Interaction of cosmic rays with anisotropic magnetic-field turbulence

Details Interaction of cosmic rays with anisotropic magnetic-field turbulence Interaction of cosmic rays with anisotropic magnetic-field turbulence

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2120d&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

Physics

Cosmic Rays, Nonuniform Magnetic Fields, Plasma-Electromagnetic Interaction, Plasma-Particle Interactions, Solar Wind, Cosmic Plasma, Electric Field Strength, Particle Acceleration, Solar Activity Effects

Scientific paper

The propagation of high-energy charged particles in turbulent, statistically anisotropic plasma of the solar wind is analyzed on the basis of the collisionless kinetic equation. It is shown that an effective particle-acceleration mechanism connected with the presence of a mean electric field of fluctuations directed along the regular field arises in a magnetized cosmic plasma with reflectively invariant turbulence of the magnetic field.

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