About the character of the ``knee'' at E~3.1015eV in the energy spectrum and the mass composition of primary cosmic rays in the energy range 1015-1017eV

Physics – Nuclear Physics

Scientific paper

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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, nμ, is presented. The method allows the direct comparison of data obtained in different experiments with muon groups. The direct comparison of the data at nμ>1800 and nμ=75-650 has been carried out. The data in the region nμ=75-3500 agree better with assumption that the slope change in the energy spectrum of primary cosmic rays occurs at the same energy per nucleus Ec~3.1015eV and the mass composition in energy range 1015-1017eV is close to the one observed at 1014eV.

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