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

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arxiv 0902.3156 v1 pith:Q22JTEAK submitted 2009-02-18 astro-ph.HE

N. M. Budnev , O. A. Chvalaiev , O. A. Gress , N. N. Kalmykov , V. A. Kozhin , E. E. Korosteleva , L. A. Kuzmichev , B. K. Lubsandorzhiev
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R. R. Mirgazov G. Navarra M. I. Panasyuk L. V. Pankov V. V. Prosin V. S. Ptuskin Yu. A. Semeney B. A. Shaibonov-junior A. A. Silaev A. A. Silaev-junior A. V. Skurikhin C. Spiering R. Wischnewski I. V. Yashin A. V. Zablotsky A. V. Zagorodnikov
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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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