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Locating the Seat of the Solar Dynamo

Published online by Cambridge University Press:  19 July 2016

Arnab Rai Choudhuri
Arnab Rai Choudhuri*
Affiliation:
Department of Physics Indian Institute of Science Bangalore 560012. India

Abstract

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By analyzing the hypothesis that the solar dynamo operates in a thin layer at the bottom of the convection zone, we conclude that this hypothesis can fit observational facts only if there is turbulence with the length scale of a few hundred kilometers in and around the dynamo region.

Type
II. The Solar Interior
Information
Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 51 - 55
Copyright
Copyright © Kluwer 1990 

References

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