Autor: |
Puchkov, V. S., Kanevskaya, E. A., Maximenko, V. M., Mukhamedshin, R. A., Pyatovsky, S. E. |
Rok vydání: |
2018 |
Předmět: |
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Zdroj: |
32nd International Cosmic Ray Conference, Beijing 2011 |
Druh dokumentu: |
Working Paper |
Popis: |
Adjusted data on the fraction of protons in the mass composition of primary cosmic rays (PCRs) in the energy range of 10^15-10^17 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 = 10^15-10^16 eV and does not change within the error for E0 = 10^16-10^17 eV. |
Databáze: |
arXiv |
Externí odkaz: |
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