{
  "id": "1101.4342",
  "version": "v1",
  "published": "2011-01-23T04:56:51.000Z",
  "updated": "2011-01-23T04:56:51.000Z",
  "title": "Possible explanations of the Maunder minimum from a flux transport dynamo model",
  "authors": [
    "Bidya Binay Karak",
    "Arnab Rai Choudhuri"
  ],
  "comment": "4 pages, 2 figures, Proceedings of IAU symposium 273, Physics of Sun and star spots, Ventura, California 22-26 August 2010",
  "categories": [
    "astro-ph.SR",
    "astro-ph.EP",
    "astro-ph.HE"
  ],
  "abstract": "We propose that at the beginning of the Maunder minimum the poloidal field or amplitude of meridional circulation or both fell abruptly to low values. With this proposition, a flux transport dynamo model is able to reproduce various important aspects of the historical records of the Maunder minimum remarkably well.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2011-01-23T04:56:51.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "flux transport dynamo model",
      "explanations",
      "poloidal field",
      "meridional circulation",
      "low values"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1017/S1743921311015705"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 885243,
      "adsabs": "2011IAUS..273..430K"
    }
  }
}