Cosmic ray anisotropy in the diffusion model of a single source

Details Cosmic ray anisotropy in the diffusion model of a single source Cosmic ray anisotropy in the diffusion model of a single source

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989zhetf..96..798b&link_type=abstract

Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0044-4510), vol. 96, Sept. 1989, p. 798-810. In Russian.

Astronomy and Astrophysics

Astronomy

4

Anisotropic Media, Cosmic Rays, Diffusion Theory, Energetic Particles, Particle Diffusion, Active Galactic Nuclei, Diffusion Coefficient, Local Group (Astronomy)

Scientific paper

The anisotropy of ultrahigh energy cosmic rays is studied in the diffusion model of a single pulsed source. It is shown that, for short-duration pulses generated by the source, the anisotropy decreases with increasing energy. A model for an ultrahigh energy cosmic ray source generating the rays in the neighboring active nucleus of the galaxy is considered.

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