THE TUNKA EXPERIMENT: TOWARDS A 1-KM2 CHERENKOV EAS ARRAY IN THE TUNKA VALLEY-Reference-Cited by-同舟云学术

THE TUNKA EXPERIMENT: TOWARDS A 1-KM2 CHERENKOV EAS ARRAY IN THE TUNKA VALLEY

Published:2005-11-20 Issue:29 Volume:20 Page:6796-6798
ISSN:0217-751X
Container-title:International Journal of Modern Physics A
language:en
Short-container-title:Int. J. Mod. Phys. A

Author:

CHERNOV D. V.¹,KALMYKOV N. N.¹,KOROSTELEVA E. E.¹,KUZMICHEV L. A.¹,PROSIN V. V.¹,PANASYUK M. I.¹,SHIROKOV A. V.¹,YASHIN I. V.¹,BUDNEV N. M.²,GRESS O. A.²,PANKOV L. V.²,PARFENOV YU. V.²,SEMENEY YU. A.²,LUBSANDORZHIEV B. K.³,POKHIL P. G.³,PTUSKIN V. S.⁴,SPIERING CH.⁵,WISCHNEWSKI R.⁵,NAVARRA G.⁶

Affiliation:

1. Skobeltsyn Institute of Nuclear Physics of Moscow State University, Moscow, RU-119234, Russia

2. Institute of Applied Physics of Irkutsk State University, Irkutsk, RU-664003, Russia

3. Institute for Nuclear Research of Russian Academy of Sciences, Moscow, RU-117312, Russia

4. Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation of Russian Academy of Sciences (IZMIRAN), Troitsk, Moscow Region, 142092, Russia

5. Deutsches Elektronen Synchrotron (DESY), Zeuthen, D-15738, Germany

6. Dipartimento di Fisica Generale Universitá di Torino and INFN, Torino, I-10125, Italy

Abstract

The project of an EAS Cherenkov array in the Tunka Valley/Siberia with an area of about 1 km2 is presented. The new array will have a ten times bigger area than the existing TUNKA-25 array and will permit a detailed study of the cosmic ray energy spectrum and the mass composition in the energy range from 1015 to 1018 eV.

Publisher

World Scientific Pub Co Pte Lt

Subject

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

Link

https://www.worldscientific.com/doi/pdf/10.1142/S0217751X05030119

Reference3 articles.

1. Limits on diffusive shock acceleration in supernova remnants in the presence of cosmic-ray streaming instability and wave dissipation

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

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