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Filament eruptions, flaring arches and eruptive flares

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Eruptive Solar Flares

Part of the book series: Lecture Notes in Physics ((LNP,volume 399))

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Abstract

Several cases of erupting filaments showing distinctly their “feet” have been studied. Role of the feet and their anchorage with the photosphere in maintaining filament stability is established; apart from the footpoint separation and height criteria. Further, a homologous series of more energetic events, namely, the flaring arches and eruptive flares of March 5–7, 1991, suggest a repetitive restoration of magnetic field conditions and energy build-up within a day. High resolution H-alpha observations of these events indicate that large amount of ejected material was “siphoned out” from the chromosphere through, the top. of a low-lying compact emission loop within the active region.

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Zdeněk Švestka Bernard V. Jackson Marcos E. Machado

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© 1992 Springer-Verlag

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Bhatnagar, A., Ambastha, A., Srivastava, N. (1992). Filament eruptions, flaring arches and eruptive flares. In: Švestka, Z., Jackson, B.V., Machado, M.E. (eds) Eruptive Solar Flares. Lecture Notes in Physics, vol 399. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-55246-4_77

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  • DOI: https://doi.org/10.1007/3-540-55246-4_77

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-55246-8

  • Online ISBN: 978-3-540-46794-6

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