Particle acceleration in supernova remnants

Details Particle acceleration in supernova remnants Particle acceleration in supernova remnants

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..264..189d&link_type=abstract

In: Particle acceleration in cosmic plasmas; Proceedings of the Workshop, Bartol Research Inst., Newark, DE, Dec. 4-6, 1991 (A93

Astronomy and Astrophysics

Astronomy

2

Diffusion Coefficient, Particle Acceleration, Particle Energy, Shock Heating, Supernova Remnants, Astronomical Models, Interstellar Matter

Scientific paper

The paper surveys evidence for particle acceleration in SNRs and discusses theoretical models. Observations of shocks in the heliosphere show convincingly that at plasma parameters quite comparable to those of the ISM strong shocks are associated with copious particle acceleration. In one case where simplified models were tested, the simplified models are in reasonable agreement with detailed hydrodynamic two-fluid models (which are in turn in reasonable agreement with calculations incorporating the full spectrum).

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