Primary CR energy spectrum and mass composition by the data of Tunka-133 array
Primary CR energy spectrum and mass composition by the data of Tunka-133 array
复制标题
Tunka-133 阵列数据的初级 CR 能谱和质量组成
DOI：
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发表时间：
2015
期刊：
影响因子：
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通讯作者：
A. Zagorodnikov
中科院分区：
文献类型：
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作者：
V. Prosin;S. Berezhnev;N. Budnev;A. Chiavassa;O. Chvalaev;A. Dyachok;S. Epimakhov;O. Gress;T. Gress;N. Kalmykov;N. Karpov;E. Konstantinov;A. Korobchenko;E. Korosteleva;V. Kozhin;L. Kuzmichev;B. Lubsandorzhiev;N. Lubsandorzhiev;R. Mirgazov;R. Monkhoev;É. Osipova;A. Pakhorukov;M. Panasyuk;L. Pankov;E. Popova;V. Ptuskin;Y. Semeney;A. Silaev;A. Skurikhin;C. Spiering;L. Sveshnikova;A. Zagorodnikov
切伦科夫光阵列登记广泛的空气阵雨（EAS）通卡-133收集的数据在5个冬季从2009年到2014年。本文给出了1540小时观测的所有粒子的微分能谱，以及在6 ·1015 - 1018 eV范围内平均最大深度与能量的关系。
The Cherenkov light array for the registration of extensive air showers (EAS) Tunka-133 collected data during 5 winter seasons from 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 · 10 15 -10 18 eV measured for 1540 hours of observation are presented.