STRUCTURE OF THE DISSIPATION REGION DURING MAGNETIC RECONNECTION IN COLLISIONLESS PLASMA

The results of an analytic and numerical investigation of the structure of the X line during steady state magnetic reconnection in collisionless plasma are presented. The structure of the X line essentially depends on a single dimensionless parameter F, which is a measure of the influx of plasma into the reconnection region. For small F the self-consistent plasma current driven at the X line is small, and the magnetic fields are nearly unchanged from the initial vacuum state. With increasing F the current driven at the X line becomes large, and the dissipation region collapses in the direction of the inflow and elongates along the outflow. For sufficiently large F the velocity of the plasma ejected from the X line exceeds the local Alfven velocity. In this regime a fast mode shock forms at the outflow end of the dissipation region which slows the high-velocity outflow plasma to the subsonic flow characteristic of the broader outflow region. Finally, at a critical plasma flux F(c) the dissipation region collapses to zero thickness; no steady solutions are found for F > F(c). By matching the energy dissipated at the neutral line with the change in global magnetic energy, a self-consistent equation for F is derived which indicates that F always adjusts so that F similar-to-or-less-than F(c). Predictions of reconnection rates and associated parameters for the geomagnetic tail are presented which are in reasonable agreement with observations.