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Activity Cycle in the Solar Core

Published online by Cambridge University Press:  12 April 2016

Attila Grandpierre
Attila Grandpierre*
Affiliation:
Konkoly Observatory, 1525 Budapest, P.O. Box 67, Hungary

Abstract

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I analyze here the recent solar seismology data relevant to the core regarding the energetics. The result is that the magnetic torsional oscillations are hardly able to support the observed rate of change of the solar core rotation. Interpreting the solar neutrino data as directly coming from the core and showing the activity cycle of the core, the energetics of the core can be balanced. I show here a simple model for the global and local activity-related changes of the solar core. The parameters of this model are consistent with the values derived by the Convective Flare Theory. This model is able to interpret the anticorrelation of the sunspot number with the neutrino flux, the related changes in the rotation of the core and the first which interprets the observed activity-related element abundance anomalies with a model for the solar core.

Type
I. Setting the stage: Sun, Stars Galaxies and the Universe
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 75 - 77
Copyright
Copyright © Astronomical Society of the Pacific 1993

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