A large radio array at the Pierre Auger Observatory Precision measurements of the properties of cosmic rays at the highest energies

被引：1

作者：

Horandel, Jorg R. ^{[1
,2
,3
]}

机构：

[1] Radboud Univ Nijmegen, Dept Astrophys IMAPP, POB 9010, NL-6500 GL Nijmegen, Netherlands

[2] Nikhef, Sci Pk 105, NL-1098 XG Amsterdam, Netherlands

[3] Vrije Univ Brussel, Dept Phys & Astron, B-1050 Brussels, Belgium

[4] Observ Pierre Auger, Av San Martin Norte 304, RA-5613 Malargue, Argentina

来源：

8TH INTERNATIONAL CONFERENCE ON ACOUSTIC AND RADIO EEV NEUTRINO DETECTION ACTIVITIES (ARENA 2018) | 2019年 / 216卷

基金：

欧洲研究理事会;

关键词：

D O I：

10.1051/epjconf/201921601010

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Pierre Auger observatory is presently being upgraded to enlarge its detection capabilities for ultra-high-energy cosmic rays. Part of this upgrade is a radio detector array, aimed to cover a surface area of 3000 km(2) to measure the properties of the highest-energy cosmic rays. The plans for this radio upgrade are outlined.

引用

页数：7

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