  We investigate the possibility of using globular clusters as targets for
microlensing searches. Such searches will be challenging and require more
powerful telescopes than now employed, but are feasible in the 0 future.
Although expected event rates are low, we show that the wide variety of lines
of sight to globular clusters greatly enhances the ability to distinguish
between halo models using microlensing observations as compared to LMC/SMC
observations alone.
