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Observations of NOAA 8210 Using MOF and DHC of Kanzelhöhe Solar Observatory

  • A. Warmuth
  • A. Hanslmeier
  • M. Messerotti
  • A. Cacciani
  • P. F. Moretti
  • W. Otruba
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 259)

Abstract

Two new instruments have recently been introduced at Kanzelhohe Solar Observatory: the Magneto-Optical Filter (MOF), a compact imaging Doppler-magnetograph and the Digital Hα Camera (DHC). In 1998, these instruments were first used in high-cadence mode to support a SOHO/UVCS campaign. During this campaign, NOAA 8210 rotated onto the disk, evolved rapidly and produced several major flares. Furthermore, we point out the perspectives for our planned Flare Monitoring and Alerting System, since the two new instruments are crucial components for this program.

Keywords

Solar Phys Neutral Line Solar Observatory Moreton Wave Free Magnetic Energy 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

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Copyright information

© Springer Science+Business Media Dordrecht 2001

Authors and Affiliations

  • A. Warmuth
    • 1
  • A. Hanslmeier
    • 1
  • M. Messerotti
    • 2
  • A. Cacciani
    • 3
  • P. F. Moretti
    • 4
  • W. Otruba
    • 5
  1. 1.Institut für Geophysik, Astrophysik und MeteorologieKarl-Franzens-Universität GrazGrazAustria
  2. 2.Osservatorio Astronomico di TriesteTriesteItaly
  3. 3.Department of PhysicsUniversity of Rome "La Sapienza"RomeItaly
  4. 4.Osservatorio Astronomico di CapodimonteNapoliItaly
  5. 5.Sonnenobservatorium KanzelhöheTreffenAustria

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