We have obtained $VI$ CCD photometry for the young globular clusters
Ruprecht 106, Terzan 7, and Arp 2 using the 0.9m and 1.5m telescopes
at Cerro Tololo Inter-American Observatory. The resulting $V\sim(V-I)$
color-magnitude diagrams extend from the tip of the red giant branch
to approximately 3 magnitudes below the horizontal branch. We have
applied the SRM method of Sarajedini (1994) to the RGBs of these
clusters in order to measure their reddenings and metallicities.
Furthermore, we have formulated the SRM method in the $V\sim(B-V)$
color-magnitude plane and applied it to published $BV$ photometry for
these young globular clusters.  The implications of these derived
parameters will be discussed.