Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype

Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype

Data obtained with two detectors located at the Tunka Cosmic Ray facility are presented. The Cherenkov light array for registration of extensive air showers (EAS) Tunka-133 collected data during 5 winter seasons since 2009 to 2014. The differential energy spectrum of all particles and the dependence...

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Main Authors: Prosin V.V., Berezhnev S.F., Budnev N.M., Brückner M., Chiavassa A., Chvalaev O.A., Dyachok A.V., Epimakhov S.N., Gafarov A.V., Gress O.A., Gress T.I., Horns D., Kalmykov N.N., Karpov N.I., Kiryuhin S.N., Konstantinov E.N., Korobchenko A.V., Korosteleva E.E., Kozhin V.A., Kunnas M., Kuzmichev L.A., Lubsandorzhiev B.K., Lubsandorzhiev N.B., Mirgazov R.R., Monkhoev R.D., Nachtigall R., Osipova E.A., Pakhorukov A.L., Panasyuk M.I., Pankov L.V., Poleschuk V.A., Popova E.G., Porelli A., Ptuskin V.S., Rubtsov G.I., Rüger M., Samoliga V.S., Semeney Y.A., Silaev A.A., Skurikhin A.V., Spiering C., Sveshnikova L.G., Tluczykont M., Wischnewski R., Zagorodnikov A.V., Zurbanov A.V.
Format: Article
Language:English
Published: EDP Sciences 2016-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/201612103004
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author Prosin V.V.
Berezhnev S.F.
Budnev N.M.
Brückner M.
Chiavassa A.
Chvalaev O.A.
Dyachok A.V.
Epimakhov S.N.
Gafarov A.V.
Gress O.A.
Gress T.I.
Horns D.
Kalmykov N.N.
Karpov N.I.
Kiryuhin S.N.
Konstantinov E.N.
Korobchenko A.V.
Korosteleva E.E.
Kozhin V.A.
Kunnas M.
Kuzmichev L.A.
Lubsandorzhiev B.K.
Lubsandorzhiev N.B.
Mirgazov R.R.
Monkhoev R.D.
Nachtigall R.
Osipova E.A.
Pakhorukov A.L.
Panasyuk M.I.
Pankov L.V.
Poleschuk V.A.
Popova E.G.
Porelli A.
Ptuskin V.S.
Rubtsov G.I.
Rüger M.
Samoliga V.S.
Semeney Y.A.
Silaev A.A.
Silaev A.A.
Skurikhin A.V.
Spiering C.
Sveshnikova L.G.
Tluczykont M.
Wischnewski R.
Zagorodnikov A.V.
Zurbanov A.V.
spellingShingle Prosin V.V.
Berezhnev S.F.
Budnev N.M.
Brückner M.
Chiavassa A.
Chvalaev O.A.
Dyachok A.V.
Epimakhov S.N.
Gafarov A.V.
Gress O.A.
Gress T.I.
Horns D.
Kalmykov N.N.
Karpov N.I.
Kiryuhin S.N.
Konstantinov E.N.
Korobchenko A.V.
Korosteleva E.E.
Kozhin V.A.
Kunnas M.
Kuzmichev L.A.
Lubsandorzhiev B.K.
Lubsandorzhiev N.B.
Mirgazov R.R.
Monkhoev R.D.
Nachtigall R.
Osipova E.A.
Pakhorukov A.L.
Panasyuk M.I.
Pankov L.V.
Poleschuk V.A.
Popova E.G.
Porelli A.
Ptuskin V.S.
Rubtsov G.I.
Rüger M.
Samoliga V.S.
Semeney Y.A.
Silaev A.A.
Silaev A.A.
Skurikhin A.V.
Spiering C.
Sveshnikova L.G.
Tluczykont M.
Wischnewski R.
Zagorodnikov A.V.
Zurbanov A.V.
Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype
EPJ Web of Conferences
author_facet Prosin V.V.
Berezhnev S.F.
Budnev N.M.
Brückner M.
Chiavassa A.
Chvalaev O.A.
Dyachok A.V.
Epimakhov S.N.
Gafarov A.V.
Gress O.A.
Gress T.I.
Horns D.
Kalmykov N.N.
Karpov N.I.
Kiryuhin S.N.
Konstantinov E.N.
Korobchenko A.V.
Korosteleva E.E.
Kozhin V.A.
Kunnas M.
Kuzmichev L.A.
Lubsandorzhiev B.K.
Lubsandorzhiev N.B.
Mirgazov R.R.
Monkhoev R.D.
Nachtigall R.
Osipova E.A.
Pakhorukov A.L.
Panasyuk M.I.
Pankov L.V.
Poleschuk V.A.
Popova E.G.
Porelli A.
Ptuskin V.S.
Rubtsov G.I.
Rüger M.
Samoliga V.S.
Semeney Y.A.
Silaev A.A.
Silaev A.A.
Skurikhin A.V.
Spiering C.
Sveshnikova L.G.
Tluczykont M.
Wischnewski R.
Zagorodnikov A.V.
Zurbanov A.V.
author_sort Prosin V.V.
title Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype
title_short Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype
title_full Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype
title_fullStr Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype
title_full_unstemmed Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype
title_sort results from tunka-133 (5 years observation) and from the tunka-hiscore prototype
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2016-01-01
description Data obtained with two detectors located at the Tunka Cosmic Ray facility are presented. The Cherenkov light array for registration of extensive air showers (EAS) Tunka-133 collected data during 5 winter seasons since 2009 to 2014. The differential energy spectrum of all particles and the dependence of the average maximum depth on the energy in the range of 6 · 1015−1018 eV measured for 1540 hours of observation are presented. The preliminary all particle energy spectrum by the data of Tunka-HiSCORE prototype array, installed in 2013, is presented. Some additional experiments in the Tunka Valley are briefly described.
