Possible contribution of primary gamma-rays to the observed cosmic-ray anisotropy

Details Possible contribution of primary gamma-rays to the observed cosmic-ray anisotropy Possible contribution of primary gamma-rays to the observed cosmic-ray anisotropy

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nciml..42..321a&link_type=abstract

Nuovo Cimento, Lettere, Serie 2, vol. 42, April 1, 1985, p. 321-324.

Physics

15

Anisotropy, Cosmic Ray Showers, Galactic Cosmic Rays, Gamma Rays, Primary Cosmic Rays, Cos-B Satellite, High Energy Interactions, Particle Energy, Particle Flux Density

Scientific paper

The contribution of gamma-rays from the galactic plane to the cosmic-ray counting rate is calculated. The calculations are based on gamma-ray flux measurements carried out by means of the Baksan extensive air shower (EAS) gamma-ray detector. A good fit to the known cosmic-ray anisotropy was found for primary energies of 10 to the 13-10 to the 14th eV.

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