Two-dimensional compressible magnetohydrodynamic simulations of the co
alescence instability in a low-beta plasma are presented in which anom
alous resistivity is permitted to occur. The instability is considered
in a uniform current sheet configuration, initially perturbed by an i
nfinite chain of spots of anomalous resistivity. The two phases of the
instability known from simulations based on the Fadeev equilibrium -
ideal and resistive - can clearly be distinguished also in this config
uration. It is found that the conversion of magnetic energy into kinet
ic energy dominates Ohmic heating. The main energy release occurs with
in a few Alfven transit times. The scaling of several key parameters i
n the current layer formed between the coalescing islands is compared
to the scalings obtained with uniform resistivity. The numerical resul
ts indicate that the peak reconnection rate decreases toward large Lun
dquist numbers (S much greater than 10(4)) as S-a with a = 1/5 - 1/3 a
nd that a transition to slow reconnection (a similar to 1/2) may occur
at S greater than or similar to 10(7), where S is based on the backgr
ound resistivity. (C) 1997 American Institute of Physics.