{
  "id": "1804.07216",
  "version": "v1",
  "published": "2018-04-19T15:11:41.000Z",
  "updated": "2018-04-19T15:11:41.000Z",
  "title": "The Protons in Primary Cosmic Rays in the Energy Range 10^15-10^17 eV According to Data from the PAMIR Experiment",
  "authors": [
    "V. S. Puchkov",
    "E. A. Kanevskaya",
    "V. M. Maximenko",
    "R. A. Mukhamedshin",
    "S. E. Pyatovsky"
  ],
  "journal": "32nd International Cosmic Ray Conference, Beijing 2011",
  "categories": [
    "astro-ph.HE",
    "hep-ex",
    "physics.ins-det",
    "physics.space-ph"
  ],
  "abstract": "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.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2018-04-19T15:11:41.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "primary cosmic rays",
      "energy range",
      "pamir experiment",
      "x-ray emulsion chamber",
      "mass composition"
    ],
    "tags": [
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}