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• W2023124111 startingPage "A119" @default.
• W2023124111 abstract "Context. Solar flares are powered by energy stored in the coronal magnetic field, a portion of which is released when the field reconfigures into a lower energy state. Investigation of sunspot magnetic field topology during flare activity is useful to improve our understanding of flaring processes." @default.
• W2023124111 created "2016-06-24" @default.
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• W2023124111 date "2013-02-01" @default.
• W2023124111 modified "2023-10-18" @default.
• W2023124111 title "Evidence for partial Taylor relaxation from changes in magnetic geometry and energy during a solar flare" @default.
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• W2023124111 doi "https://doi.org/10.1051/0004-6361/201219964" @default.
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