Observation of ``the knee" in cosmic ray energy spectrum with underground muons and primary mass composition in the range 10^15-10^17 eV

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Scientific paper

The method of recalculation from the muon multiplicity spectrum to the extensive air showers spectrum vs the total muon number, n_mu, is presented. The method allows the direct comparison of data obtained in different experiments with muon groups. The direct comparison of the data at n_mu> 1800 and n_mu= 75-660 has been carried out. The data in the region n_mu= 75-3500 agree better with the assumption that the slope change in the energy spectrum of primary cosmic rays occurs at the same energy per nucleus E_c~=3.10^15 eV and the mass composition in energy range 10^15-10^17 eV is close to the one observed at 10^14 eV.

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