Discussion of plasma instability between solar wind and type-I comet tail

Details Discussion of plasma instability between solar wind and type-I comet tail Discussion of plasma instability between solar wind and type-I comet tail

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991chjss..11..187g&link_type=abstract

Chinese Journal of Space Science (ISSN 0254-6124), vol. 11, no. 3, p. 187-192.

Physics

Comet Tails, Force-Free Magnetic Fields, Giacobini-Zinner Comet, Magnetohydrodynamic Stability, Solar Wind, Comets, International Sun Earth Explorer 3

Scientific paper

In this paper, the 'two-stream' plasma instability between solar wind and comet tail in a force-free field case is discussed. The data come from the exploration for the Comet Giacobini-Zinner by the International Cometary Explorer Spacecraft. The conclusion shows that the two stream instability exists in the inner part of a comet if a reasonable plasma distribution is considered.

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