Structure of the Venusian tail

Details Structure of the Venusian tail Structure of the Venusian tail

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980kosis..18..651v&link_type=abstract

Kosmicheskie Issledovaniia, vol. 18, July-Aug. 1980, p. 651-655. In Russian.

Mathematics

Logic

Planetary Magnetic Fields, Planetary Magnetospheres, Planetary Structure, Venus Atmosphere, Computerized Simulation, Planetary Ionospheres, Solar Wind, Venera 10 Satellite, Venera 9 Satellite

Scientific paper

The structure of the field in the tail of the induced Venusian magnetosphere has been studied by Dubinin et al. (1978) on the basis of laboratory simulation of solar wind/ionosphere interaction, showing that the nature of the magnetic fields in the tail of the natural and induced Venusian magnetospheres is topologically indistinguishable. In the present paper, Venera 9 and 10 data are used to show that the tails of induced magnetospheres possess apparently a helical structure, as distinct from the magnetospheric tails of planets possessing a substantial proper magnetic field.

Affiliated with

Also associated with

No associations

Rating

Structure of the Venusian tail does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Structure of the Venusian tail, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure of the Venusian tail will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-804433