Analysis of cosmic ray propagation through the atmosphere in the light of scaling breakdown

Details Analysis of cosmic ray propagation through the atmosphere in the light of scaling breakdown Analysis of cosmic ray propagation through the atmosphere in the light of scaling breakdown

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981izssr..45.1226e&link_type=abstract

(Evropeiskii Simpozium po Kosmicheskim Lucham, 7th, Leningrad, USSR, Sept. 15-19, 1980.) Akademiia Nauk SSSR, Izvestiia, Seriia

Physics

Atmospheric Physics, Cosmic Rays, Energy Spectra, Particle Interactions, Scaling, Bosons, Gamma Rays, Hadrons, Inelastic Scattering, Primary Cosmic Rays, Sensitivity

Scientific paper

The propagation of cosmic rays through the atmosphere is analyzed by the multigroup method for the energy range 10 to the 11th - 10 to the 15th eV assuming three different kinds of the primary energy spectrum. Comparison of calculations with experimental data shows that none of the models preserving scaling in the inclusive spectrum fragmentation region agrees with the experimental data, while a satisfactory fit is obtained with a nonscaling model of the Bose-Planck type.

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