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Abstract

We show that the magnetic analogue of the Rädler effect of mean-field dynamo theory leads to a non-linear backreaction that quenches a large-scale galactic dynamo, and can result in saturation of the large-scale magnetic field at near-equipartition with turbulent kinetic energy density. In a rotating fluid containing small-scale magnetic fluctuations, anisotropic terms in the mean electromotive force are induced via the Coriolis effect and these terms lead to a reduction of the growth rate in a predominantly αΩ-type galactic dynamo. By including the generation of small-scale magnetic fluctuations by turbulent tangling of the large-scale magnetic field, one obtains a negative feedback effect that quenches the dynamo and leads to the saturation of the large-scale field. This saturation mechanism is found to be competitive with the dynamical α-quenching mechanism for realistic galactic parameter values. Furthermore, in the context of the dynamical α-quenching model, a separate non-linear term is obtained which has the same form as the helicity flux term of Vishniac & Cho, but which depends on the strength of small-scale magnetic fluctuations. We briefly discuss the observational implications of the magnetic Rädler effect for galaxies.