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Magnetic Fields in the Solar Convection Zone
DOI: 10.12942/lrsp-2004-1
Bibcode: 2004LRSP....1....1F
Fan, Yuhong
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 magnetic fields generated by the solar dynamo mec…
2004
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Living Reviews in Solar Physics
SOHO
74