We investigate the possibility of using globular clusters as targets f
or microlensing searches. Such searches will be challenging and requir
e more powerful telescopes than now employed, but are feasible in the
near future. Although expected event rates are low, we show that the w
ide variety of lines of sight to globular clusters greatly enhances th
e ability to distinguish between halo models using microlensing observ
ations as compared with LMC/SMC observations alone, In particular, the
halo core radius and power-law exponent can be determined with good a
ccuracy.