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spelling paper:paper_17480221_v8_n12_p_Platino2023-06-08T16:28:34Z AMIGA at the Auger observatory: The telecommunications system Data Handling Large detector systems for particle and astroparticle physics Trigger concepts and systems (hardware and software) Astroparticle physics Data acquisition system Data processing systems Fluorescence detector Hardware and software Photo multiplier tube Pierre Auger observatory Scintillator strips Augers Data handling Data processing Detectors Observatories Optical fibers Radio links Scintillation counters Telecommunication Charged particles AMIGA is an extension of the Pierre Auger Observatory that will consist of 85 detector pairs, each one composed of a surface water-Cherenkov detector and a buried muon counter. Each muon counter has an area of 30 square meters and is made of scintillator strips, with doped optical fibers glued to them, which guide the light to 64 pixel photomultiplier tubes. The detector pairs are arranged at 433 m and 750 m array spacings. In this paper we present the telecommunications system designed to connect the muon counters with the central data processing system at the observatory campus in Malarg"ue. The telecommunications system consists of a point-to-multipoint radio link designed to connect the 85 muon counters or subscribers to two coordinators located at the Coihueco fluorescence detector building. The link provides TCP/IP remote access to the scintillator modules through router boards installed on each of the surface detectors of AMIGA. This setup provides a flexible LAN configuration for each muon counter connected to a WAN that links all the data generated by the muon counters and the surface detectors to the Central Data Acquisition System, or CDAS, at the observatory campus. We present the design parameters, the proposed telecommunications solution and the laboratory and field tests proposed to guarantee its functioning for the whole data traffic generated between each surface detector and muon counter in the AMIGA array and the CDAS.© 2013 IOP Publishing Ltd and Sissa Medialab srl. 2013 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17480221_v8_n12_p_Platino http://hdl.handle.net/20.500.12110/paper_17480221_v8_n12_p_Platino
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Data Handling
Large detector systems for particle and astroparticle physics
Trigger concepts and systems (hardware and software)
Astroparticle physics
Data acquisition system
Data processing systems
Fluorescence detector
Hardware and software
Photo multiplier tube
Pierre Auger observatory
Scintillator strips
Augers
Data handling
Data processing
Detectors
Observatories
Optical fibers
Radio links
Scintillation counters
Telecommunication
Charged particles
spellingShingle Data Handling
Large detector systems for particle and astroparticle physics
Trigger concepts and systems (hardware and software)
Astroparticle physics
Data acquisition system
Data processing systems
Fluorescence detector
Hardware and software
Photo multiplier tube
Pierre Auger observatory
Scintillator strips
Augers
Data handling
Data processing
Detectors
Observatories
Optical fibers
Radio links
Scintillation counters
Telecommunication
Charged particles
AMIGA at the Auger observatory: The telecommunications system
topic_facet Data Handling
Large detector systems for particle and astroparticle physics
Trigger concepts and systems (hardware and software)
Astroparticle physics
Data acquisition system
Data processing systems
Fluorescence detector
Hardware and software
Photo multiplier tube
Pierre Auger observatory
Scintillator strips
Augers
Data handling
Data processing
Detectors
Observatories
Optical fibers
Radio links
Scintillation counters
Telecommunication
Charged particles
description AMIGA is an extension of the Pierre Auger Observatory that will consist of 85 detector pairs, each one composed of a surface water-Cherenkov detector and a buried muon counter. Each muon counter has an area of 30 square meters and is made of scintillator strips, with doped optical fibers glued to them, which guide the light to 64 pixel photomultiplier tubes. The detector pairs are arranged at 433 m and 750 m array spacings. In this paper we present the telecommunications system designed to connect the muon counters with the central data processing system at the observatory campus in Malarg"ue. The telecommunications system consists of a point-to-multipoint radio link designed to connect the 85 muon counters or subscribers to two coordinators located at the Coihueco fluorescence detector building. The link provides TCP/IP remote access to the scintillator modules through router boards installed on each of the surface detectors of AMIGA. This setup provides a flexible LAN configuration for each muon counter connected to a WAN that links all the data generated by the muon counters and the surface detectors to the Central Data Acquisition System, or CDAS, at the observatory campus. We present the design parameters, the proposed telecommunications solution and the laboratory and field tests proposed to guarantee its functioning for the whole data traffic generated between each surface detector and muon counter in the AMIGA array and the CDAS.© 2013 IOP Publishing Ltd and Sissa Medialab srl.
title AMIGA at the Auger observatory: The telecommunications system
title_short AMIGA at the Auger observatory: The telecommunications system
title_full AMIGA at the Auger observatory: The telecommunications system
title_fullStr AMIGA at the Auger observatory: The telecommunications system
title_full_unstemmed AMIGA at the Auger observatory: The telecommunications system
title_sort amiga at the auger observatory: the telecommunications system
publishDate 2013
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17480221_v8_n12_p_Platino
http://hdl.handle.net/20.500.12110/paper_17480221_v8_n12_p_Platino
_version_ 1768543154249662464