Author/Authors :
Antokhonov، نويسنده , , B.V. and Beregnev، نويسنده , , S.F. and Budnev، نويسنده , , N.M. and Chvalaev، نويسنده , , O.B. and Chiavassa، نويسنده , , A. and Gress، نويسنده , , O.A. and Kalmykov، نويسنده , , N.N. and Karpov، نويسنده , , N.N. and Korosteleva، نويسنده , , E.E. and Kozhin، نويسنده , , V.A. and Kuzmichev، نويسنده , , L.A. and Lubsandorzhiev، نويسنده , , B.K. and Mirgazov، نويسنده , , R.R. and Panasy، نويسنده ,
Abstract :
The deployment of the new Extensive air shower Cherenkov installation Tunka-133 with about 1 km2 geometric acceptance area was completed in October 2009. The array will permit a detailed long-term study of the cosmic ray energy spectrum and mass composition in the energy range 1015–1018 eV with a unique and more elaborate method. The array construction and data acquisition system, preliminary results and plans for future development are presented.
Keywords :
Cosmic rays , Extensive Air Shower , Cherenkov light , Data acquisition system
