Computer Science
Scientific paper
Sep 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982izssr..46.1833b&link_type=abstract
(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Samarkand, Uzbek SSR, Oct. 27-29, 1981.) Akademiia Nauk SSSR, Izvestiia, Ser
Computer Science
Cosmic Ray Showers, Electron Photon Cascades, Particle Energy, Particle Flux Density, Primary Cosmic Rays, Energy Spectra, Muons, Nuclear Interactions, Nucleons
Scientific paper
Calculations obtained on the basis of the model of Boyadjian et al. (1981) are discussed. The dependence of Ne on atmospheric depth is calculated for showers produced by a primary nucleon and nucleus with A-10; and the dependence of the number of muons with energy exceeding 10 GeV on the primary energy for a height of 700 g/sq cm is presented. It is shown that in scaling models with allowance for complex chemical composition, it is possible to obtain mean EAS characteristics which do not differ much from experimentally measured characteristics.
Boiadzhian N. G.
Dallakian Iu. P.
Gariaka A. P.
Mamidzhanian E. A.
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