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AMS02 experiment has collected data on Cosmic Rays for three years on the International Space Station, since its installation on May, 19 2011. The fluxes of electrons, positrons and protons, together with the results on Boron and Carbon ratio, will be discussed, as well as their implication in terms of Cosmic Ray propagation and in terms of limits on the existence of Dark Matter in the electroweak energy range. 7KLV LV DQ 2SHQ $FFHVV DUWLFOH GLVWULEXWHG XQGHU WKH WHUPV RI WKH &UHDWLYH &RPPRQVdoi:10.1051/epjconf/20159503017 fatcat:u4uwulm5rzfirf2n3pnat4rliy