Magnetic Fields in the Solar Convection Zone
Active regions on the solar surface are generally thought to originate from a strong toroidal magnetic field generated by a deep seated solar dynamo mechanism operating at the base of the solar convection zone. Thus the magnetic fields need to traverse the entire convection zone before they reach th...
| Main Author: | |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
SpringerOpen
2009-12-01
|
| Series: | Living Reviews in Solar Physics |
| Subjects: | |
| Online Access: | http://www.livingreviews.org/lrsp-2009-4 |