  We present a general overview and the first results of the SUMO project (a
SUrvey of Multiple pOpulations in Globular Clusters). The objective of this
survey is the study of multiple stellar populations in the largest sample of
globular clusters homogeneously analysed to date. To this aim we obtained high
signal-to-noise (S/N>50) photometry for main sequence stars with mass down to
~0.5 M_SUN in a large sample of clusters using both archival and proprietary U,
B, V, and I data from ground-based telescopes. In this paper, we focus on the
occurrence of multiple stellar populations in twenty three clusters. We have
defined a new photometric index cubi= (U-B)-(B-I), that turns out to be very
effective for identifying multiple sequences along the red giant branch (RGB).
We found that in the V-cubi diagram all clusters presented in this paper show
broadened or multimodal RGBs, with the presence of two or more components. We
found a direct connection with the chemical properties of different sequences,
that display different abundances of light elements (O, Na, C, N, and Al). The
cubi index is also a powerful tool to identify distinct sequences of stars
along the horizontal branch and, for the first time in the case of NGC104 (47
Tuc), along the asymptotic giant branch. Our results demonstrate that i) the
presence of more than two stellar populations is a common feature among
globular clusters, as already highlighted in previous work; ii) multiple
sequences with different chemical contents can be easily identified by using
standard Johnson photometry obtained with ground-based facilities; iii) in the
study of GC multiple stellar populations the cubi index is alternative to
spectroscopy, and has the advantage of larger statistics.
