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The Initiation of Coronal Mass Ejections by Newly Emerging Magnetic Flux

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dc.contributor.author Feynman, J. en_US
dc.contributor.author Martin, S. F. en_US
dc.date.accessioned 2004-10-05T05:40:05Z
dc.date.available 2004-10-05T05:40:05Z
dc.date.issued 1994
dc.identifier.clearanceno 94-1229
dc.identifier.uri http://hdl.handle.net/2014/33291
dc.description.abstract We present observational evidence that eruptions of quiescent filaments and associated coronal mass ejections (CMEs) occur as a consequence of the destabilization of large-scale coronal arcades due to interactions between these structures and new and growing active regions. en_US
dc.format.extent 1966176 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other solar flares en_US
dc.title The Initiation of Coronal Mass Ejections by Newly Emerging Magnetic Flux en_US


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