KM3NeT acoustic positioning and detection system

In the Mediterranean Sea, the KM3NeT Collaboration is constructing a the deep-sea research infrastructure hosting next generation neutrino telescopes. In the KM3NeT telescopes the Cherenkov radiation induced by the secondary charged particles produced in the interaction of cosmic and atmospheric neu...

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Main Author: Viola Salvatore
Format: Article
Language:English
Published: EDP Sciences 2019-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2019/21/epjconf_arena2018_02006.pdf
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author Viola Salvatore
author_facet Viola Salvatore
author_sort Viola Salvatore
collection DOAJ
description In the Mediterranean Sea, the KM3NeT Collaboration is constructing a the deep-sea research infrastructure hosting next generation neutrino telescopes. In the KM3NeT telescopes the Cherenkov radiation induced by the secondary charged particles produced in the interaction of cosmic and atmospheric neutrinos within an effective volume between megaton and several cubic kilometers of water are detected by an array of thousands of photomultipliers. The capability of the telescope to determine the direction of secondary charged particles and to point back to the neutrino source is strongly connected to the accuracy on photomultipliers positions. In KM3NeT, the photomultiplier positions are continuously monitored by an acoustic positioning system, designed by the KM3NeT Collaboration to reach an accuracy of the photomultiplier positions better than 20 cm.
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spelling doaj.art-0ef414a1280e4ee3b279075224a58a3a2022-12-21T21:25:26ZengEDP SciencesEPJ Web of Conferences2100-014X2019-01-012160200610.1051/epjconf/201921602006epjconf_arena2018_02006KM3NeT acoustic positioning and detection systemViola SalvatoreIn the Mediterranean Sea, the KM3NeT Collaboration is constructing a the deep-sea research infrastructure hosting next generation neutrino telescopes. In the KM3NeT telescopes the Cherenkov radiation induced by the secondary charged particles produced in the interaction of cosmic and atmospheric neutrinos within an effective volume between megaton and several cubic kilometers of water are detected by an array of thousands of photomultipliers. The capability of the telescope to determine the direction of secondary charged particles and to point back to the neutrino source is strongly connected to the accuracy on photomultipliers positions. In KM3NeT, the photomultiplier positions are continuously monitored by an acoustic positioning system, designed by the KM3NeT Collaboration to reach an accuracy of the photomultiplier positions better than 20 cm.https://www.epj-conferences.org/articles/epjconf/pdf/2019/21/epjconf_arena2018_02006.pdf
spellingShingle Viola Salvatore
KM3NeT acoustic positioning and detection system
EPJ Web of Conferences
title KM3NeT acoustic positioning and detection system
title_full KM3NeT acoustic positioning and detection system
title_fullStr KM3NeT acoustic positioning and detection system
title_full_unstemmed KM3NeT acoustic positioning and detection system
title_short KM3NeT acoustic positioning and detection system
title_sort km3net acoustic positioning and detection system
url https://www.epj-conferences.org/articles/epjconf/pdf/2019/21/epjconf_arena2018_02006.pdf
work_keys_str_mv AT violasalvatore km3netacousticpositioninganddetectionsystem