Kinematic α-effect in isotropic turbulence simulations

Using numerical simulations at moderate magnetic Reynolds numbers up to 220, it is shown that in the kinematic regime, isotropic helical turbulence leads to an α-effect and a turbulent diffusivity whose values are independent of the magnetic Reynolds number, R<SUB>m</SUB>, provided R<SUB>m</SUB> exceeds unity. These turbulent coefficients are also consistent with expectations from the first-order smoothing approximation. For small values of R<SUB>m</SUB>, α and turbulent diffusivity are proportional to R<SUB>m</SUB>. Over finite time-intervals, meaningful values of α and turbulent diffusivity can be obtained even when there is small-scale dynamo action that produces strong magnetic fluctuations. This suggests that the fields generated by the small-scale dynamo do not make a correlated contribution to the mean electromotive force