Cosmic rays and magneto-acoustic instability of the solar-wind stream near the heliosphere shock wave.

Details Cosmic rays and magneto-acoustic instability of the solar-wind stream near the heliosphere shock wave. Cosmic rays and magneto-acoustic instability of the solar-wind stream near the heliosphere shock wave.

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30...24c&link_type=abstract

Geomagn. Aeron., Vol. 30, No. 1, p. 24 - 27

Physics

Heliosphere: Cosmic Rays, Heliosphere: Shock Waves, Heliosphere: Solar Wind

Scientific paper

The instability of fast magneto-acoustic waves propagating near the equatorial plane ahead of a heliospheric shock front where the solar wind is retarded by the cosmic-ray pressure gradient is investigated. The unstable waves with the highest increment are propagated normal to the equatorial plane. The direction of the propagation of these waves depends on the polarity of the interplanetary magnetic field.

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