Satellite data-based 3D simulation of Kelvin-Helmholtz instability and induced magnetic reconnection at the Earth's magnetopause

We present a 3D two-fluid simulation using plasma parameters as measured by MMS on September 8th 2015 concerning the nonlinear development of the Kelvin-Helmholtz instability at the Earth's magnetopause. We observe an extremely rich nonlinear dynamics including the development of a complex magnetic topology, vortex merging and secondary KH instability driven by large-scale vortices distributed asymmetrically in latitude. Vortex induced and mid-latitude magnetic reconnection coexist and produce an asymmetric distribution of magnetic reconnection events. These results are in good agreement with MMS observations on the same day, in particular for the presence of both equatorial and o-equator reconnection. Regarding the latter only we note a predominance of reconnection in the southern hemisphere during the early nonlinear phase. The estimated eective diusion coecient associated to the dynamics is found to be large enough to account for the observed mass transport at the Earth's magnetospheric flanks.