Anisotropy of cosmic rays at energies of 5 X 10 to the 11th 10 to the 14th eV in the diffusional approximation

Details Anisotropy of cosmic rays at energies of 5 X 10 to the 11th 10 to the 14th eV in the diffusional approximation Anisotropy of cosmic rays at energies of 5 X 10 to the 11th 10 to the 14th eV in the diffusional approximation

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61..610p&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, May-June 1984, p. 610-613) Soviet Astronomy (ISSN 0038-5301), vol. 28, May-June 1984, p. 357

Astronomy and Astrophysics

Astronomy

2

Cosmic Rays, Interstellar Matter, Angular Distribution, Anisotropy, Harmonics, Relativistic Particles

Scientific paper

The amplitudes of the second and third angular harmonics of the
anisotropy of cosmic rays diffusing in the interstellar medium are
calculated. The observed amplitude of the second harmonic is evidently
due to the nonuniformity of the local galactic magnetic field at scales
of 3-10 pc.

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