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The HiSCORE Project

Authors :
M. Brückner
Martin Tluczykont
L. G. Sveshnikova
Petr Satunin
S. Epimakhov
Grigory Rubtsov
N. N. Kalmykov
A. L. Pakhorukov
Bayarto Lubsandorzhiev
E. E. Korosteleva
V. S. Ptuskin
V. Kozin
V. V. Prosin
V. Zirakashvili
R. D. Monkhoev
V. A. Poleschuk
M. Kunnas
R. R. Mirgazov
A. N. Dyachok
Mikhail Panasyuk
O. A. Gress
Yu. Semeney
E. N. Konstantinov
A. Skukhin
N. M. Budnev
D. Hampf
Aleksey Zagorodnikov
A. Ivanova
O. Chvalaev
A. Porelli
D. Spitschan
R. Nachtigall
Dieter Horns
Ralf Wischnewski
L. A. Kuzmichev
Source :
Acta Polytechnica CTU Proceedings, Vol 1, Iss 1, Pp 283-287 (2014)
Publication Year :
2014
Publisher :
Czech Technical University in Prague - Central Library, 2014.

Abstract

A central question of Astroparticle Physics, the origin of cosmic rays, still remains unsolved. HiSCORE (Hundred*i Square-km Cosmic ORigin Explorer) is a concept for a large-area wide-angle non-imaging air shower detector, addressing this question by searching for cosmic ray pevatrons in the energy range from 10TeV to few PeV and cosmic rays in the energy range above 100TeV. In the framework of the Tunka-HiSCORE project, first prototypes have been deployed on the site of the Tunka-133 experiment, where we plan to install an engineering array covering an area of the order of 1km2. On the same site, also imaging and particle detectors are planned, potentially allowing a future hybrid detector system. Here we present the HiSCORE detector principle, its potential for cosmic ray origin search and the status of ongoing activities in the framework of the Tunka-HiSCORE experiment.

Details

ISSN :
23365382
Volume :
1
Database :
OpenAIRE
Journal :
Acta Polytechnica CTU Proceedings
Accession number :
edsair.doi.dedup.....8f0dfb63049b60f76877a5f2c60f7beb
Full Text :
https://doi.org/10.14311/app.2014.01.0283