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arxiv: 2207.09680 · v2 · pith:7ZWX2EW3new · submitted 2022-07-20 · 🌌 astro-ph.IM · astro-ph.HE

The Tunka-Grande scintillation array: current results

A. L. Ivanova , I. Astapov , P. Bezyazeekov , E. Bonvech , A. Borodin , N. Budnev , A. Bulan , D. Chernov
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A. Chiavassa A. Dyachok A. Gafarov A. Garmash V. Grebenyuk E. Gress O. Gress T. Gress A. Grinyuk O. Grishin A. D. Ivanova N. Kalmykov V. Kindin S. Kiryuhin R. Kokoulin K. Kompaniets E. Korosteleva V. Kozhin E. Kravchenko A. Kryukov L. Kuzmichev A. Lagutin M. Lavrova Y. Lemeshev B. Lubsandorzhiev N. Lubsandorzhiev A. Lukanov D. Lukyantsev S. Malakhov R. Mirgazov R. Monkhoev E. Osipova A. Pakhorukov L. Pankov A. Pan A. Panov A. Petrukhin I. Poddubnyi D. Podgrudkov V. Poleschuk V. Ponomareva E. Popova E. Postnikov V. Prosin V. Ptuskin A. Pushnin R. Raikin A. Razumov G. Rubtsov E. Ryabov Y. Sagan V. Samoliga A. Satyshev A. Silaev A. Silaev (junior) A. Sidorenkov A. Skurikhin A. Sokolov L. Sveshnikova V. Tabolenko L. Tkachev A. Tanaev M. Ternovoy R. Togoo N. Ushakov A. Vaidyanathan P. Volchugov N. Volkov D. Voronin A. Zagorodnikov D. Zhurov I. Yashin
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classification 🌌 astro-ph.IM astro-ph.HE
keywords tunka-grandearraycosmiccurrentenergyexperimentrangeresults
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The Tunka-Grande experiment is a scintillation array with about 0.5 sq.km sensitive area at Tunka Valley, Siberia, for measuring charged particles and muons in extensive air showers (EASs). Tunka-Grande is optimized for cosmic ray studies in the energy range 10 PeV to about 1 EeV, where exploring the composition is of fundamental importance for understanding the transition from galactic to extragalactic origin of cosmic rays. This paper attempts to provide a synopsis of the current results of the experiment. In particular, the reconstruction of the all-particle energy spectrum in the range of 10 PeV to 1 EeV based on experimental data from four observation seasons is presented.

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