The Cosmic Ray Mass Composition in the Energy Range 1015 - 1018 eV measured with the Tunka Array: Results and Perspectives
Abstract
The final analysis of the Extensive Air Shower (EAS) maximum Xmax depth distribution derived from the data of Tunka-25 atmospheric Cherenkov light array in the energy range 3.1015 - 3.1016 eV is presented. The perspectives of Xmax studies with the new Cherenkov light array Tunka-133 of 1 km2 area, extending the measurements up to 1018 eV, are discussed.
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