The asymmetry of the inner stream in the flow circulation behind Venus

Details The asymmetry of the inner stream in the flow circulation behind Venus The asymmetry of the inner stream in the flow circulation behind Venus

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980kosis..18..809v&link_type=abstract

Kosmicheskie Issledovaniia, vol. 18, Sept.-Oct. 1980, p. 809-812. In Russian.

Physics

1

Cosmic Plasma, Interplanetary Magnetic Fields, Solar Wind, Venus Atmosphere, Asymmetry, Space Exploration, Venera 10 Satellite, Venera 9 Satellite

Scientific paper

Venera-9 and Venera-10 data on the flow circulation of the solar wind behind Venus are examined. The structure of the boundary between inner and outer plasma streams observed in the Venera plasma measurements is investigated. Results reveal an asymmetry of the plasma circulation behind Venus; it is suggested that this asymmetry is associated with the orientation of the interplanetary magnetic field.

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