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Please use this identifier to cite or link to this item:
http://hdl.handle.net/2014/27598
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| Title: | Evolving Magnetic Structures and Their Relation to Coronal Mass Ejections |
| Authors: | Feynman, J. |
| Issue Date: | 1996 |
| 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. |
| URI: | http://hdl.handle.net/2014/27598 |
| Appears in Collections: | JPL TRS 1992+
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