The Protons in Primary Cosmic Rays in the Energy Range 1015-1017 eV According to Data from the PAMIR Experiment
Abstract
Adjusted data on the fraction of protons in the mass composition of primary cosmic rays (PCRs) in the energy range of 1015-1017 eV are presented. Adjustments are made according to detailed calculations of the response of the X-ray emulsion chamber in the PAMIR experiment. It is demonstrated that the fraction of protons in a PCR is 16-18% for E0 = 1015-1016 eV and does not change within the error for E0 = 1016-1017 eV.
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