Hydromagnetic turbulence, shock waves and particle acceleration in supernova remnants

Details Hydromagnetic turbulence, shock waves and particle acceleration in supernova remnants Hydromagnetic turbulence, shock waves and particle acceleration in supernova remnants

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..96...25f&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 96, no. 1, Oct. 1983, p. 25-36.

Astronomy and Astrophysics

Astrophysics

10

Magnetohydrodynamic Turbulence, Particle Acceleration, Shock Waves, Supernova Remnants, Small Perturbation Flow

Scientific paper

A number of mechanisms for generation of the small-scale hydromagnetic
turbulence in supernova remnants is investigated. It is shown that the
mechanisms of particle acceleration on the shock waves and on the
large-scale turbulence face considerable difficulties.

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