Evolving Magnetic Structures and Their Relation to Coronal Mass Ejections

Feynman, J.

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