The Swelling and Destabilization of a Coronal Mass Ejection (abstract)

Martin, S. F.; Feynman, J.

dc.contributor.author	Martin, S. F.	en_US
dc.contributor.author	Feynman, J.	en_US
dc.date.accessioned	2004-10-06T05:17:34Z
dc.date.available	2004-10-06T05:17:34Z
dc.date.issued	1993-12-06	en_US
dc.identifier.citation	San Francisco, CA	en_US
dc.identifier.clearanceno	93-1658	en_US
dc.identifier.uri	http://hdl.handle.net/2014/35929
dc.description.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	en_US
dc.format.extent	34527 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en_US
dc.subject.other	bugle destabilization coronal mass ejection swelling active region	en_US
dc.title	The Swelling and Destabilization of a Coronal Mass Ejection (abstract)	en_US