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On the twist of emerging flux loops in the solar convection zone

✍ Scribed by Y. Fan; Donglai Gong


Book ID
110221944
Publisher
Springer
Year
2000
Tongue
English
Weight
139 KB
Volume
192
Category
Article
ISSN
0038-0938

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If the solar dynamo operates at the bottom of the convection zone, then the magnetic flux created there has to rise to the surface. When the convection zone is regarded as passive, the rising flux is deflected by the Coriolis force to emerge at rather high latitudes, poleward of typical sunspot zone