A new method to identify active reconnection in kinetic turbulent plasmas

Abstract:

Magnetic reconnection has been suggested to play an important role in the dynamics and energetics of plasma turbulence by spacecraft observations, numerical simulations and theory over the past two decades, and recently, by magnetosheath observations of MMS. A new method based on magnetic flux transport (MFT) has been developed to identify reconnection activity in kinetic turbulent plasmas. It is applied to a gyrokinetic simulation of two-dimensional plasma turbulence. Results on the identification of three active reconnection X-points are reported. The first two X-points have developed bi-directional electron outflow jets. The third X-point does not have bi-directional electron outflow jets because the flow is modified by turbulence. In all cases, this method successfully identifies active reconnection through clear inward and outward flux transport around the X-points. This transport pattern defines reconnection and produces a new quadrupolar structure in the divergence of MFT. This new method will be widely applicable to heliospheric plasmas from spacecraft missions such as MMS, Parker Solar Probe and Solar Orbiter.