{
  "id": "1504.03533",
  "version": "v1",
  "published": "2015-04-14T13:19:08.000Z",
  "updated": "2015-04-14T13:19:08.000Z",
  "title": "Multi-wavelength Fibril Dynamics and Oscillations Above Sunspot - I. Morphological Signature",
  "authors": [
    "Emanuel Sungging Mumpuni",
    "Dhani Herdiwijaya",
    "Mitra Djamal",
    "Thomas Djamaluddin"
  ],
  "comment": "16 pages, 13 figures",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "In this work we selected one particular fibril from a high resolution solar chromosphere observation from the Dutch Open Telescope, and tried to obtain a broad picture of the intricate mechanism that might be incorporated in the multiple layer of the Solar atmosphere in high cadence multi-wavelength observation. We analyzed the changingvfibril patter using multi-wavelength tomography, which consists of both H$\\alpha$ line center \\& the blue wing, Doppler-signal, Ca II H, and the G-band. We have found that the intermittent ejected material through fibril from Doppler images has clearly shown oscillation mode, as seen in the H$\\alpha$ blue wing. The oscillations in the umbrae and penumbrae magnetic field lines that are above the sunspot cause a broadening and forms the area like a ring shape from 3 to 15-minute oscillations as function of height. These made a distinct boundary of umbrae and penumbrae which suggest the comb structure, and indicate that the oscillations could propagate along the inclined magnetic flux tubes from below. The 3-minute strongly appeared in the broadly inclined penumbrae magnetic filed lines and gave the clear light-bridge. The well known 5-minute was dominated in the umbrae-penumbrae region boundary, the long 7-minute one was transparent in the H$\\alpha$ blue wing, but this was the same with 10 and 15-minute, it was concentrated in the inner-penumbrae, as seen in the H$\\alpha$ line center. From these findings we propose a picture on the role of fibril as the fabric of interaction between the layers, also the related activites around the active region under investigation.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2015-04-14T13:19:08.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "multi-wavelength fibril dynamics",
      "oscillation",
      "penumbrae magnetic filed lines",
      "morphological signature",
      "inclined penumbrae magnetic"
    ],
    "publication": {
      "doi": "10.1088/1674-4527/15/11/007",
      "journal": "Research in Astronomy and Astrophysics",
      "year": 2015,
      "month": "Nov",
      "volume": 15,
      "number": 11,
      "pages": 1843
    },
    "note": {
      "typesetting": "TeX",
      "pages": 16,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "adsabs": "2015RAA....15.1843S"
    }
  }
}