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• W2049549181 abstract "In this paper we summarize and synthesize the results on the role of magnetic shear in the flare process that have been derived from the series of Flare Buildup Study Workshops in the Solar Maximum Analysis program. With emphasis on observations, we discuss the mechanisms that seem to produce the sheared magnetic configurations observed in flaring active regions. The spatial and temporal correlations of this shear with the onset of solar flares are determined from quantitative analyses of measurements of the vector magnetic field. The question of why some areas of sheared magnetic fields are the sites of flares and others are not is investigated observationally. We conclude by synthesizing these findings with current theoretical models of stressed magnetic fields that lead to the eruption of a flare." @default.
• W2049549181 created "2016-06-24" @default.
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• W2049549181 date "1986-01-01" @default.
• W2049549181 modified "2023-10-16" @default.
• W2049549181 title "Measurement and interpretation of magnetic shear in solar active regions" @default.
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• W2049549181 doi "https://doi.org/10.1016/0273-1177(86)90105-5" @default.
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