Dynamo action is demonstrated numerically in the forced Taylor-Green (
TG) vortex made up of a confined swirling flow composed of a shear lay
er between two counter-rotating eddies, corresponding to a standard ex
perimental setup in the study of turbulence. The critical magnetic Rey
nolds number above which the dynamo sets in depends crucially on the f
undamental symmetries of the TG vortex. These symmetries can be broken
by introducing a scale separation in the how, or by letting develop a
small non-symmetric perturbation which can be either kinetic and magn
etic, or only magnetic. The nature of the boundary conditions for the
magnetic field (either conducting or insulating) is essential in selec
ting the fastest growing mode; implications of these results to a plan
ned laboratory experiment are briefly discussed. (C) 1997 American Ins
titute of Physics.