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VOLUME 42 (1985) | ISSUE 7 | PAGE 307
Underground cascades in muon groups: new method for determining the chemical composition of the primary cosmic rays
Data from the underground scintillation telescope at the Baksan Neutrino Observatory are used to propose a new experimental method for determining the average atomic number of the primary nuclei in the energy range 1012-1014 eVY nucleon. The first results, from 7500 h of observation, are reported.