Dynamical Quenching of the $α^2$ Dynamo

Abstract

We present a two-scale approximation for the dynamics of a nonlinear $α^2$ dynamo. Solutions of the resulting nonlinear equations agree with the numerical simulations of Brandenburg (2001), and show that $α$ is quenched by the buildup of magnetic helicity at the forcing scale $1/k_2$ as the $α$ effect transfers it from the large scale $1/k_1$. For times $t > (k_1/k_2)R_{M,2}$ in eddy turnover units (where $R_{M,2}$ is the magnetic Reynolds number of the forcing scale), $α$ is resistively limited in the form predicted for the steady-state case. However, for $t << R_{M,2}$, $α$ takes on its kinematic value, independent of $R_{M,2}$, allowing the production of large-scale magnetic energy equal to $k_1/k_2$ times equipartition. Thus the dynamic theory of $α$ predicts substantial "fast" growth of large-scale field despite being "slow" at large times.