{
  "id": "2010.04236",
  "version": "v1",
  "published": "2020-10-08T19:37:49.000Z",
  "updated": "2020-10-08T19:37:49.000Z",
  "title": "Results of the further analysis of Tien-Shan array data on the energy spectrum of primary cosmic rays at 2x10$^{13}$ - 3x10$^{17}$ eV",
  "authors": [
    "E. Gudkova",
    "N. Nesterova"
  ],
  "comment": "4 pages, 3 figures",
  "journal": "Physics of Atomic Nuclei, 83 (4), pp. 629-633 (2020)",
  "doi": "10.1134/S1063778820030102",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "The energy spectrum of primary cosmic rays at energies between at 2x10$^{13}$ - 3x10$^{17}$ eV is presented according to data from the Tien Shan array on the basis of the detection of the number of electrons in extensive air showers. In the energy range 5x10$^{15}$ - 3x10$^{17}$ eV, the spectrum was obtained by means of the HADRON array and was extended to the region of lower energies from 2x10$^{13}$ eV on the basis of the results of an individual experiment. The changes in the slope of the spectrum in the energy range of 10$^{16}$ - 3x10$^{17}$ eV and a feature of this spectrum at about 1017 eV are analyzed in detail and are described. The spectrum in question is compared with the results obtained at some other arrays.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2020-10-08T19:37:49.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "primary cosmic rays",
      "tien-shan array data",
      "energy spectrum",
      "energy range 5x10",
      "tien shan array"
    ],
    "tags": [
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}