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- W2004193362 abstract "Abstract Coronal mass ejections (CMEs) are now considered as the solar events causing non-corotating interplanetary shocks. These mass ejections frequently occur in association with flares and/or prominence eruptions, and a coronal hole is always found at the region of departure of the CME. Here we present a scenario for the associated occurrence of all these events. In it the interplanetary shock is formed by a sudden change in the velocity of the solar wind from the hole produced by the same cause that triggers the CME, the flare, and the eruption of the prominence, namely a large scale restructuring of the coronal field due to the emergence at the photosphere of new material with opposite magnetic polarity." @default.
- W2004193362 created "2016-06-24" @default.
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- W2004193362 date "1996-01-01" @default.
- W2004193362 modified "2023-10-02" @default.
- W2004193362 title "A possible scenario for the associated occurrence of flares, prominence eruptions, coronal mass ejections, and coronal holes in relation to interplanetary shocks" @default.
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- W2004193362 doi "https://doi.org/10.1016/0273-1177(95)00586-4" @default.
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