Cosmic-ray diffusion in the coronal phase of the interstellar medium

Details Cosmic-ray diffusion in the coronal phase of the interstellar medium Cosmic-ray diffusion in the coronal phase of the interstellar medium

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60.1102f&link_type=abstract

(Astronomicheskii Zhurnal, vol. 60, Nov.-Dec. 1983, p. 1102-1106) Soviet Astronomy (ISSN 0038-5301), vol. 27, Nov.-Dec. 1983, p.

Astronomy and Astrophysics

Astronomy

1

Cosmic Rays, Interstellar Matter, Magnetohydrodynamic Turbulence, Magnetohydrodynamic Waves, Anisotropy, Particle Diffusion, Relativistic Particles, Stellar Coronas

Scientific paper

Hydromagnetic turbulence in the coronal phase of the interstellar medium
is examined. It is shown that Alfven waves generated by the relativistic
cosmic ray particles will produce turbulence that can act as a cosmic
ray diffusion mechanism. Cosmic rays would then acquire an anisotropy
compatible with observations.

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