{
  "id": "1812.07293",
  "version": "v1",
  "published": "2018-12-18T11:00:32.000Z",
  "updated": "2018-12-18T11:00:32.000Z",
  "title": "Observations of the solar chromosphere with ALMA and comparison with theoretical models",
  "authors": [
    "R. Brajša",
    "D. Sudar",
    "I. Skokic",
    "A. O. Benz",
    "M. Kuhar",
    "A. Kobelski",
    "S. Wedemeyer",
    "S. M. White",
    "H. -G. Ludwig",
    "M. Temmer",
    "S. H. Saar",
    "C. L. Selhorst"
  ],
  "comment": "4 pages, presented at The 20th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, July 29 - Aug 3 2018, Boston / Cambridge, USA",
  "doi": "10.5281/zenodo.1462863",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "In this work we use solar observations with the ALMA radio telescope at the wavelength of 1.21 mm. The aim of the analysis is to improve understanding of the solar chromosphere, a dynamic layer in the solar atmosphere between the photosphere and corona. The study has an observational and a modeling part. In the observational part full-disc solar images are analyzed. Based on a modified FAL atmospheric model, radiation models for various observed solar structures are developed. Finally, the observational and modeling results are compared and discussed.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2018-12-18T11:00:32.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "solar chromosphere",
      "theoretical models",
      "observational part full-disc solar images",
      "comparison",
      "alma radio telescope"
    ],
    "tags": [
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}