  A transport-like framework for the study of magnetic reconnection mediated by
self-driven turbulence is proposed, based on timescale separation between the
reconnection time and the characteristic timescale of the turbulent
fluctuations which arise in the reconnection layer. We argue that the mean
fields remain on MHD scales even in collisionless cases. These observations
provide theoretical justification for an efficient computational approach to
this problem, which we discuss.
