Three‐dimensional X‐line spreading in asymmetric magnetic reconnection

Three-dimensional X-line spreading is important for the coupling between global dynamics and local kinetic physics of magnetic reconnection. Using large-scale 3-D particle-in-cell simulations, we investigate the spreading of the X-line out of the reconnection plane under a strong guide field in asymmetric reconnection. The X-line spreading speed depends strongly on the equilibrium current sheet thickness. In a simulation with a thick, ion-scale equilibrium current sheet (CS), the X-line spreads at the ambient species drift speeds, which are significantly lower than the Alfven speed based on the guide field V-Ag(sub-Alfvenic spreading). In simulations with a sub-ion-scale CS, the X-line spreads at V-Ag instead (Alfvenic spreading). An Alfvenic signal consistent with kinetic Alfven waves develops and propagates, leading to CS thinning and extending, which ultimately causes reconnection onset. The continuous onset of reconnection along the propagation direction of the signal manifests as Alfvenic X-line spreading. The strong dependence on the CS thickness of the spreading speeds and the orientation of the X-line are consistent with the collisionless tearing instability. Our simulations indicate that when the collisionless tearing growth is sufficiently strong in a thinner CS such that delta/Omega(cl) >= O(1), Alfvenic X-line spreading can effectively take place. Our results compare favorably with a number of numerical simulations and recent magnetopause observations. An important implication of this work is that the magnetopause CS is typically too thick for the X-line to spread at the Alfven speed.