Energy spectra of protons and nuclei of primary cosmic rays at energies exceeding 10 TeV

Details Energy spectra of protons and nuclei of primary cosmic rays at energies exceeding 10 TeV Energy spectra of protons and nuclei of primary cosmic rays at energies exceeding 10 TeV

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2083a&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

Computer Science

Energy Spectra, Interstellar Chemistry, Primary Cosmic Rays, Stratosphere Radiation, Cascades, Chemical Composition, Nuclear Emulsions, Nuclei, Particle Energy, Protons

Scientific paper

A nuclear-emulsion technique for determining the chemical composition of primary cosmic rays in the stratosphere is described, and results on protons and nuclei at energies exceeding 10 TeV are reported. Integrated and differential energy spectra of cascades are presented. It is shown that a significant change in the chemical composition of primary cosmic rays at energies exceeding 10 TeV/nucleon results from a sharp increase in the inclination of the proton spectrum as the spectrum of the nuclear component remains unchanged.

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