Study on the muon lateral distribution based on the first stage of LHAASO-KM2A

被引：0

作者：

Xin, Guang-Guang ^{[1
,2
]}

Zhang, Yi ^{[2
]}

Feng, You-Liang ^{[3
]}

Zhao, Shiping ^{[2
]}

Guo, Ying-Ying ^{[2
]}

Xiao, Gang ^{[2
]}

Li, Cong ^{[2
]}

Zuo, Xiong ^{[2
]}

Wang, Ling-Yu ^{[2
]}

Cheng, Ning ^{[2
]}

机构：

[1] Wuhan Univ, Sch Phys & Technol, Wuhan 430072, Peoples R China

[2] Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China

[3] Chinese Acad Sci, Key Lab Dark Matter & Space Astron, Purple Mt Observ, Nanjing 210034, Peoples R China

来源：

36TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2019 | 2021年

基金：

中国国家自然科学基金; 国家重点研发计划;

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The first stage of LHAASO-KM2A has been completed in Sichuan, China. KM2A is composed of electromagnetic particle detectors (ED) and muon detectors (MD), focusing on gamma ray astronomy above 30 TeV and cosmic ray physics in the "knee" region. The ED array in the first stage is installed into two clusters and the distance between the two clusters is around 230 meters. The MDs are distributed in one of the clusters. Each MD is covered with soil of 2.5 meters thick. We analyzed the lateral distribution of muons which are 140-300 meters away from Shower axis, and the primary cosmic ray energy is about 100TeV.

引用

页数：8

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