The Primary CR Spectrum by the Data of the Tunka-133 Array

Авторы: Berezhnev S.F., Budnev N.M., Chiavassa A., Chvalaev O.A., Gress O.A., Gress T.I., Dyachok A.N., Epimakhov S.N., Karpov N.I., Kalmykov N.N., Konstantinov E.N., Korobchenko A.V., Korosteleva E.E., Kozhin V.A., Kuzmichev L.A., Lubsandorzhiev B.K., Mirgazov R.R., Monkhoev R.D., Osipova E.A., Pakhorukov A.L., Panasyuk M.I., Pankov L.V., Popova E.G., Prosin V.V., Ptuskin V.S., Semeney Yu A., Silaev A.A., Silaev A.A., Skurikhin A.V., Spiering C., Sveshnikova L.G., Zagorodnikov A.V.
Журнал: JPS Conference Proceedings
Том: 9
Год издания: 2016
Первая страница: 010009
DOI: 10.7566/JPSCP.9.010009
Аннотация: The Cherenkov-light EAS array Tunka-133, with ∼3 km2 geometric area, is taking data since 2009. The array permits a detailed study of energy spectrum and mass composition of cosmic rays in the energy range from 5•1015 to 1018 eV. We describe the array construction, the DAQ and the array calibration and discuss the method of energy reconstruction and absolute calibration. We present the all-particle energy spectrum based on 5 seasons of array operation. In the last part of the paper, we discuss possible interpretations of the obtained results and sketch plans for upgrading the array
Добавил в систему: Кузьмичев Леонид Александрович

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