Rotation of the polarization vector of MHD waves in a flare stream.

Details Rotation of the polarization vector of MHD waves in a flare stream. Rotation of the polarization vector of MHD waves in a flare stream.

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..268p&link_type=abstract

Geomagn. Aeron., Vol. 29, No. 2, p. 268 - 270

Computer Science

Interplanetary Magnetic Field: Magnetohydrodynamics, Interplanetary Magnetic Field: Alfven Waves, Interplanetary Magnetic Field: Solar Wind

Scientific paper

Long-period oscillations of the magnetic field observed in a region of compressed solar wind in flare streams and accompanied by rotation of the polarization vector are discussed. The phenomenon under discussion has been explained as a result of the superposition of Alfvén and slow magnetosonic waves arising as a result of transformation of linearly polarized Alfvén waves interacting with a fast shock wave.

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