Dependence of the Occurrence of Coronal Mass Ejections on the Initial Length of the Eruptive Prominence

A model of the eruption of a magnetic flux rope with ends rigidly fixed in the photosphere is analyzed. Long and short flux ropes exhibit different scenarios of eruption, other conditions being equal. Short flux ropes accelerate quickly but for a short time, and they can be quite easily stopped at a...

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Bibliographic Details
Published in:Geomagnetism and Aeronomy Vol. 62; no. 3; pp. 151 - 158
Main Author: Filippov, B. P.
Format: Journal Article
Language:English
Published: Moscow Pleiades Publishing 01-06-2022
Springer Nature B.V
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Online Access:Get full text
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