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A theoretical model of torsional oscillations from a flux transport dynamo model
Published online by Cambridge University Press: 26 August 2011
Abstract
Assuming that the torsional oscillation is driven by the Lorentz force of the magnetic field associated with the sunspot cycle, we use a flux transport dynamo to model it and explain its initiation at a high latitude before the beginning of the sunspot cycle.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 6 , Symposium S273: The Physics of Sun and Star Spots , August 2010 , pp. 366 - 368
- Copyright
- Copyright © International Astronomical Union 2011