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A&A 393, 339-343 (2002)
DOI: 10.1051/0004-6361:20021007
A Taylor-Couette dynamo
A. P. Willis and C. F. BarenghiDepartment of Mathematics, University of Newcastle, Newcastle upon Tyne, NE2 7RU, UK
(Received 19 April 2002 / Accepted 8 July 2002)
Abstract
Recent experiments have shown that it is possible to study
a fundamental astrophysical process such as dynamo action in
controlled laboratory conditions using simple MHD flows.
In this paper we explore the possibility that Taylor-Couette flow,
already proposed as a model of the magneto-rotational instability of
accretion discs, can sustain generation of a magnetic field. Firstly, by
solving the kinematic dynamo problem, we identify the region of
parameter space where the magnetic field's growth rate is higher.
Secondly, by solving simultaneously the coupled nonlinear equations
which govern velocity field and magnetic field, we find a
self-consistent nonlinearly saturated dynamo.
Key words: instabilities -- MHD
Offprint request: C. F. Barenghi, c.f.barenghi@newcastle.ac.uk
© ESO 2002
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