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Non-Linear Diamagnetic Transport of the Large-Scale Magnetic Field in the Solar Convection Zone
Published online by Cambridge University Press: 19 July 2016
Abstract
The mean magnetic field transport due to inhomogeneity of the turbulence intensity is considered taking the field back reaction on motion into account. In spite of the magnetic quenching, the downward diamagnetic pumping is still powerful enough to keep the fields of 3 to 4 kG strength near the SCZ base against the magnetic buoyancy.
- Type
- 1. The Solar Dynamo
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- Copyright © Kluwer 1993