The energy spectrum of primary cosmic rays in the range 10 to the 13th-10 to the 16th eV

Details The energy spectrum of primary cosmic rays in the range 10 to the 13th-10 to the 16th eV The energy spectrum of primary cosmic rays in the range 10 to the 13th-10 to the 16th eV

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982izssr..46.1827k&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Samarkand, Uzbek SSR, Oct. 27-29, 1981.) Akademiia Nauk SSSR, Izvestiia, Ser

Physics

1

Cosmic Ray Showers, Energy Spectra, Particle Flux Density, Primary Cosmic Rays, Electron Flux Density, High Energy Electrons, Muons

Scientific paper

Data gathered at Tien Shan over 13,000 hrs are analyzed. At energies between 10 to the 13th and 5 x 10 to the 14th eV, the number of electrons is arrived at using only measurements of shower spectra based on the number of particles. Between 5 x 10 to the 14th and 10 to the 16th eV, the number of electrons comes from an analysis of shower spectra on the basis of the number of electrons and of the number of muons having energies above 5 GeV.

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