The structure of magnetic reconnection-driven outflows and their dissipation are explored with large-scale, 3-D particle-in-cell (PIC) simulations. Outflow jets resulting from 3-D reconnection with a finite length x-line form fronts as they propagate into the downstream medium. A large pressure increase ahead of this ``reconnection jet front'' (RJF), due to reflected and transmitted ions, slows the front so that its velocity is well below the velocity of the ambient ions in the core of the jet. As a result, the RJF slows and diverts the high-speed flow into the direction perpendicular to the reconnection plane. The consequence is that the RJF acts as a thermalization site for the ion bulk flow and contributes significantly to the dissipation of magnetic energy during reconnection even though the outflow jet is subsonic. This behavior has no counterpart in 2-D reconnection. A simple analytic model predicts the front velocity and the fraction of the ion bulk flow energy that is dissipated.
Digital Commons Citation
Drake, J. F.; Swisdak, M.; Cassak, P. A.; and Phan, T. D., "On the 3-D structure and dissipation of reconnection-driven flow bursts" (2014). Faculty Scholarship. 263.
Drake, J. F., Swisdak, M., Cassak, P. A., & Phan, T. D. (2014). On The 3-D Structure And Dissipation Of Reconnection-Driven Flow Bursts. Geophysical Research Letters, 41(11), 3710-3716. http://doi.org/10.1002/2014GL060249