We study three-dimensional magnetic reconnection caused by the Kelvin-Helmh
oltz (KH) instability and differential rotation in subsonic and sub-Alfveni
c flows. The flows, which are modeled by the resistive magnetohydrodynamic
equations with constant resistivity, are stable in the direction of the mag
netic field but unstable perpendicular to the magnetic field. Localized tra
nsient reconnection is observed on the KH time scale, and kinetic energy in
creases with decreasing resistivity. As in flux-transfer events in the Eart
h's magnetopause boundary layer, bipolar structures in the normal flux and
bidirectional jetting away from reconnection zones are observed.