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The Swelling and Destabilization of a Coronal Mass Ejection (abstract)We will present and discuss data for a bugle that was particularly well observed. Apparently the swelling of the bugle and its destabilization were caused by the newly emerging flux and its interaction with the pre-existing active regions and coronal structures.
Document ID
20060039416
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
hdl:2014/35929
Authors
Martin, S. F.
Feynman, J.
Date Acquired
August 23, 2013
Publication Date
December 6, 1993
Distribution Limits
Public
Copyright
Other
Keywords
bugle destabilization coronal mass ejection swelling active region

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