Dynamos in weakly chaotic two-dimensional flows
- 19 August 1995
- journal article
- research article
- Published by Taylor & Francis in Geophysical & Astrophysical Fluid Dynamics
- Vol. 79 (1-4) , 239-257
- https://doi.org/10.1080/03091929508228999
Abstract
The dynamo action of a time-periodic two-dimensional flow close to integrability is analyzed. At fixed Reynolds number R M and frequency ω, magnetic structures develop in the form of both eddies and filaments. The growth rate of the eddies appears to be the same for all frequencies and decreases with R M, while the growth rate of the filaments displays a strong co-dependence and, except in the limit of zero or infinite frequencies, converges to a non-zero value as R M → ∞. Magnetic filaments develop in the widest chaotic zones located near the homoclinic or heteroclinic tangles, and their growth rate is strongly influenced by the width of these zones which is estimated using Melnikov formalism. This study illustrates quantitatively that not only a local stretching but also a sizable chaotic zone is required for fast dynamo action.Keywords
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