Two-dimensional compressible magnetohydrodynamic simulations of curren
t sheet dynamics under the influence of localized anomalous resistivit
y are presented. The system is initially perturbed by several spots of
anomalous resistivity distributed in the sheet. Following a phase of
induced tearing resulting from the initial perturbation, magnetic isla
nd coalescence occurs until one island persists. Finally the evolution
becomes eruptive, dominated by the acceleration and ejection of a pla
smoid, as a consequence of the amplification of a small initial asymme
try after a few 10(2) Alfven times. These processes are accompanied by
strong enhancements of the current density. It exceeds the threshold
of kinetic instability repeatedly and leads to recurrence of anomalous
resistivity, which drives the evolution. Jets are formed, driven by h
eld line reconnection and locally enhanced dissipation at dominant X-p
oints. The conversion of magnetic energy into kinetic energy is most e
fficient during the acceleration phase of the plasmoid. The evolution
becomes more impulsive and leads to stronger current density enhanceme
nts for higher Lundquist numbers. (C) 1996 American Institute of Physi
cs.