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- W2044218887 abstract "We investigate the factors responsible for initiating coronal mass ejections (CMEs), specifically, the role of magnetic helicity. Using numerical simulations of the breakout model for CMEs, we show that eruption occurs at a fixed magnitude of free energy in the corona, independent of the value of helicity. Almost identical eruptions are obtained for both large and zero-helicity cases. Furthermore, the eruption can actually lead to an increase in the helicity remaining in the corona. These results argue strongly against recent models that postulate a critical helicity buildup and shedding as the determining factors for CME initiation." @default.
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- W2044218887 date "2005-04-15" @default.
- W2044218887 modified "2023-09-27" @default.
- W2044218887 title "The Role of Magnetic Helicity in Coronal Mass Ejections" @default.
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- W2044218887 doi "https://doi.org/10.1086/430516" @default.
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