Combining Models of Coronal Mass Ejections and Solar Dynamos
Observations show that Coronal Mass Ejections (CMEs) are associated with twisted magnetic flux configurations. Conventionally, CMEs are modeled by shearing and twisting the footpoints of a certain distribution of magnetic flux at the solar surface and letting it evolve at the surface. Of course, the...
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| Format: | Doctoral Thesis |
| Language: | English |
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Stockholms universitet, Institutionen för astronomi
2013
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| Online Access: | http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-88896 http://nbn-resolving.de/urn:isbn:978-91-7447-675-0 |