Aller au contenu principal
Accès ouvert déclaré 2021 article

Design and implementation of the AMIGA embedded system for data acquisition

7Citations signalées, ce qui n’est pas une note de qualité
102Institutions déclarées
20Pays d’affiliation déclarés

Rattachement africain : nl, pt, it, au, ar, es, us, de, mx, ro, cz, pe, fr, br, pl, be, si, jp, co, gb. Niveau de preuve : code pays fourni par la source.

Le résumé fourni par la source

Abstract 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.

Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.

Le contrôle bibliographique ouvert

DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.

Titre Crossref
Design and implementation of the AMIGA embedded system for data acquisition
Date Crossref
01/07/2021
Éditeur
IOP Publishing
Type
journal-article

Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.

Les institutions déclarées

Radboud University NijmegenUniversity of LisbonLIP - Laboratory of Instrumentation and Experimental Particle PhysicsIstituto Nazionale di Fisica Nucleare, Sezione di TorinoOsservatorio Astrofisico di TorinoThe University of AdelaideConsejo Nacional de Investigaciones Científicas y TécnicasBalseiro InstituteBariloche Atomic CentreNational Technological UniversityNational University of General San MartínInstituto de Tecnologías en Detección y AstropartículasUniversidade de Santiago de CompostelaUniversity of TurinLehman CollegeIstituto Nazionale di Fisica Nucleare, Sezione di NapoliRWTH Aachen UniversityUniversidad Michoacana de San Nicolás de HidalgoComisión Nacional de Energía AtómicaUniversitatea Națională de Știință și Tehnologie Politehnica BucureștiFZU ‒ Institute of Physics of the Academy of Sciences of the Czech RepublicHoria Hulubei National Institute for R and D in Physics and Nuclear EngineeringIstituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran SassoGran Sasso Science InstituteUniversity of WuppertalUniversidad Nacional de San Agustin de ArequipaCentre National de la Recherche ScientifiqueUniversité Grenoble AlpesMax Planck Institute for Radio AstronomyInstitute of Physics RosarioUniversité Paris-SaclayInstitut National de Physique Nucléaire et de Physique des ParticulesLaboratoire de Physique des 2 Infinis Irène Joliot-CurieUniversity of L'AquilaUniversidade Federal do Rio de JaneiroUniversidade de São PauloInstitute of Nuclear Physics, Polish Academy of SciencesColorado State UniversityUniversity of SiegenUniversidad de GranadaVrije Universiteit BrusselIstituto Nazionale di Fisica Nucleare, Sezione di CataniaUniversidad Autónoma de ChiapasUniversity of MilanIstituto Nazionale di Fisica Nucleare, Sezione di MilanoNational Institute for Subatomic PhysicsUniversity of CataniaIstituto Nazionale di Fisica Nucleare, Sezione di LeccePierre Auger ObservatoryUniversidade Estadual de Campinas (UNICAMP)Université Libre de BruxellesPalacký University OlomoucUniversity of Naples Federico IIUniversity of DelawarePolitecnico di MilanoUniversity of SalentoUniversidade Federal FluminenseCase Western Reserve UniversityUniversidad de Buenos AiresInstitute of Astronomy and Space PhysicsKarlsruhe Institute of TechnologyValongo ObservatoryUniversidad Nacional Autónoma de MéxicoUniversidade Federal do ParanáUniversidad Nacional de La PlataFermi National Accelerator LaboratoryNetherlands Institute for Radio AstronomyReproductive Medicine InstituteNew York UniversityMichigan Technological UniversityUniversity of Nova GoricaJožef Stefan InstituteKyoto UniversityUniversity of ŁódźUniversidade Estadual de Feira de SantanaInstitute of Space Science - INFLPR SubsidiaryColorado School of MinesFederal Center for Technological Education Celso Suckow da FonsecaUniversidade Federal do ABCUniversité Paris CitéSorbonne UniversitéLaboratoire de Physique Nucléaire et de Hautes ÉnergiesBenemérita Universidad Autónoma de PueblaUniversity of Wisconsin–MadisonUniversität HamburgUniversity of PalermoLouisiana State UniversityUniversity of Rome Tor VergataIstituto Nazionale di Fisica Nucleare, Roma Tor VergataPennsylvania State UniversityCharles UniversityIndustrial University of SantanderInstitute of Scientific and Technical Research for DefenseInstituto Politécnico NacionalUniversity of GroningenIstituto di Astrofisica Spaziale e Fisica cosmica di PalermoCentro Brasileiro de Pesquisas FísicasUniversity of BucharestUniversidad de MedellínUniversity of AmsterdamUniversity of LeedsCentro de Investigación y de Estudios Avanzados del Instituto Politécnico Nacional

Une affiliation ne permet pas de déduire la nationalité d’un auteur.

Les sujets associés

Astrophysics and Cosmic PhenomenaDark Matter and Cosmic PhenomenaParticle Detector Development and Performance

BNTIC News n’est pas le producteur de ces données. Les publications sont interrogées à la demande dans Crossref, OpenAIRE, DOAJ, Europe PMC, HAL, DataCite, AfricArXiv, ROR et la Banque mondiale, sans clé d’accès. OpenAlex reste optionnel. Aucun service payant n’est nécessaire et aucune donnée externe n’est enregistrée en base. Consulter les sources et leurs limites.