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Diagnostics of the Solar Dynamo Using the Observed Pattern of Surface Magnetic Fields

Published online by Cambridge University Press:  12 April 2016

J.O. Stenflo
J.O. Stenflo*
Affiliation:
Institute of Astronomy, ETH-Zentrum, CH-8092 Zurich, Switzerland

Abstract

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The solar surface represents for the solar dynamo an outer boundary that is directly accessible to observations. The evolutionary and rotational properties of the magnetic fields at this boundary can be empirically determined using existing synoptic magnetograph data. The derived properties provide detailed constraints on the underlying theory, such that an inversion approach to the dynamo problem becomes feasible. Ambiguities in the interpretation may be removed using the independent constraints from helioseismology.

Type
Part III Solar magnetism and large-scale flows
Information
International Astronomical Union Colloquium , Volume 130: The Sun and Cool Stars: activity, magnetism, dynamos , 1991 , pp. 193 - 212
Copyright
Copyright © Springer-Verlag 1991

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