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

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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


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