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- W193459008 abstract "Although various models of CME initiation have been proposed, it is still difficult to test them on the basis of observations, because the observables, as they have been suggested, are controversial in themselves. We point out that the existing models are either biased to the three-part structure that contains a flux rope, or leaving the properties of the associated flare unexplained, even though some models are essentially flare models. We emphasize the possible importance of flares in the whole picture of the CME processes, especially when we discuss large and energetic CMEs, which gain high velocities close to the Sun. It is these fast and extended CMEs that seem to have major impact in space weather." @default.
- W193459008 created "2016-06-24" @default.
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- W193459008 date "2002-01-01" @default.
- W193459008 modified "2023-09-26" @default.
- W193459008 title "Initiation of Coronal Mass Ejections Constraints on Models from Observations" @default.
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- W193459008 doi "https://doi.org/10.1016/s0964-2749(02)80144-5" @default.
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