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Turbulent Cascades and the alpha Dynamo

2012/10/13 by J. B. Taylor, Taylor, J B
Biochemistry, Genetics and Molecular Biology · Physics and Astronomy · #Astro and Planetary Science #Earth and Planetary Astrophysics (astro-ph.EP) #FOS: Physical sciences #Fluid Dynamics (physics.flu-dyn) #Geomagnetism and Paleomagnetism Studies #Plasma Physics (physics.plasm-ph) #Solar and Space Plasma Dynamics

paper · pdf · doi:10.48550/arxiv.1210.3714

openalex publication_date 2012/10/13 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

The well known mean-field model of a turbulence driven dynamo is reviewed in relation to Laboratory experiments in which a turbulent cascade is created by a pair of large rotors. It is argued that in such experiments the alpha-effect, driving a dynamo field, will be much less than the dissipative beta-effect. Consequently a mean field dynamo cannot be sustained. This conclusion is supported by recent measurements of the alpha and beta effects in the Madison Dynamo Experiment.

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