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Design and implementation of the AMIGA embedded system for data acquisition
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SYSNO ASEP 0548312 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Design and implementation of the AMIGA embedded system for data acquisition Author(s) Aab, A. (NL)
Abreu, A. (PT)
Aglietta, M. (IT)
Bakalová, Alena (FZU-D) ORCID
Blažek, Jiří (FZU-D) ORCID, RID
Boháčová, Martina (FZU-D) RID, ORCID
Chudoba, Jiří (FZU-D) RID, ORCID
Ebr, Jan (FZU-D) RID, ORCID
Hamal, Petr (FZU-D) ORCID
Janeček, Petr (FZU-D) RID, ORCID
Juryšek, Jakub (FZU-D) ORCID
Mandát, Dušan (FZU-D) RID, ORCID
Palatka, Miroslav (FZU-D) RID, ORCID, SAI
Pech, Miroslav (FZU-D) RID, ORCID
Prouza, Michael (FZU-D) RID, ORCID
Řídký, Jan (FZU-D) RID, ORCID
dos Santos, Eva M. Martins (FZU-D) ORCID
Schovánek, Petr (FZU-D) RID, ORCID
Tobiška, Petr (FZU-D) ORCID
Trávníček, Petr (FZU-D) RID, ORCID
Vícha, Jakub (FZU-D) RID, ORCID
Yushkov, Alexey (FZU-D) ORCIDNumber of authors 383 Article number T07008 Source Title Journal of Instrumentation. - : Institute of Physics Publishing - ISSN 1748-0221
Roč. 16, č. 7 (2021)Number of pages 33 s. Language eng - English Country GB - United Kingdom Keywords data acquisition concepts ; particle detectors ; detector control systems (detector and experiment monitoring and slow ̧control systems,architecture, hardware,algorithms, databases) Subject RIV BF - Elementary Particles and High Energy Physics OECD category Particles and field physics R&D Projects LM2015038 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) LG15014 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) GA14-17501S GA ČR - Czech Science Foundation (CSF) LM2018102 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) Method of publishing Open access Institutional support FZU-D - RVO:68378271 UT WOS 000694891700007 EID SCOPUS 85111600452 DOI 10.1088/1748-0221/16/07/T07008 Annotation 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 km(2) 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 10(17) 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. Workplace Institute of Physics Contact Kristina Potocká, potocka@fzu.cz, Tel.: 220 318 579 Year of Publishing 2022 Electronic address http://hdl.handle.net/11104/0324389
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