Titlebook: Eruptive Solar Flares; Proceedings of Collo Zdeněk ?vestka,Bernard V. Jackson,Marcos E. Machad Conference proceedings 1992 Springer-Verlag

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The intrinsic relationship between flares and eruption of filament currents,ance of the X-ray flare is proportional to the rate of the increase of the total energy prior to the filament eruption. On the basis of these results, we concluded that there is an intimate relationship between the flare and eruptive filament quantitatively.

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MODE

History and basic characteristics of eruptive flares, of a white-light flare by Carrington and Hodgson in 1859, we cover in succession the highlights: Hale‘s invention of the spectroheliograph in 1892 and the spectrohelioscope in 1926 started flare observations in Hα. The institution of a world-wide flare patrol brought significant advances in knowled

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Basic magnetic configuration and energy supply processes for an interacting flux model of eruptive s and interactions of separate flux systems; the process of preflare energy storage in excess of potential due to photospheric motions; the conditions for flare occurrence, including shear in the corona and complexity and the roles of spot motions, flux cancellation and prominences; theories for eru

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The role of cancelling magnetic fields in the buildup to erupting filaments and flares,this scenario involves the formation of a filament magnetic field in the corona above a photospheric polarity inversion where cancelling magnetic fields are observed. The formation of a filament magnetic field is accomplished in several recent models by first interpreting the cancelling fields as a

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Interaction of large-scale magnetic structures in solar flares,ved the likely location of the separatrices, surfaces that separate cells of different field line connectivities, and of the separator which is the intersection of the separatrices. The connectivity of every magnetic field line, which is defined by the dipoles located at its ends, is computed by a c

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死亡

Filament eruptions, flaring arches and eruptive flares,intaining 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 bui

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