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Magnetic Field and Differential Rotation of the Sun

Published online by Cambridge University Press:  19 July 2016

W. Kundt
W. Kundt*
Affiliation:
Institut für Astrophysik, Univ. Bonn, D-5300 Bonn 1

Abstract

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The solar magnetized surface reveals a stable spin period — the Carrington period — and a stable oscillation period — the Hale period. The latter is traced by each of the low-order multipole moments, whereby the total magnetic energy (near the surface) is more or less constant. This highly non-stochastic structure is reminiscent of a permanent magnetic flux frozen into the Sun's radiative core, and dragged out into the heliosphere by the solar wind. The radius-dependent torque exerted by this magnetic flux can restore the observed system of torsional oscillations of the convection zone.

Type
2. Long-Term Variability of the Solar Magnetic Cycle
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993 , pp. 77 - 82
Copyright
Copyright © Kluwer 1993 

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