Theory of particle acceleration by shock fronts with large-scale motions of plasma in a turbulent medium

Details Theory of particle acceleration by shock fronts with large-scale motions of plasma in a turbulent medium Theory of particle acceleration by shock fronts with large-scale motions of plasma in a turbulent medium

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979izyer..43.2552b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yerevan, Armenian SSR, June 1979.) Akademiia Nauk SSSR, Izvestiia, Seriia Fi

Physics

Magnetohydrodynamic Turbulence, Particle Acceleration, Plasma-Particle Interactions, Shock Fronts, Stellar Evolution, Supernova Remnants, Cassiopeia A, Gas Flow, Magnetic Fields, Particle Diffusion, Solar Wind, Supersonic Speed, Turbulence Effects

Scientific paper

The acceleration of fast particles by a combination of shock fronts and large-scale plasma motions with frozen-in magnetic field is examined. An equation describing fast-particle acceleration is obtained, and the effective time of particle acceleration by supersonic turbulence is determined. The study is applied to the examination of acceleration in the shell of Cassiopeia A.

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