{
  "id": "0910.3746",
  "version": "v1",
  "published": "2009-10-20T05:40:11.000Z",
  "updated": "2009-10-20T05:40:11.000Z",
  "title": "On Formation Of A Shock Wave In Front Of A Coronal Mass Ejection With Velocity Exceeding The Critical One",
  "authors": [
    "M Eselevich"
  ],
  "comment": "3 figures",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "New study confirms conclusions made in [M. Eselevich, and V. Eselevich, 2008]; according to it, there is a disturbed region expended along the CME propagation direction in front of a coronal mass ejection whose velocity $u$ is lower than the critical $u_C$ relative to the surrounding coronal plasma. The time difference brightness (plasma density) in the disturbed region smoothly decreases to larger distances in front of CME. A shock wave forms at u higher than $u_C$ in the front part of the disturbed region manifested as a discontinuity in radial distributions of the difference brightness.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2009-10-20T05:40:11.000Z"
    }
  ],
  "analyses": {
    "subjects": [
      "95.30.Qd",
      "94.20.Fg",
      "96.50.Fm",
      "96.60.ph"
    ],
    "keywords": [
      "coronal mass ejection",
      "velocity exceeding",
      "disturbed region",
      "cme propagation direction",
      "study confirms conclusions"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1063/1.3395899",
      "journal": "Twelfth International Solar Wind Conference",
      "year": 2010,
      "month": "Mar",
      "volume": 1216,
      "pages": 444
    },
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 834507,
      "adsabs": "2010AIPC.1216..444E"
    }
  }
}