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Existence and Energy Balance of the Solar Dynamo
Published online by Cambridge University Press: 19 July 2016
Abstract
The idea behind the use of ensemble averaging and the finite magnetic energy method of van Geffen and Hoyng (1992) is briefly discussed. Applying this method to the solar dynamo shows that the turbulence — an essential ingredient of traditional mean field dynamo theory — poses grave problems: the turbulence makes the magnetic field so unstable that it becomes impossible to recognize any period.
- Type
- 1. The Solar Dynamo
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- Copyright © Kluwer 1993