Tunka-25 Air Shower Cherenkov array: The main results

被引：31

作者：

Budnev, N. ^{[2
]}

Chernov, D. ^{[1
]}

Gress, O. ^{[2
]}

Korosteleva, E. ^{[1
]}

Kuzmichev, L. ^{[1
]}

Lubsandorzhiev, B. ^{[3
]}

Navarra, G. ^{[4
,5
]}

Pankov, L. ^{[2
]}

Prosin, V. ^{[1
]}

Semeney, Yu. ^{[2
]}

Spiering, C. ^{[6
]}

Wischnewski, R. ^{[6
]}

Yashin, J. ^{[1
]}

机构：

[1] MSU, Skobeltsyn Inst Nucl Phys, RU-119991 Moscow, Russia

[2] Irkutsk State Univ, RU-664003 Irkutsk, Russia

[3] Russian Acad Sci, Inst Nucl Res, RU-117312 Moscow, Russia

[4] Dipartimento Fis Gen Univ, I-10125 Turin, Italy

[5] Ist Nazl Fis Nucl, I-10125 Turin, Italy

[6] DESY, D-15738 Zeuthen, Germany

来源：

ASTROPARTICLE PHYSICS | 2013年 / 50-52卷

基金：

俄罗斯基础研究基金会;

关键词：

High energy cosmic rays; Air shower; Cherenkov radiation; Energy spectrum; Mass composition; RAY ENERGY-SPECTRUM; COSMIC-RAYS; LIGHT; REGION; KNEE;

D O I：

10.1016/j.astropartphys.2013.09.006

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the main results of the Extensive Air Shower Cherenkov array Tunka-25. They cover the energy spectrum from 8.10(14) to 10(17) eV and mass composition of primary cosmic rays in the energy range of 3.10(15)-3.10(16) eV. A new lateral distribution function (LDF) of Air Shower Cherenkov light and a new method to analyze the maximum depth distribution of the shower have been developed. Both have been successfully applied in the data analysis of Tunka-25. We also discuss methods of time and amplitude calibration of the array, providing an accurate determination of the primary energy and the steepness of the LDF. (C) 2013 Elsevier B.V. All rights reserved.

引用

页码：18 / 25

页数：8

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