  We derive [Cu/Fe] for 117 giant stars in ten globular clusters (M3, M4, M5,
M10, M13, M15, M71, NGC 7006, NCG 288, and NGC 362) and find that globular
cluster Cu abundances appear to follow [Cu/Fe] trends found in the field. This
result is interesting in light of recent work which indicates that the globular
cluster Omega Centauri shows no trend in [Cu/Fe] with [Fe/H] over the abundance
range -2.0 <[Fe/H]< -0.8. Of particular interest are the two clusters M4 and
M5. While at a similar metallicity ([Fe/H] ~- 1.2), they differ greatly in some
elemental abundances: M4 is largely overabundant in Si, Ba, and La compared to
M5. We find that it is also overabundant in Cu with respect to M5, though this
overabundance is in accord with [Cu/Fe] ratios found in the field.
