Design and implementation of the AMIGA embedded system for data acquisition

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The Auger Muon Infill Ground Array (AMIGA) is part of the AugerPrime upgrade of the Pierre Auger Observatory. It consists of particle counters buried 2.3 m underground next to the water-Cherenkov stations that form the 23.5 km2 large infilled array. The reduced distance between detectors in this den...

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Detalles Bibliográficos
Autores principales: Binet, V., The Pierre Auger collaboration
Lenguaje:Inglés
Publicado: IOP Publishing 2022
Materias:
Data acquisition concepts
Detector control systems (detector and experiment monitoring and slow-control systems, architecture, hardware, algorithms, databases)
Control and monitor systems online
Acceso en línea:http://hdl.handle.net/2133/23265
http://hdl.handle.net/2133/23265
Aporte de:
Repositorio Hipermedial de la Universidad Nacional de Rosario (UNR) de Universidad Nacional de Rosario
id I15-R121-2133-23265
record_format dspace
institution Universidad Nacional de Rosario
institution_str I-15
repository_str R-121
collection Repositorio Hipermedial de la Universidad Nacional de Rosario (UNR)
language Inglés
orig_language_str_mv eng
topic Data acquisition concepts
Detector control systems (detector and experiment monitoring and slow-control systems, architecture, hardware, algorithms, databases)
Control and monitor systems online
spellingShingle Data acquisition concepts
Detector control systems (detector and experiment monitoring and slow-control systems, architecture, hardware, algorithms, databases)
Control and monitor systems online
Binet, V.
The Pierre Auger collaboration
Design and implementation of the AMIGA embedded system for data acquisition
topic_facet Data acquisition concepts
Detector control systems (detector and experiment monitoring and slow-control systems, architecture, hardware, algorithms, databases)
Control and monitor systems online
description The Auger Muon Infill Ground Array (AMIGA) is part of the AugerPrime upgrade of the Pierre Auger Observatory. It consists of particle counters buried 2.3 m underground next to the water-Cherenkov stations that form the 23.5 km2 large infilled array. The reduced distance between detectors in this denser area allows the lowering of the energy threshold for primary cosmic ray reconstruction down to about 1017 eV. At the depth of 2.3 m the electromagnetic component of cosmic ray showers is almost entirely absorbed so that the buried scintillators provide an independent and direct measurement of the air showers muon content. This work describes the design and implementation of the AMIGA embedded system, which provides centralized control, data acquisition and environment monitoring to its detectors. The presented system was firstly tested in the engineering array phase ended in 2017, and lately selected as the final design to be installed in all new detectors of the production phase. The system was proven to be robust and reliable and has worked in a stable manner since its first deployment.
author Binet, V.
The Pierre Auger collaboration
author_facet Binet, V.
The Pierre Auger collaboration
author_sort Binet, V.
title Design and implementation of the AMIGA embedded system for data acquisition
title_short Design and implementation of the AMIGA embedded system for data acquisition
title_full Design and implementation of the AMIGA embedded system for data acquisition
title_fullStr Design and implementation of the AMIGA embedded system for data acquisition
title_full_unstemmed Design and implementation of the AMIGA embedded system for data acquisition
title_sort design and implementation of the amiga embedded system for data acquisition
publisher IOP Publishing
publishDate 2022
url http://hdl.handle.net/2133/23265
http://hdl.handle.net/2133/23265
work_keys_str_mv AT binetv designandimplementationoftheamigaembeddedsystemfordataacquisition
AT thepierreaugercollaboration designandimplementationoftheamigaembeddedsystemfordataacquisition
bdutipo_str Repositorios
_version_ 1764820411900493824

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