Home
For authors
Submission status

Current
Archive
Archive (English)
   Volumes 21-40
   Volumes 1-20
   Volumes 41-62
      Volume 62
      Volume 61
      Volume 60
      Volume 59
      Volume 58
      Volume 57
      Volume 56
      Volume 55
      Volume 54
      Volume 53
      Volume 52
      Volume 51
      Volume 50
      Volume 49
      Volume 48
      Volume 47
      Volume 46
      Volume 45
      Volume 44
      Volume 43
      Volume 42
      Volume 41
Search
VOLUME 50 | ISSUE 1 | PAGE 5
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.




Permission given by American Institute of Physics is appreciated.