  We present radial velocities and chemical abundances for red giant branch
stars in the Galactic bulge globular clusters NGC 6342 and NGC 6366. The
velocities and abundances are based on measurements of high resolution (R >
20,000) spectra obtained with the MMT-Hectochelle and WIYN-Hydra spectrographs.
We find that NGC 6342 has a heliocentric radial velocity of +112.5 km/s (sigma
= 8.6 km/s), NGC 6366 has a heliocentric radial velocity of -122.3 km/s (sigma
= 1.5 km/s), and that both clusters have nearly identical metallicities ([Fe/H]
~ -0.55). NGC 6366 shows evidence of a moderately extended O-Na
anti-correlation, but more data are needed for NGC 6342 to determine if this
cluster also exhibits the typical O-Na relation likely found in all other
Galactic globular clusters. The two clusters are distinguished from similar
metallicity field stars as having larger [Na/Fe] spreads and enhanced [La/Fe]
ratios, but we find that NGC 6342 and NGC 6366 display alpha and Fe-peak
element abundance patterns that are typical of other metal-rich ([Fe/H] > -1)
inner Galaxy clusters. However, the median [La/Fe] abundance may vary from
cluster-to-cluster.
