Shock generation of turbulence and cosmic-ray diffusion in the interstellar medium

Details Shock generation of turbulence and cosmic-ray diffusion in the interstellar medium Shock generation of turbulence and cosmic-ray diffusion in the interstellar medium

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..184b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Mar. 1985, p. 184-189) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, Mar.-Apr

Astronomy and Astrophysics

Astronomy

2

Diffusion Coefficient, Galactic Cosmic Rays, Interstellar Matter, Shock Wave Interaction, Turbulence, Interstellar Magnetic Fields, Molecular Clouds, Supernovae, Wave Reflection

Scientific paper

The distribution function of shock waves in the interstellar medium is
derived for a model of supernova shocks interacting with interstellar
clouds. The spectrum of the turbulence fluctuations accompanying the
shocks is established, as are the cosmic-ray diffusion coefficients.

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