Depth of the Maximum of Extensive Air Showers (EASes) and the Mean Mass Composition of Primary Cosmic Rays in the 1015–1018 eV Range of Energies, According to Data from the TUNKA-133 and TAIGA-HiSCORE Arrays for Detecting EAS Cherenkov Light in the Tunkinsk Valley
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Prosin, V. V.; Astapov, I. I.; Voronin, D.; Gafarov, A. R.; Garmash, A. Yu.; Grebenyuk, V. M.; Gress, O. A.; +69 Authors
Prosin, V. V.; Astapov, I. I.; Voronin, D.; Gafarov, A. R.; Garmash, A. Yu.; Grebenyuk, V. M.; Gress, O. A.; Gress, T. I.; Grinyuk, A. A.; Grishin, O. G.; Dyachok, A. N.; Zhurov, D. P.; Bezyazeekov, P. A.; Zagorodnikov, A. V.; Ivanova, A. L.; Kalmykov, N. N.; Kindin, V. V.; Kiryuhin, S. N.; Kozhin, V. A.; Kokoulin, R. P.; Kompaniets, K. G.; Korosteleva, E. E.; Kravchenko, E. A.; Borodin, A. N.; Kryukov, A. P.; Kuzmichev, L. A.; Chiavassa, A.; Lavrova, M.; Lagutin, A. A.; Lemeshev, Yu.; Lubsandorzhiev, B. K.; Lubsandorzhiev, N. B.; Mirgazov, R. R.; Mirzoyan, R.; Brueckner, Martin; Monkhoev, R. D.; Osipova, E. A.; Pan, A.; Panasyuk, M. I.; Pankov, L. V.; Pakhorukov, A. L.; Petrukhin, A. A.; Poleschuk, V. A.; Popesku, M.; Popova, E. G.; Budnev, N. M.; Porelli, Andrea; Postnikov, E. B.; Ptuskin, V. S.; Pushnin, A. A.; Raikin, R. I.; Rubtsov, G. I.; Ryabov, E. V.; Sagan, Ya. I.; Samoliga, V. S.; Sveshnikova, L. G.; Bulan, A.; Sidorenkov, A. Yu.; Silaev, A. A.; Silaev, A. A.; Skurikhin, A. V.; Slunecka, M.; Sokolov, A. V.; Suvorkin, Y.; Tabolenko, V. A.; Tanaev, A.; Tarashansky, B. A.; Vaidyanathan, A.; Ternovoy, M.; Tkachev, L. G.; Tluczykont, M.; Ushakov, N.; Horns, D.; Yashin, I. I.; Wischnewski, Ralf; Volchugov, P.;
Depth of the Maximum of Extensive Air Showers (EASes) and the Mean Mass Composition of Primary Cosmic Rays in the 1015–1018 eV Range of Energies, According to Data from the TUNKA-133 and TAIGA-HiSCORE Arrays for Detecting EAS Cherenkov Light in the Tunkinsk Valley
A corrected energy dependence of the depth of the maximum in the wide range of energies 10$^{15}$ to 10$^{18}$ eV is obtained using data collected at the Tunka-133 facility over 7 years of operation (2009–2017) and the TAIGA-HiSCORE facility in the 2019–2020 season. At the highest energies, our results match those of the Pierre Auger observatory. The results are converted to parameter ❬ln A❭, which characterizes the mean EAS composition.
Germany
- University of Turin Italy
- Russian Academy of Sciences Russian Federation
- Institute for Nuclear Research Russian Federation
- Joint Institute for Nuclear Research Russian Federation
- Joint Institute for Nuclear Research Russian Federation
cosmic radiation: primary, mass spectrum, observatory, showers: atmosphere, air, info:eu-repo/classification/ddc/530, radiation: Cherenkov, energy dependence, Auger
cosmic radiation: primary, mass spectrum, observatory, showers: atmosphere, air, info:eu-repo/classification/ddc/530, radiation: Cherenkov, energy dependence, Auger
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
Citations provided by BIP!popularityPopularity provided by BIP!
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
Popularity provided by BIP! 9
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