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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

V.N. Krivodubskij
V.N. Krivodubskij*
Affiliation:
Kiev University Astronomical Observatory, Kiev 254053, Ukraine

Abstract

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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.

Keywords

Sun: magnetic fieldsdiamagnetismescape problem
Type
1. The Solar Dynamo
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993 , pp. 49 - 50
Copyright
Copyright © Kluwer 1993 

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