Magnetic Fields in the Solar Convection Zone
Recent studies of the dynamic evolution of magnetic flux tubes in the solar convection zone are reviewed with focus on emerging flux tubes responsible for the formation of solar active regions. The current prevailing picture is that active regions on the solar surface originate from strong toroidal...
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| Format: | Article |
| Language: | English |
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Springer
2004-07-01
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| Series: | Living Reviews in Solar Physics |
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| Online Access: | http://www.livingreviews.org/lrsp-2004-1 |