Instabilities of MHD waves in the solar wind

Details Instabilities of MHD waves in the solar wind Instabilities of MHD waves in the solar wind

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ge%26ae..26..373m&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 26, May-June 1986, p. 373-377. In Russian.

Physics

Halos, Magnetohydrodynamic Stability, Plasma-Particle Interactions, Solar Protons, Solar Wind, Earth Orbits, Vertical Distribution

Scientific paper

The paper investigates the effect of the solar-wind proton halo on the generation of MHD waves propagating at an angle to the magnetic field. Increments and development conditions for the MHD-wave instabilities are determined. The instabilities are most likely to arise in the heliospheric region with R = 5-20 solar radii. The occurrence of the instability near earth orbit is found to be possible.

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