The Cosmic Ray Mass Composition in the Energy Range 10^15 - 10^18 eV measured with the Tunka Array: Results and Perspectives

Details The Cosmic Ray Mass Composition in the Energy Range 10^15 - 10^18 eV measured with the Tunka Array: Results and Perspectives The Cosmic Ray Mass Composition in the Energy Range 10^15 - 10^18 eV measured with the Tunka Array: Results and Perspectives

2009-02-18

arxiv.org/abs/0902.3156v1

Nucl.Phys.Proc.Suppl.190:247-252,2009

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

6 pages, 7 figures, Proceedings of CRIS 2008 - Cosmic Ray International Seminar - Malfa, Salina Island, Eolian Islands, Italy,

Scientific paper

10.1016/j.nuclphysbps.2009.03.09

The final analysis of the Extensive Air Shower (EAS) maximum X_max 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_max 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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