The Nature of Solar Prominences pp 237-273 | Cite as
The Death of Prominences
Chapter
Abstract
Whether prominences, like surges, exist for only hours, or, like quiescent filaments, live for many months, sooner or later they disappear, and we are faced with the task of explaining the physical processes that bring about their demise. The disappearing act may take any of several forms, ranging from spectacular displays of violent disruptive motions to slow dimming and disappearance in situ. In some cases the disappearance coincides with changes of the above lying corona; in other instances hardly any effect is noticed in the prominence’s environment.
Keywords
Current Sheet Coronal Mass Ejection Flux Tube Flux Rope Pivot Point
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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Copyright information
© Springer Science+Business Media Dordrecht 1995