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• W2086358970 startingPage "A40" @default.
• W2086358970 abstract "Context. Magnetic reconnection is understood to be fundamental to energy release in solar eruptive events (SEEs). In these events reconnection produces a magnetic flux rope above an arcade of hot flare loops. Breakout reconnection, a secondary reconnection high in the corona between this flux rope and the overlying magnetic field, has been hypothesized. Direct observational evidence for breakout reconnection has been elusive, however." @default.
• W2086358970 created "2016-06-24" @default.
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• W2086358970 date "2013-06-26" @default.
• W2086358970 modified "2023-10-18" @default.
• W2086358970 title "Radio evidence for breakout reconnection in solar eruptive events" @default.
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• W2086358970 doi "https://doi.org/10.1051/0004-6361/201321111" @default.
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