Hybrid simulations with electron inertia, along with analytic scaling argum
ents, are presented which demonstrate that magnetic reconnection remains Al
fvenic in a collisionless system even as the macroscopic scale length of th
e system becomes very large. This fast reconnection is facilitated by the w
histler physics present near the x-line. The reconnection rate is found to
be a universal constant corresponding to an inflow velocity towards the x-l
ine of around 0.1 c(A).