Rotation of the MHD-wave polarization vector in a flare stream

Details Rotation of the MHD-wave polarization vector in a flare stream Rotation of the MHD-wave polarization vector in a flare stream

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..306p&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, Mar.-Apr. 1989, p. 306-309. In Russian.

Mathematics

Magnetic Variations, Magnetohydrodynamic Waves, Polarization Characteristics, Solar Flares, Space Plasmas, Plasma Interactions, Shock Wave Interaction, Solar Wind, Vectors (Mathematics)

Scientific paper

The paper examines long-period fluctuations of the magnetic observed in a compressed solar-wind region in flare streams and the accompanying rotation of the polarization vector. The observed phenomenon is found to be the result of the superposition of Alfven and slow magnetoacoustic waves, arising due to the transformation of linearly polarized Alfven waves interacting with a fast shock wave.

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