Asymmetry effects driving secondary instabilities in two-dimensional collisionless magnetic reconnection

In the framework of the studies on magnetic reconnection, much interest has been recently devoted to asymmetric magnetic configurations,which can naturally be found in solar and astrophysical environments and in laboratory plasmas. Several aspects of this problem have beeninvestigated, mainly in a two-dimensional geometry and by means of particle-in-cell (PIC) simulations. Still, there are open questions concerningthe onset and the effects of secondary instabilities in the nonlinear phase of an asymmetric reconnection process. In this work, wefocus on the conditions that lead to the appearance of the Kelvin-Helmholtz instability following an asymmetric reconnection event in a collisionlessplasma. This investigation is carried out by means of two-dimensional numerical simulations based on a reduced fluid modelassuming a strong guide field. We show that, unlike the symmetric case, in the presence of asymmetry, a Kelvin-Helmholtz-like instabilitycan develop also for a finite equilibrium electron temperature. In particular, simulations indicate the formation of steep velocity gradients,which drive the instability, when the resonant surface of the equilibrium magnetic field is located sufficiently far from the peak of the equilibriumcurrent density. Moreover, a qualitative analysis of the vorticity dynamics shows that the turbulent behavior induced by the secondaryinstability not only is confined inside the island but can also affect the plasma outside the separatrices. The comparison between simulationscarried out with an adiabatic closure and a Landau-fluid closure for the electron fluid indicates that the latter inhibits the secondary instabilityby smoothing velocity gradients.