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

TAIGA Collaboration

Результат исследования: Научные публикации в периодических изданияхстатьярецензирование

Аннотация

A corrected energy dependence of the depth of the maximum in the wide range of energies 1015 to 1018 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.

Язык оригиналаанглийский
Страницы (с-по)395-397
Число страниц3
ЖурналBulletin of the Russian Academy of Sciences: Physics
Том85
Номер выпуска4
DOI
СостояниеОпубликовано - апр 2021

Предметные области OECD FOS+WOS

  • 1.03 ФИЗИЧЕСКИЕ НАУКИ И АСТРОНОМИЯ

ГРНТИ

  • 29 ФИЗИКА

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