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Abstract

We investigated the mechanism of the disparition brusque, i.e., the sudden disappearance of a prominence (e.g., Tandberg-Hanssen 1995), observed with an Hα limb filtergraph by comparing Yohkoh SXT observations and Hα observations.

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References

  • Tonooka, H., et al., 1995, in Magnetodynamic Phenomena in the Solar Atmosphere - Prototypes of Stellar Magnetic Activity, ed. Ucliida, Y., et al, Kluwer Acad. Publ. pp.493

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  • Tandberg-Hanssen, E., 1995, The Nature of Solar Prominences, Kluwer Acad. Publ.

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© 1998 Springer Science+Business Media Dordrecht

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Tonooka, H. et al. (1998). Soft X-ray Features of Prominence Eruption and Disappearance. In: Watanabe, T., Kosugi, T., Sterling, A.C. (eds) Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond. Astrophysics and Space Science Library, vol 229. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5220-4_65

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  • DOI: https://doi.org/10.1007/978-94-011-5220-4_65

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6198-8

  • Online ISBN: 978-94-011-5220-4

  • eBook Packages: Springer Book Archive

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