On the validity of quasi-linear kinematic mean-field electrodynamics in astrophysical flows
Mean-field theory in its kinematic form with the quasi-linear approximation is widely used for the modelling of the transport of weak magnetic fields in turbulent media. The validity of this approach to real astrophysical flows is discussed. Numerically evaluating the turbulent electromotive force using Lagrangian analysis for a set of simple
Petrovay, K. et al.
Fecha de publicación:
5
1998