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We present the preliminary results of analysis of the mean light curves of dwarf nova SS Cyg. UBV-light curves were derived from the numerous observations during the period 1982-1995 (more than 2000 measurements). All observations were performed with UBV-photometer on the 60cm telescope of Sternberg Astronomical Crimean Station at quiescence. The relative contribution of different components of the system in the total luminosity was evaluated and some important parameters determined.