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On the Nonlinear Nature of the Turbulent α-Effect
Published online by Cambridge University Press: 30 March 2016
Abstract
Galactic magnetic fields are, typically, modelled by mean-field dynamos involving the α-effect. Here we consider, very briefly, some of the issues involving the nonlinear dependence of α on the mean field.
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- II. Joint Discussions
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- Copyright © Astronomical Society of Pacific 2002