The study of primary cosmic rays energy spectrum and mass composition in the energy range 0.5-50PeV with TUNKA Eas Cherenkov array

Details The study of primary cosmic rays energy spectrum and mass composition in the energy range 0.5-50PeV with TUNKA Eas Cherenkov array The study of primary cosmic rays energy spectrum and mass composition in the energy range 0.5-50PeV with TUNKA Eas Cherenkov array

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999nuphs..75..299g&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 75, Issue 1-2, p. 299-301.

Physics

Nuclear Physics

14

Scientific paper

The Tunka-13 EAS array has operated two winter seasons since 1996 until 1998 years. It consists of 13 Cherenkov light detectors based upon the QUASAR-370 phototubes. The array covers the area 240x240m2 and measures the primary energy, derived from Cherenkov light flux, and individual lateral distribution functions (LDF). Good energy and angular resolution of the array permits to study the irregularities in energy spectrum following the classic ``knee''.

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