{
  "id": "1410.3725",
  "version": "v1",
  "published": "2014-10-14T15:15:14.000Z",
  "updated": "2014-10-14T15:15:14.000Z",
  "title": "Magnetohydrodynamics and Solar Physics",
  "authors": [
    "Michel Rieutord"
  ],
  "comment": "6 pages; 4 figures; Contribution to the SF2A 2014 annual conference",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "In this short review, I present some of the recent progresses on the pending questions of solar physics. These questions let us revisit the solar wind, the solar dynamo problem, the dynamics of the photosphere and finally have a glimpse at other solar type stars. Discussing the use of direct numerical simulations in solar physics, I show that the full numerical calculation of the flow in a single supergranule would require more electric power than the luminosity of the sun itself with present computer technology.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2014-10-14T15:15:14.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "solar physics",
      "magnetohydrodynamics",
      "solar dynamo problem",
      "solar type stars",
      "computer technology"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 6,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "adsabs": "2014sf2a.conf...45R"
    }
  }
}