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Distant interplanetary wake of Venus: plasma observations from pioneer Venus

Journal Article · · J. Geophys. Res.; (United States)
In June 1979 the Pioneer Venus orbiter made its first series of passes through the distant solar wind wake of Venus at distances of 8--12 R/sub V/ behind the planet. During this period the plasma analyzer aboard the spacecraft detected disturbed magnetosheath plasma that intermittently disappeared and reappeared, suggesting a tattered, filamentary cavity trailing behind the planet. The magnetosheath dropouts almost always occurred inside the region of 'magnetotail' observed by Russell et al. Sporadic bursts of energetic ions (E/q> or approx. =4kV) are detected inside and, occasionally, outside the magnetotail; all such bursts are consistent with identification of the ion as O/sup +/ of planetary origin moving at the local magnetosheath flow speed. The morphology of the plasma dropouts and of the O/sup +/ bursts is analyzed in detail. The cavity appears to contract at times of high solar wind dynamic pressure. The intensity of the O/sup +/ component is highly variable, and appears not to be strongly correlated with solar wind dynamic pressure. The most intense bursts correspond to a flux < or approx. =10/sup 7/ ions cm/sup -2/ s/sup -1/. This maximum flux, if steady and filling a cylinder 1 R/sub V/ in radius would correspond to a mass loss rate of < or approx. =10/sup 25/ ions s/sup -1/; the intermittency and variability of the flux suggest that the true mean loss rate is very much lower. The kinetic temperature of the O/sup +/ component is estimated as 10/sup 5/--10/sup 6/ K in order of magnitude.
Research Organization:
Theoretical and Planetary Studies Branch, NASA Ames Research Center, Moffett Field, California 94035
OSTI ID:
6848526
Journal Information:
J. Geophys. Res.; (United States), Journal Name: J. Geophys. Res.; (United States) Vol. 87:A11; ISSN JGREA
Country of Publication:
United States
Language:
English