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...
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| Autor principal: | |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Springer
2009-12-01
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| Col·lecció: | Living Reviews in Solar Physics |
| Matèries: | |
| Accés en línia: | http://www.livingreviews.org/lrsp-2009-4 |
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