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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© 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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