url http://dx.doi.org/10.1051/epjconf/201612103004
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spelling doaj-2176f88177f74875a163e628e3ce23132021-08-02T17:24:24ZengEDP SciencesEPJ Web of Conferences2100-014X2016-01-011210300410.1051/epjconf/201612103004epjconf-RICAP-14_03004Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototypeProsin V.V.0Berezhnev S.F.1Budnev N.M.2Brückner M.3Chiavassa A.4Chvalaev O.A.5Dyachok A.V.6Epimakhov S.N.7Gafarov A.V.8Gress O.A.9Gress T.I.10Horns D.11Kalmykov N.N.12Karpov N.I.13Kiryuhin S.N.14Konstantinov E.N.15Korobchenko A.V.16Korosteleva E.E.17Kozhin V.A.18Kunnas M.19Kuzmichev L.A.Lubsandorzhiev B.K.20Lubsandorzhiev N.B.21Mirgazov R.R.22Monkhoev R.D.23Nachtigall R.24Osipova E.A.25Pakhorukov A.L.26Panasyuk M.I.27Pankov L.V.28Poleschuk V.A.29Popova E.G.30Porelli A.31Ptuskin V.S.32Rubtsov G.I.33Rüger M.34Samoliga V.S.35Semeney Y.A.36Silaev A.A.37Silaev A.A.38Skurikhin A.V.39Spiering C.40Sveshnikova L.G.41Tluczykont M.42Wischnewski R.43Zagorodnikov A.V.44Zurbanov A.V.45Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State UniversitySkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State UniversityInstitute of Applied Physics, Irkutsk State UniversityInstitute für Informatik, Humboldt UniversityUniversity of TurinInstitute of Applied Physics, Irkutsk State UniversityInstitute of Applied Physics, Irkutsk State UniversityInstitute fur Experimentalphysik, University of HamburgInstitute of Applied Physics, Irkutsk State UniversityInstitute of Applied Physics, Irkutsk State UniversityInstitute of Applied Physics, Irkutsk State UniversityInstitute fur Experimentalphysik, University of HamburgSkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State UniversitySkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State UniversityInstitute of Applied Physics, Irkutsk State UniversityInstitute of Applied Physics, Irkutsk State UniversityInstitute of Applied Physics, Irkutsk State UniversitySkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State UniversitySkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State UniversityInstitute fur Experimentalphysik, University of HamburgInstitute of Nuclear Research, Russian Academy of SciencesSkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State UniversityInstitute of Applied Physics, Irkutsk State UniversityInstitute of Applied Physics, Irkutsk State UniversityInstitute fur Experimentalphysik, University of HamburgSkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State UniversityInstitute of Applied Physics, Irkutsk State UniversitySkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State UniversityInstitute of Applied Physics, Irkutsk State UniversityInstitute of Applied Physics, Irkutsk State UniversitySkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State UniversityDESY ZeuthenPushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Waves Distribution, Russian Academy of SciencesInstitute of Nuclear Research, Russian Academy of SciencesDESY ZeuthenInstitute of Applied Physics, Irkutsk State UniversityInstitute of Applied Physics, Irkutsk State UniversitySkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State UniversitySkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State UniversitySkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State UniversityDESY ZeuthenSkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State UniversityInstitute fur Experimentalphysik, University of HamburgDESY ZeuthenInstitute of Applied Physics, Irkutsk State UniversityInstitute of Applied Physics, Irkutsk State UniversityData obtained with two detectors located at the Tunka Cosmic Ray facility are presented. The Cherenkov light array for registration of extensive air showers (EAS) Tunka-133 collected data during 5 winter seasons since 2009 to 2014. The differential energy spectrum of all particles and the dependence of the average maximum depth on the energy in the range of 6 · 1015−1018 eV measured for 1540 hours of observation are presented. The preliminary all particle energy spectrum by the data of Tunka-HiSCORE prototype array, installed in 2013, is presented. Some additional experiments in the Tunka Valley are briefly described.http://dx.doi.org/10.1051/epjconf/201612103004

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