Radio detection of extensive air showers at the Pierre Auger Observatory

被引：0
|
作者：
Maller, Jennifer [1 ]
机构：
[1] Univ Nantes, CNRS, IN2P3, Ecole Mines Nantes,Subatech, Nantes, France
来源：
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2014年 / 742卷
关键词：
AERA; Radio detection; High energy cosmic rays; Pierre Auger Observatory; COSMIC-RAYS; EMISSION; RADIATION;
D O I：
10.1016/j.nima.2013.11.077
中图分类号：
TH7 [仪器、仪表];
学科分类号：
0804 ; 080401 ; 081102 ;
摘要：
Deployed at the end of 2010 at the Pierre Auger Observatory, the first stage of the Auger Engineering Radio Array, AERA24, consists of 24 radio stations covering an area of 0.5 km(2). AERA measures the radio emission from cosmic-ray induced air showers. The amplitude of this radio emission is used to constrain the characteristics of the primary particle: arrival direction, energy and nature. These studies are possible thanks to an instrumentation development allowing self-triggered and externally triggered measurements in the MHz domain and an improved understanding of radio emission processes. In May 2013, 100 new stations were installed to cover an area of similar or equal to 6 km(2), for a total of 124 stations. This stage 2 will provide higher statistics and will enhance both the estimate of the nature of the primary cosmic ray and the energy resolution above 10(17) eV as an addition to detectors such as the Auger fluorescence telescopes and particle detectors. We will present the main results obtained with the stage 1 of AERA and the current status of the experiment. We will end with a brief overview of the GHz-experiments installed at the Pierre Auger Observatory. (C) 2013 Elsevier B.V. All rights reserved.
引用
收藏
页码：232 / 236
页数：5
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