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Analytic Fast Dynamo Solution for a Two-dimensional Pulsed Flow

Published online by Cambridge University Press:  11 May 2010

M. R. E. Proctor
Affiliation:
University of Cambridge
P. C. Matthews
Affiliation:
University of Cambridge
A. M. Rucklidge
Affiliation:
University of Cambridge
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Summary

Recent results concerning the amplification of magnetic field frozen to a two-dimensional spatially periodic flow consisting of two distinct pulsed Beltrami waves are summarised. The period a of each pulse is long (α ≫ 1) so that fluid particles make excursions large compared to the periodicity length. The action of the flow is reduced to a map T of a complex vector field Z measuring the magnetic field at the end of each pulse. Attention is focused on the mean field (Z) produced. Under the assumption, (Tk+2Z) − |λ|2«TkZ) → 0 as K → ∈, an asymptotic representation of the complex constant λ is obtained, which determines the growth rate α1(α|λ|). The main result is the construction of a family of smooth vector fields ZN and complex constants λN with the properties (for even N), and for all integers K(> 0), where ∈ = α−3/2. The relation of ZN and λN to the modes of the corresponding dissipative problem with the fastest growth rates is discussed.

INTRODUCTION

The key characteristic of a fluid motion necessary for fast dynamo action is the existence of a positive Liapunov exponent. Childress (1992) calls a motion with this property a stretching flow and it is generally manifest by chaotic particle paths. For steady flows the regions of exponential stretching are often small, as they are, for example, in the case of the spatially periodic flows discussed by Dombre et al. (1986). The numerical demonstration of fast dynamos in such flows has proved difficult and Galloway & Frisch's (1984, 1986) results were inconclusive even at the largest values of the magnetic Reynolds number reached.

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Publisher: Cambridge University Press
Print publication year: 1994

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