The HiSCORE Project

Authors

  • M. Tluczykont Institute for Experimental physics, University of Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany
  • M. Brückner Institute for Computer Science, Humboldt-University Berlin, Rudower Chaussee 25, 12489 Berlin, Germany
  • N. Budnev Institute of Applied Physics ISU, Irkutsk, Russia
  • O. Chvalaev Institute of Applied Physics ISU, Irkutsk, Russia
  • A. Dyachok Institute of Applied Physics ISU, Irkutsk, Russia
  • S. Epimakhov Institute for Experimental physics, University of Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany
  • O. Gress Institute of Applied Physics ISU, Irkutsk, Russia
  • D. Hampf Institute for Experimental physics, University of Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany
  • D. Horns Institute for Experimental physics, University of Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany
  • A. Ivanova Institute of Applied Physics ISU, Irkutsk, Russia
  • N. Kalmykov Skobeltsyn institute for Nuclear Physics, Lomonosov Moscow State University, 1 Leninskie gory, 119991 Moscow, Russia
  • E. Konstantinov Institute of Applied Physics ISU, Irkutsk, Russia
  • E. Korosteleva Skobeltsyn institute for Nuclear Physics, Lomonosov Moscow State University, 1 Leninskie gory, 119991 Moscow, Russia
  • V. Kozin Skobeltsyn institute for Nuclear Physics, Lomonosov Moscow State University, 1 Leninskie gory, 119991 Moscow, Russia
  • M. Kunnas Institute for Experimental physics, University of Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany
  • L. Kuzmichev Skobeltsyn institute for Nuclear Physics, Lomonosov Moscow State University, 1 Leninskie gory, 119991 Moscow, Russia
  • B. Lubsandorzhiev Institute for Nuclear Research of the Russian Academy of Sciences 60th October Anniversary st., 7a, 117312, Moscow, Russia
  • R. Mirgazov Institute of Applied Physics ISU, Irkutsk, Russia
  • R. Monkhoev Institute of Applied Physics ISU, Irkutsk, Russia
  • R. Nachtigall Institute for Experimental physics, University of Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany
  • M. Panasyuk Skobeltsyn institute for Nuclear Physics, Lomonosov Moscow State University, 1 Leninskie gory, 119991 Moscow, Russia
  • A. Pakhorukov Institute of Applied Physics ISU, Irkutsk, Russia
  • V. Poleschuk Institute of Applied Physics ISU, Irkutsk, Russia
  • A. Porelli DESY, Platanenallee 6, 15738 Zeuthen, Germany
  • V. Prosin Skobeltsyn institute for Nuclear Physics, Lomonosov Moscow State University, 1 Leninskie gory, 119991 Moscow, Russia
  • V. Ptuskin IZMIRAN, Moscow, Russia
  • G. I. Rubtsov Institute for Nuclear Research of the Russian Academy of Sciences 60th October Anniversary st., 7a, 117312, Moscow, Russia
  • P. S. Satunin Institute for Nuclear Research of the Russian Academy of Sciences 60th October Anniversary st., 7a, 117312, Moscow, Russia
  • Yu. Semeney Institute of Applied Physics ISU, Irkutsk, Russia
  • D. Spitschan Institute for Experimental physics, University of Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany
  • A. Skukhin Skobeltsyn institute for Nuclear Physics, Lomonosov Moscow State University, 1 Leninskie gory, 119991 Moscow, Russia
  • L. Sveshnikova Skobeltsyn institute for Nuclear Physics, Lomonosov Moscow State University, 1 Leninskie gory, 119991 Moscow, Russia
  • R. Wischnewski DESY, Platanenallee 6, 15738 Zeuthen, Germany
  • A. Zagorodnikov Institute of Applied Physics ISU, Irkutsk, Russia
  • V. Zirakashvili IZMIRAN, Moscow, Russia

DOI:

https://doi.org/10.14311/APP.2014.01.0283

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.

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Published

2014-12-04

How to Cite

Tluczykont, M., Brückner, M., Budnev, N., Chvalaev, O., Dyachok, A., Epimakhov, S., Gress, O., Hampf, D., Horns, D., Ivanova, A., Kalmykov, N., Konstantinov, E., Korosteleva, E., Kozin, V., Kunnas, M., Kuzmichev, L., Lubsandorzhiev, B., Mirgazov, R., Monkhoev, R., Nachtigall, R., Panasyuk, M., Pakhorukov, A., Poleschuk, V., Porelli, A., Prosin, V., Ptuskin, V., Rubtsov, G. I., Satunin, P. S., Semeney, Y., Spitschan, D., Skukhin, A., Sveshnikova, L., Wischnewski, R., Zagorodnikov, A., & Zirakashvili, V. (2014). The HiSCORE Project. Acta Polytechnica CTU Proceedings, 1(1), 283–287. https://doi.org/10.14311/APP.2014.01.0283

Issue

Vol. 1 No. 1 (2014): FRASCATI WORKSHOP 2013

Section

Articles