Efficiency of charged-particle acceleration by shocks in supernova remnants and in solar flares

Details Efficiency of charged-particle acceleration by shocks in supernova remnants and in solar flares Efficiency of charged-particle acceleration by shocks in supernova remnants and in solar flares

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..594b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Aug. 1984, p. 594-599) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, July-Aug

Astronomy and Astrophysics

Astronomy

3

Cosmic Rays, Particle Acceleration, Shock Wave Propagation, Solar Flares, Supernova Remnants, Radio Emission, Stellar Envelopes, Turbulence Effects

Scientific paper

An assumption on cosmic rays acceleration by shock waves in supernova shells is shown to be able to explain some characteristics of radio emission of old supernova remnants. The role of accelerated particles pressure in shell dynamics seems not to be great. A level of turbulence is evaluated which is necessary for this mechanism of acceleration taking place in solar flares.

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