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We present an event-by-event study of cosmic ray (CR) composition with thereflected Cherenkov light method. The fraction of CR light component above 5PeV was reconstructed using the 2013 run data of the SPHERE experiment whichobserved optical Vavilov-Cherenkov radiation of extensive air showers,reflected from snow surface of Lake Baikal. Additionally, we discuss apossibility to improve the elemental groups separability by means ofmultidimensional criteria.

Event-by-event study of CR composition with the SPHERE experiment using the 2013 data