The KM3NeT/ARCA: Status and results of the Acoustic Positioning System

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F25%3A00389206" target="_blank" >RIV/68407700:21670/25:00389206 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.22323/1.501.1156" target="_blank" >https://doi.org/10.22323/1.501.1156</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.22323/1.501.1156" target="_blank" >10.22323/1.501.1156</a>

Jazyk výsledku

angličtina

Název v původním jazyce

The KM3NeT/ARCA: Status and results of the Acoustic Positioning System

Popis výsledku v původním jazyce

The KM3NeT (Cubic Kilometre Neutrino Telescope) Collaboration is currently building two underwater neutrino detectors: ORCA (Oscillation Research with Cosmics in the Abysses) located offshore Toulon, France, at 2500 m water depth, and ARCA (Astronomy Research with Cosmics in the Abysses) offshore Capo Passero, Italy, at 3500 m water depth. The basic element of the detector is the DOM (Digital Optical Module), housing 31 photomultiplier tubes (PMTs), capable of recording single photon arrival time and charge, to be sent to shore for triggering, filtering, and data analysis. A vertical line of 18 DOMs forms a Detection Unit (DU): about 700 m long in ARCA, and about 200 m long in ORCA. A custom Acoustic Positioning System (APS) was designed and developed by the KM3NeT collaboration to obtain an accuracy of a few centimeters in the determination of the position of each DOM. In the case of KM3NeT-ARCA, the subject of this paper, this is required in order to be able to reconstruct neutrino directions with the desired pointing resolution. Building upon the White Rabbit time synchronization, the APS operates as a phased array of several thousand digital acoustic receivers, hosted in all DOMs and the anchors of the DUs. Each receiver records acoustic signals emitted by a long baseline of georeferenced acoustic emitters anchored on the seafloor. The APS allows constant monitoring of the position and movements of the detector elements, subject to underwater currents. Acoustic data are continuously sampled at 195.3 kHz and streamed to shore for analysis. The time of arrival of acoustic signals is used to measure the distance between APS elements. This contribution presents the results and performance of a position and orientation reconstruction system based on multilateration, along with results for ARCA.

Název v anglickém jazyce

The KM3NeT/ARCA: Status and results of the Acoustic Positioning System

Popis výsledku anglicky

The KM3NeT (Cubic Kilometre Neutrino Telescope) Collaboration is currently building two underwater neutrino detectors: ORCA (Oscillation Research with Cosmics in the Abysses) located offshore Toulon, France, at 2500 m water depth, and ARCA (Astronomy Research with Cosmics in the Abysses) offshore Capo Passero, Italy, at 3500 m water depth. The basic element of the detector is the DOM (Digital Optical Module), housing 31 photomultiplier tubes (PMTs), capable of recording single photon arrival time and charge, to be sent to shore for triggering, filtering, and data analysis. A vertical line of 18 DOMs forms a Detection Unit (DU): about 700 m long in ARCA, and about 200 m long in ORCA. A custom Acoustic Positioning System (APS) was designed and developed by the KM3NeT collaboration to obtain an accuracy of a few centimeters in the determination of the position of each DOM. In the case of KM3NeT-ARCA, the subject of this paper, this is required in order to be able to reconstruct neutrino directions with the desired pointing resolution. Building upon the White Rabbit time synchronization, the APS operates as a phased array of several thousand digital acoustic receivers, hosted in all DOMs and the anchors of the DUs. Each receiver records acoustic signals emitted by a long baseline of georeferenced acoustic emitters anchored on the seafloor. The APS allows constant monitoring of the position and movements of the detector elements, subject to underwater currents. Acoustic data are continuously sampled at 195.3 kHz and streamed to shore for analysis. The time of arrival of acoustic signals is used to measure the distance between APS elements. This contribution presents the results and performance of a position and orientation reconstruction system based on multilateration, along with results for ARCA.

Druh

D - Stať ve sborníku

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

<a href="/cs/project/LM2023063" target="_blank" >LM2023063: Podzemní laboratoř LSM - účast České republiky</a><br>

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Rok uplatnění

2025

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název statě ve sborníku

39th International Cosmic Ray Conference (ICRC2025)

ISBN

—

ISSN

1824-8039

e-ISSN

—

Počet stran výsledku

11

Strana od-do

1-11

Název nakladatele

PoS - Proceedings of Science, Sissa Medialab srl

Místo vydání

Trieste

Místo konání akce

Geneva

Datum konání akce

14. 7. 2025

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

—