{
  "id": "1001.1635",
  "version": "v1",
  "published": "2010-01-11T12:02:27.000Z",
  "updated": "2010-01-11T12:02:27.000Z",
  "title": "Physics of Solar Prominences: II - Magnetic Structure and Dynamics",
  "authors": [
    "D. H. Mackay",
    "J. T. Karpen",
    "J. L. Ballester",
    "B. Schmieder",
    "G. Aulanier"
  ],
  "comment": "75 pages, 31 pictures, review paper",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "Observations and models of solar prominences are reviewed. We focus on non-eruptive prominences, and describe recent progress in four areas of prominence research: (1) magnetic structure deduced from observations and models, (2) the dynamics of prominence plasmas (formation and flows), (3) Magneto-hydrodynamic (MHD) waves in prominences and (4) the formation and large-scale patterns of the filament channels in which prominences are located. Finally, several outstanding issues in prominence research are discussed, along with observations and models required to resolve them.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2010-01-11T12:02:27.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "magnetic structure",
      "solar prominences",
      "prominence research",
      "observations",
      "prominence plasmas"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1007/s11214-010-9628-0",
      "journal": "Space Science Reviews",
      "year": 2010,
      "month": "Apr",
      "volume": 151,
      "number": 4,
      "pages": 333
    },
    "note": {
      "typesetting": "TeX",
      "pages": 75,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 842544,
      "adsabs": "2010SSRv..151..333M"
    }
  }
}