491
Distribution Limits
Public
Copyright
Other

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