Large-scale dynamo produced by negative magnetic eddy diffusivities.

Lanotte, A., Noullez, A., Vergassola, M. and Wirth, A. (1999) Large-scale dynamo produced by negative magnetic eddy diffusivities. Geophysical and Astrophysical Fluid Dynamics (91). pp. 131-146. DOI 10.1080/03091929908203701.

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Abstract

The existence of incompressible flow producing negative magnetic eddy diffusivities is demonstrated. This provides for a dynamo mechanism, alternative to α-type effects, requiring neither the presence of mean heliciiy nor the breaking of parity invariance. In the kinematic dynamo phase, the magnetic field grows exponentially with a growth rate proportional to the square of the wavenumber. The concrete example, analyzed by means of multiscale techniques, is a parity-invariant flow of the Taylor-Green type.

Document Type: Article
Keywords: Dynamo processes, Stability, turbulent diffusion
Research affiliation: OceanRep > Institute for Marine Science Kiel
Refereed: Yes
Open Access Journal?: No
Publisher: Gordon and Breach
Date Deposited: 18 Feb 2008 17:24
Last Modified: 28 Sep 2017 08:48
URI: https://oceanrep.geomar.de/id/eprint/4271

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