Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype
oleh: 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.
| Format: | Article |
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| Diterbitkan: | EDP Sciences 2016-01-01 |
Deskripsi
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.