The ideal initial value problem for the neutral sheet is considered, w
ith the emphasis on fieldwise-independent, infinitesimal velocity dist
urbances. It is shown analytically that cross-field velocity perturbat
ions persist, and that they also set up fieldwise magnetic disturbance
s that grow algebraically in time. When these disturbances attain fini
te amplitude they should distort the neutral sheet configuration, and
hence they could provide an alternative route by which magnetic reconn
ection can become turbulent. Some supporting numerical simulations, pe
rformed at large Lundquist numbers, are then described. In an Appendix
the analysis is extended to include fieldwise-dependent disturbances.