Unipolar induction effects in the Venusian magnetic tail

Details Unipolar induction effects in the Venusian magnetic tail Unipolar induction effects in the Venusian magnetic tail

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979kosis..17...93e&link_type=abstract

Kosmicheskie Issledovaniia, vol. 17, Jan.-Feb. 1979, p. 93-105. In Russian.

Computer Science

5

Magnetic Induction, Planetary Magnetic Fields, Planetary Magnetospheres, Venus Atmosphere, Geomagnetic Tail, Interplanetary Magnetic Fields, Magnetic Field Configurations, Magnetic Signatures, Satellite Observation, Solar Wind, Venera Satellites

Scientific paper

Venera 4, 9, and 10 measurements of the magnetic field in the Venusian tail are analyzed. A correlation is detected between the field structure in the tail and the orientation of the transverse component of the interplanetary magnetic field. It is shown that the Venus data can be interpreted within the framework of a model of the unipolar induction field which forms in the daytime ionosphere and is extended to the dark side by interaction with the solar wind.

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