Precision measurements of cosmic rays up to the highest energies with a large radio array at the Pierre Auger Observatory

被引：6

作者：

Horandel, JOrg R. ^{[1
,2
,3
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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：

ULTRA HIGH ENERGY COSMIC RAYS 2018 (UHECR 2018) | 2019年 / 210卷

基金：

欧洲研究理事会;

关键词：

MONTE-CARLO SIMULATIONS; AIR-SHOWERS; EMISSION; RADIATION; PULSES;

D O I：

10.1051/epjconf/201921006005

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：9

共 23 条

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