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

  • Published:1999-03 Issue:1-2 Volume:75 Page:299-301
  • ISSN:0920-5632
  • Container-title:Nuclear Physics B - Proceedings Supplements
  • language:en
  • Short-container-title:Nuclear Physics B - Proceedings Supplements

Author:

Gress O.A.,Gress T.I.,Korosteleva E.E.,Kuzmichev L.A.,Lubsandorzhiev B.K.,Pan'kov L.V.,Parfenov Yu. V.,Pohil P.G.,Prosin V.V.,Semeney Yu. A.

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

Reference5 articles.

1. O.A.Gress et al.,Proc. 25th ICRC, Durban, 4 129

2. High energy cosmic ray spectroscopy. I. status and prospects

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1. The energy spectrum of cosmic rays beyond the turn-down around $$\varvec{10^{17}}$$ eV as measured with the surface detector of the Pierre Auger Observatory;The European Physical Journal C;2021-11

2. Tunka Advanced Instrument for cosmic rays and Gamma Astronomy;Journal of Physics: Conference Series;2019-06-01

3. Study of Cherenkov light lateral distribution function around the knee region in extensive air showers;Serbian Astronomical Journal;2015

4. A new 1km2 EAS Cherenkov array in the Tunka Valley;Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment;2011-05

5. Muon production height studies with the air shower experiment KASCADE-Grande;Astroparticle Physics;2011-01
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