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 ]
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.
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收藏
页数：9
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