Primary cosmic rays in the ultrahigh energy region based on data from the EAS array of the Moscow State University

Details Primary cosmic rays in the ultrahigh energy region based on data from the EAS array of the Moscow State University Primary cosmic rays in the ultrahigh energy region based on data from the EAS array of the Moscow State University

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993roizf..57...74a&link_type=abstract

Rossijskaya Akademiya Nauk, Izvestiya, Seriya Fizicheskaya (ISSN 0367-6765), vol. 57, no. 4, p. 74-77.

Computer Science

Chemical Composition, Cosmic Ray Showers, Cosmochemistry, Energetic Particles, Primary Cosmic Rays, Energy Spectra, Muons, Spatial Distribution

Scientific paper

The experimental data obtained for the EAS array of the Moscow State
University over the period of 1984-1988 are analyzed with particular
reference to the chemical composition of primary cosmic rays in the
energy range 10 exp 15 - 5 x 10 exp 17 eV. The chemical composition of
primary cosmic rays is derived from the muon component of EAS.

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