  The structure of dipolarization jets with finite width in the dawn-dusk
direction relevant to magnetic reconnection in the Earth's magnetotail is
explored with particle-in-cell simulations. We carry out Riemann simulations of
the evolution of the jet in the dawn-dusk, north-south plane to investigate the
dependence of the jet structure on the jet width in the dawn-dusk direction. We
find that the magnetic field and Earth-directed ion flow structure depend on
the dawn-dusk width. A reversal in the usual Hall magnetic field near the
center of the current sheet on the dusk side of larger jets is observed. For
small widths, the maximum velocity of the Earthward flow is significantly
reduced below the theoretical limit of the upstream Alfv\'en speed. However,
the ion flow speed approaches this limit once the width exceeds the ion Larmor
radius based on the normal magnetic field, $B_z$.
