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VOLUME 50 (1989) | ISSUE 1 | PAGE 6
Use of superposition model in analyzing muon groups generated by high-energy nuclei of the primary cosmic rays
The Monte Carlo method is used to analyze muon groups generated by the nuclei of the primary cosmic rays. A comparison of the characteristics of showers generated by nuclei and protons leads to the conclusion that the superposition model is valid. Calculations have been carried out for Εμ = 0.2 TeV, which corresponds to the lowest threshold energy for the detection of muons at the Baksan underground scintillation telescope.