Analysis of the arrival direction distribution of primary cosmic rays with energies greater than 5 X 10 exp 18 eV

Details Analysis of the arrival direction distribution of primary cosmic rays with energies greater than 5 X 10 exp 18 eV Analysis of the arrival direction distribution of primary cosmic rays with energies greater than 5 X 10 exp 18 eV

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993roizf..57...78k&link_type=abstract

Rossijskaya Akademiya Nauk, Izvestiya, Seriya Fizicheskaya (ISSN 0367-6765), vol. 57, no. 4, p. 78-81.

Physics

Cosmic Ray Showers, Energetic Particles, Primary Cosmic Rays, Radiation Distribution, Anisotropy, Statistical Analysis

Scientific paper

Data from the Yakutsk EAS array on the distribution of the arrival directions of EAS with primary particle energies in excess of 5 x 10 exp 18 eV are presented for the period 1974-1992. Analysis results reveal no statistically meaningful anisotropy in the arrival direction of air showers in the region investigated, although there are indications of a possible increase in particle flow from the equatorial region of the Galaxy at energies of (1-4) x 10 exp 19 eV.

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