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The results of simulation showing the possibility of mass analysis of primary cosmic-ray particles in the energy range 1016–1018 eV with the use of the SPHERE-2 balloon system are reported. The system is lifted by a tethered balloon at an altitude of 1 km. It has almost continuous sensitivity at an area of about 1 km2 that is viewed by 109 photoelectron multipliers. This property makes it possible...
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