Composition of Cosmic Rays with E0 1017 eV Based on Data from the Ground Scintillation Detectors of the Yakutsk EAS Array

被引：7
|
作者：
Glushkov, A. V. [1 ]
Pravdin, M. I. [1 ]
Saburov, A. V. [1 ]
机构：
[1] Russian Acad Sci, Shafer Inst Cosmophys Res & Aeron, Siberian Branch, Pr Lenina 31, Yakutsk 677007, Russia
来源：
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2018年 / 44卷 / 10期
基金：
俄罗斯基础研究基金会;
关键词：
ultrahigh-energy cosmic rays; extensive air showers; nuclear composition of primary particles; EXTENSIVE AIR-SHOWERS; ULTRA-HIGH ENERGIES; MODEL;
D O I：
10.1134/S106377371810002X
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The lateral distribution of cascade particles in extensive air showers from cosmic rays with energy E-0 10(17) eV has been studied at the Yakutsk array by the ground scintillation detectors over the period of continuous observations 1977-2017. The experimental data are compared with those computed with various models for the development of extensive air showers from the CORSIKA software package. The best agreement between the theory and experiment is observed for the QGSjet-01-d model. In the energy range (1-20)x 10(17) eV there is a change in the cosmic-raymass composition from lnA approximate to 2.5 to the proton one.
引用
收藏
页码：588 / 592
页数：5
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