Chemical composition of primary cosmic rays in the energy region 10 exp 15 - 10 exp 16 eV based on data from the Baksan neutrino observatory

Details Chemical composition of primary cosmic rays in the energy region 10 exp 15 - 10 exp 16 eV based on data from the Baksan neutrino observatory Chemical composition of primary cosmic rays in the energy region 10 exp 15 - 10 exp 16 eV based on data from the Baksan neutrino observatory

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993roizf..57..117v&link_type=abstract

Rossijskaya Akademiya Nauk, Izvestiya, Seriya Fizicheskaya (ISSN 0367-6765), vol. 57, no. 4, p. 117-120.

Computer Science

Chemical Composition, Cosmochemistry, Energy Spectra, Muons, Primary Cosmic Rays, Elementary Particle Interactions, Particle Telescopes

Scientific paper

A multiplicity spectrum is obtained for muons with a threshold energy of 0.25 TeV in groups of 20-200 particles in a telescope. The spectrum is used to derive the chemical composition of primary cosmic rays with energies of 10 exp 15 - 10 exp 16. The experimental data contradict the hypothesis about the increased role of iron nuclei in primary cosmic rays beyond the bend.

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