Table of Contents
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I. INTRODUCTION
This experiment was performed as a fluid flow
visualization of the flow field preliminary to a liquid sodium dynamo
experiment. This dynamo is presumed to be the analogue of an
astrophysical α - Ω dynamo. In an α - Ω dynamo
a differentially rotating conducting fluid wraps up an orthogonal
field line and after many turns produces a greatly amplified toroidal
field, the Ω-deformation. In astrophysical circumstances there
is negligible doubt concerning the occurrence of such differentially
rotating flows because of gravity and angular momentum, e.g. a
Keplerian accretion disk. However, the process of conversion of a
fraction of the toroidal field back into the original poloidal field,
i.e. the original orthogonal field line, is far more problematic.
This process is called the α-effect and requires a net
helicity. This paper is concerned with the laboratory demonstration
of a previously unrecognized, naturally occurring flow which produces
a large scale, coherent α-effect. The large scale is important
because of the magnitude of the flux affected. Coherence is important
because it implies a positive α-effect for each occurrence of
the flow so that averaging does not result in a null effect. This flow
is the partial rotation of an off-axis, axially-aligned, expanding
pulsed jet relative to its rotating frame. Although such a
differential rotation may be expected on the most elementary of
arguments, namely the conservation of angular momentum, a laboratory
demonstration is necessary for confidence in modeling of the dynamo as
well as the endeavor of attempting a dynamo experiment itself.
The structure of this paper is as follows. Section II discusses
previous experiments of convection in rotating frames, and the dynamo
flow field is discussed in relation to the experiment. Section III
describes the experimental apparatus and flow visualization methods
employed. Section IV presents the results of the experiment. The
conclusions reached from the experimental results follows in Sec. V.
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