Experimental data on the plasma envelopes of Mars, Venus, and Halley's and Giacobini-Zinner's comets: comparison of loading effects.

Details Experimental data on the plasma envelopes of Mars, Venus, and Halley's and Giacobini-Zinner's comets: comparison of loading effects. Experimental data on the plasma envelopes of Mars, Venus, and Halley's and Giacobini-Zinner's comets: comparison of loading effects.

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990cosre..27..638v&link_type=abstract

Cosmic Res., Vol. 27, No. 5, p. 638 - 649

Mathematics

Logic

Cometary Plasma

Scientific paper

Results of research on the interaction of the solar wind with gaseous obstacles, which are the atmospheres of planets and comets, are described from a unique point of view. It is shown that with such interaction there results a specific plasma formation - a mantle, the boundary between which and the solar wind is distinctly marked. Possible physical mechanisms leading to the formation of an abrupt boundary between a mantle and the external flux are discussed. The mantle formed on the day side is topologically connected to the plasma tail.

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