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Evolving Magnetic Structures and Their Relation to Coronal Mass Ejections

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dc.contributor.author Feynman, J. en_US
dc.date.accessioned 2004-10-01T06:06:16Z
dc.date.available 2004-10-01T06:06:16Z
dc.date.issued 1996 en_US
dc.identifier.clearanceno 96-1649 en_US
dc.identifier.uri http://hdl.handle.net/2014/27598
dc.description.abstract Solar activity regions are frequently concentrated into cluster which persist for many solar rotations. These activity complexes are associated with weak dispersed magnetic fields which are most apparent after the activity itself has ceased. We call this combination of persistent activity and dispersed Evolving Magnetic Structures (EMS). Here we show examples of EMSs and describe the evolution of an EMS associated with major Coronal Mass Ejections (CME) and other solar and magnetic disturbances. en_US
dc.format.extent 1460819 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other evolving magnetic structures EMS coronal mass ejections CME solar activity solar magnetic activity en_US
dc.title Evolving Magnetic Structures and Their Relation to Coronal Mass Ejections en_US


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