Magnetic turbulence and particle dynamics in the Earth's magnetotail

The influence of magnetic turbulence in the near-Earth magnetotail on ion motion is investigated by numerical simulation. The magnetotail current sheet is modelled as a magnetic field reversal with a normal magnetic field component B-n plus a three-dimensional spectrum of magnetic fluctuations BB which represents the observed magnetic turbulence. The dawn-dusk electric field E-y is also considered. A test particle simulation is performed using different values of B, and of the fluctuation level deltaB/B-0. We show that when the magnetic fluctuations are taken into account, the particle dynamics is deeply affected, giving rise to an increase in the cross tail transport, ion heating, and current sheet thickness. For strong enough turbulence, the current splits in two layers, in agreement with recent Cluster observations.