Abstract
The final analysis of the Extensive Air Shower (EAS) maximum ( X m a x ) depth distribution derived from the data of Tunka-25 atmospheric Cherenkov light array in the energy range 3 ⋅ 10 15 – 3 ⋅ 10 16 eV is presented. The perspectives of X m a x studies with the new Cherenkov light array Tunka-133 of 1 km 2 area, extending the measurements up to 10 18 eV, are discussed.
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