Instability of interpenetrating plasma streams in the solar wind

Details Instability of interpenetrating plasma streams in the solar wind Instability of interpenetrating plasma streams in the solar wind

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27..358v&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, May-June 1987, p. 358-361. In Russian.

Physics

Ion Motion, Plasma Jets, Solar Wind, Space Plasmas, Linear Systems, Magnetohydrodynamic Stability, Plasma Oscillations

Scientific paper

The linear instability increment is obtained for a plasma system formed by three interpenetrating ion streams with kinetic reversal along the magnetic field in the solar wind. It is shown that the value of the increment depends on the angle between the directions of reversal and oscillation propagation. The increment reaches its greatest value in the center of the interpenetrating stream system.

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