{
  "id": "1411.4642",
  "version": "v1",
  "published": "2014-11-17T20:55:51.000Z",
  "updated": "2014-11-17T20:55:51.000Z",
  "title": "Cosmic Ray Physics",
  "authors": [
    "Domenico D'Urso"
  ],
  "comment": "Proceeding of XXXIV Physics in Collision Symposium, Bloomington, Indiana, September 16--20, 2014",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "Cosmic ray story begins at the beginning of XX century. More then 100 years later, most of the main issues are still open questions, as sources, acceleration mechanism, propagation and composition. There is a continuing fascination with the studies of cosmic radiation mostly from the several contradictions connected to its observation. The radiation has an energy spectrum ranging from $\\sim$ 1 GeV to beyond 10$^{20}$ eV with a flux going from 1 particle per m$^2$ per $\\mu$s to less then 1 particle per km$^2$ per century, and so very different experimental techniques are needed to perform cosmic ray measurements in the different energy intervals. In this contribution the actual experimental status of cosmic ray knowledge will be reviewed.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2014-11-17T20:55:51.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "cosmic ray physics",
      "cosmic ray story begins",
      "perform cosmic ray measurements",
      "cosmic ray knowledge",
      "actual experimental status"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1328461,
      "adsabs": "2014arXiv1411.4642D"
    }
  }
}