A theoretical model of torsional oscillations from a flux transport dynamo model
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🌌 astro-ph.SR
keywords
modelcycledynamofluxsunspottorsionaltransportassociated
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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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