Properties and performance of the prototype instrument for the Pierre Auger Observatory
Construction of the first stage of the Pierre Auger Observatory has begun. The aim of the Observatory is to collect unprecedented information about cosmic rays above 10 18 eV. The first phase of the project, the construction and operation of a prototype system, known as the engineering array, has no...
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todo:paper_01689002_v523_n1-2_p50_Abraham2023-10-03T15:06:43Z Properties and performance of the prototype instrument for the Pierre Auger Observatory Abraham, J. Auger Observatory Extensive air showers Ultra high energy cosmic rays Construction of the first stage of the Pierre Auger Observatory has begun. The aim of the Observatory is to collect unprecedented information about cosmic rays above 10 18 eV. The first phase of the project, the construction and operation of a prototype system, known as the engineering array, has now been completed. It has allowed all of the sub-systems that will be used in the full instrument to be tested under field conditions. In this paper, the properties and performance of these sub-systems are described and their success illustrated with descriptions of some of the events recorded thus far. © 2003 Elsevier B.V. All rights reserved. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_01689002_v523_n1-2_p50_Abraham |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Auger Observatory Extensive air showers Ultra high energy cosmic rays |
spellingShingle |
Auger Observatory Extensive air showers Ultra high energy cosmic rays Abraham, J. Properties and performance of the prototype instrument for the Pierre Auger Observatory |
topic_facet |
Auger Observatory Extensive air showers Ultra high energy cosmic rays |
description |
Construction of the first stage of the Pierre Auger Observatory has begun. The aim of the Observatory is to collect unprecedented information about cosmic rays above 10 18 eV. The first phase of the project, the construction and operation of a prototype system, known as the engineering array, has now been completed. It has allowed all of the sub-systems that will be used in the full instrument to be tested under field conditions. In this paper, the properties and performance of these sub-systems are described and their success illustrated with descriptions of some of the events recorded thus far. © 2003 Elsevier B.V. All rights reserved. |
format |
JOUR |
author |
Abraham, J. |
author_facet |
Abraham, J. |
author_sort |
Abraham, J. |
title |
Properties and performance of the prototype instrument for the Pierre Auger Observatory |
title_short |
Properties and performance of the prototype instrument for the Pierre Auger Observatory |
title_full |
Properties and performance of the prototype instrument for the Pierre Auger Observatory |
title_fullStr |
Properties and performance of the prototype instrument for the Pierre Auger Observatory |
title_full_unstemmed |
Properties and performance of the prototype instrument for the Pierre Auger Observatory |
title_sort |
properties and performance of the prototype instrument for the pierre auger observatory |
url |
http://hdl.handle.net/20.500.12110/paper_01689002_v523_n1-2_p50_Abraham |
work_keys_str_mv |
AT abrahamj propertiesandperformanceoftheprototypeinstrumentforthepierreaugerobservatory |
_version_ |
1807324355699408896 |