Dynamo action and the sun

Issue		EAS Publications Series Volume 21, 2006 Stellar Fluid Dynamics and Numerical Simulations: From the Sun to Neutron Stars


Page(s)		241 - 273
DOI		10.1051/eas:2006116
Published online		07 June 2006

Stellar Fluid Dynamics and Numerical Simulations: From the Sun to Neutron Stars
M. Rieutord and B. Dubrulle (eds)
EAS Publications Series, 21 (2006) 241-273
DOI: 10.1051/eas:2006116

M. Proctor

DAMTP, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK

Abstract
Solar magnetic fields are produced by dynamo action in or just below the solar convection zone. After an account of observations of solar magnetic activity, the fundamentals of dynamo theory are reviewed, and the ideas applied to a discussion of different models of dynamo action in the Sun.

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