Cosmic rays in supernova remnants with different rates of their injection into the regular-acceleration regime

Details Cosmic rays in supernova remnants with different rates of their injection into the regular-acceleration regime Cosmic rays in supernova remnants with different rates of their injection into the regular-acceleration regime

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987izssr..51.1790b&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskaia (ISSN 0367-6765), vol. 51, Oct. 1987, p. 1790-1792. In Russian.

Physics

1

Cosmic Rays, Particle Acceleration, Shock Wave Propagation, Supernova Remnants, Carrier Injection, Propagation Velocity, Shock Fronts

Scientific paper

Calculation results on the regular acceleration of cosmic rays by a shock wave from a supernova remnant are presented for a Mach number of 10 and a shock front velocity of 3000 km/s, and saturated and unsaturated injection regimes are shown to occur. It is found that, under saturated injection conditions, cosmic rays are efficiently shock-accelerated and have a substantial effect on the shock-wave structure. The unsaturated regime occurs for a very wide range of particle-injection rates.

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