Underground cascades in muon groups - New method for determining the chemical composition of the primary cosmic rays

Details Underground cascades in muon groups - New method for determining the chemical composition of the primary cosmic rays Underground cascades in muon groups - New method for determining the chemical composition of the primary cosmic rays

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985zhpmr..42..307b&link_type=abstract

(ZHETF Pis'ma v Redaktsiiu, vol. 42, Oct. 10, 1985, p. 307-310) JETP Letters (ISSN 0021-3640), vol. 42, Oct. 10, 1985, p. 380-38

Computer Science

Chemical Composition, Cosmic Ray Showers, Energy Spectra, Muons, Primary Cosmic Rays, Bremsstrahlung, Pions

Scientific paper

A new experimental method for determining the mean atomic number of
primary nuclei in the energy range 10 to the 12th 10 to the 14th eV per
nucleon is described. The method is based on analysis of data from the
underground scintillation telescope at the Baksan Neutrino Observatory
in the USSR. Observational data from 7500 h are reported.

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