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...
Bewaard in:
| Hoofdauteur: | |
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| Formaat: | Artigo |
| Taal: | Inglês |
| Gepubliceerd in: |
Springer
2009-12-01
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| Reeks: | Living Reviews in Solar Physics |
| Onderwerpen: | |
| Online toegang: | http://www.livingreviews.org/lrsp-2009-4 |
| Tags: |
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