A theoretical model of torsional oscillations from a flux transport dynamo model

Details A theoretical model of torsional oscillations from a flux transport dynamo model A theoretical model of torsional oscillations from a flux transport dynamo model

2010-08-12

arxiv.org/abs/1008.2161v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

3 pages, 2 figures. proceedings of IAU symposium 273, Physics of Sun and star spots, Ventura, California 22-26 August 2010

Scientific paper

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.

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