High Energy Cosmic Rays

Main Goals is to determine energy spectrum and mass composition of primary cosmic radiation at energy range1014-1017  eV, to estimate diffuse fluxes of very high energy primary gamma-quanta, to search for gamma-quanta   local sources.
Acting Head of group        Martirosov Roman

S. Garyaka Alexander
Sokhoyan Sergey Babayan Hovhanes
Djabaryan Gurgen Asatryan Karen