{
  "id": "0711.1237",
  "version": "v1",
  "published": "2007-11-08T10:26:44.000Z",
  "updated": "2007-11-08T10:26:44.000Z",
  "title": "Phenomenology of turbulent dynamo growth and saturation",
  "authors": [
    "Rodion Stepanov",
    "Franck Plunian"
  ],
  "comment": "17 pages, 6 figures, submitted to ApJ",
  "doi": "10.1086/587795",
  "categories": [
    "astro-ph"
  ],
  "abstract": "With a non local shell model of magnetohydrodynamic turbulence we investigate numerically the turbulent dynamo action for low and high magnetic Prandtl numbers ($Pm$). The results obtained in the kinematic regime and along the way to dynamo saturation are understood in terms of a phenomenological approach based on the local ($Pm\\ll 1$) or non local ($Pm\\gg 1$) nature of the energy transfers. In both cases the magnetic energy grows at small scale and saturates as an inverse `` cascade ''.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2007-11-08T10:26:44.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "turbulent dynamo growth",
      "saturation",
      "non local shell model",
      "phenomenology",
      "high magnetic prandtl numbers"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "journal": "The Astrophysical Journal",
      "year": 2008,
      "month": "Jun",
      "volume": 680,
      "number": 1,
      "pages": 809
    },
    "note": {
      "typesetting": "TeX",
      "pages": 17,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 767028,
      "adsabs": "2008ApJ...680..809S"
    }
  }
}