The back action of accelerated particles on shock-front structure

Details The back action of accelerated particles on shock-front structure The back action of accelerated particles on shock-front structure

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61..882b&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, Sept.-Oct. 1984, p. 882-891) Soviet Astronomy (ISSN 0038-5301), vol. 28, Sept.-Oct. 1984, p.

Astronomy and Astrophysics

Astronomy

1

Cosmic Rays, Magnetohydrodynamic Flow, Particle Acceleration, Shock Fronts, Supernova Remnants, Flow Velocity, Radiation Pressure, Viscosity

Scientific paper

Acceleration of particles in the vicinity of shock wave fronts is considered. Particular attention is paid to the reverse influence of the accelerated particles on the flow of plasma in the vicinity of the front. The effectiveness of particles acceleration by weakly non-linear waves is also discussed. It is demonstrated that the shock waves of the type considered are evolutionary. If the viscosity is taken into account, these waves are continuous by their structure. The results obtained are applied to the problem of acceleration of cosmic rays in supernova remnants.

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