Development of a Coronal Helmet Streamer of 24 January 1992

  • E. Hiei
  • A. J. Hundhausen

Abstract

The coronal helmet streamer of 24 January 1992 was one of the most prominent events observed with the Soft X-ray Telescope (SXT) on board the Yohkoh satellite. The helmet was interpreted as the reformation of a closed magnetic structure through reconnection, following a prominence eruption and mass ejection (Hiei et al. 1993).

Keywords

Energy Release High Temperature Region Loop Structure Coronal Loop Discontinuous Jump 
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.

References

  1. Hiei, E., Hundhausen, A.J., and Sime, D.G. (1993) Geophys. Res., L., 20, p 2785ADSCrossRefGoogle Scholar
  2. Svestka, Z., Fontenla, J.M., Machado, M.E., Martin, S.F., Neidig, D.F., and Poletto, G. (1987) Sol. Phys. 108, 237ADSCrossRefGoogle Scholar
  3. Forbes, T.G. and Acton, L.W. (1995) Submitted to Astrophys. J.Google Scholar

Copyright information

© Kluwer Academic Publishers 1996

Authors and Affiliations

  • E. Hiei
    • 1
  • A. J. Hundhausen
    • 2
  1. 1.Meisei UniversityJapan
  2. 2.High Altitude ObservatoryBoulderUSA

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