KM3NeT broadcast optical data transport system

S. Aiello; A. Albert; S. Alves Garre; Z. Aly; A. Ambrosone; F. Ameli; M. Andre; M. Anghinolfi; M. Anguita; M. Ardid; S. Ardid; J. Aublin; C. Bagatelas; L. Bailly-Salins; B. Baret; S. Basegmez du Pree; Y. Becherini; M. Bendahman; F. Benfenati; E. Berbee; V. Bertin; S. Biagi; M. Boettcher; M. Bou Cabo; J. Boumaaza; M. Bouta; M. Bouwhuis; C. Bozza; H. Branzas; R. Bruijn; J. Brunner; R. Bruno; E. Buis; R. Buompane; J. Busto; B. Caiffi; D. Calvo; S. Campion; A. Capone; F. Carenini; V. Carretero; P. Castaldi; S. Celli; L. Cerisy; M. Chabab; N. Chau; A. Chen; R. Cherkaoui El Moursli; S. Cherubini; Miroslav Filipovic; null et al.

doi:10.1088/1748-0221/18/02/T02001

KM3NeT broadcast optical data transport system

S. Aiello, A. Albert, S. Alves Garre, Z. Aly, A. Ambrosone, F. Ameli, M. Andre, M. Anghinolfi, M. Anguita, M. Ardid, S. Ardid, J. Aublin, C. Bagatelas, L. Bailly-Salins, B. Baret, S. Basegmez du Pree, Y. Becherini, M. Bendahman, F. Benfenati, E. BerbeeV. Bertin, S. Biagi, M. Boettcher, M. Bou Cabo, J. Boumaaza, M. Bouta, M. Bouwhuis, C. Bozza, H. Branzas, R. Bruijn, J. Brunner, R. Bruno, E. Buis, R. Buompane, J. Busto, B. Caiffi, D. Calvo, S. Campion, A. Capone, F. Carenini, V. Carretero, P. Castaldi, S. Celli, L. Cerisy, M. Chabab, N. Chau, A. Chen, R. Cherkaoui El Moursli, S. Cherubini, Miroslav Filipovic, et al.

Western Sydney University

Research output: Contribution to journal › Article › peer-review

Abstract

The optical data transport system of the KM3NeT neutrino telescope at the bottom of the Mediterranean Sea will provide more than 6000 optical modules in the detector arrays with a point-to-point optical connection to the control stations onshore. The ARCA and ORCA detectors of KM3NeT are being installed at a depth of about 3500 m and 2500 m, respectively and their distance to the control stations is about 100 kilometers and 40 kilometers. In particular, the two detectors are optimised for the detection of cosmic neutrinos with energies above about 1 TeV (ARCA) and for the detection of atmospheric neutrinos with energies in the range 1 GeV-1 TeV (ORCA). The expected maximum data rate is 200 Mbps per optical module. The implemented optical data transport system matches the layouts of the networks of electro-optical cables and junction boxes in the deep sea. For efficient use of the fibres in the system the technology of Dense Wavelength Division Multiplexing is applied. The performance of the optical system in terms of measured bit error rates, optical budget are presented. The next steps in the implementation of the system are also discussed.

Original language	English
Article number	T02001
Number of pages	21
Journal	Journal of Instrumentation
Volume	18
Issue number	2
DOIs	https://doi.org/10.1088/1748-0221/18/02/T02001
Publication status	Published - 1 Feb 2023

Bibliographical note

Publisher Copyright:
© 2023 The Author(s)

Open Access - Access Right Statement

2023 The Author(s). Published by IOP Publishing Ltd on behalf of Sissa Medialab. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence (https://creativecommons.org/licenses/by/4.0/). Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.

Keywords

Large detector systems for particle and astroparticle physics
Cherenkov detectors
Optics
Data Processing

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10.1088/1748-0221/18/02/T02001

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Aiello, S., Albert, A., Alves Garre, S., Aly, Z., Ambrosone, A., Ameli, F., Andre, M., Anghinolfi, M., Anguita, M., Ardid, M., Ardid, S., Aublin, J., Bagatelas, C., Bailly-Salins, L., Baret, B., Basegmez du Pree, S., Becherini, Y., Bendahman, M., Benfenati, F., ... et al. (2023). KM3NeT broadcast optical data transport system. Journal of Instrumentation, 18(2), Article T02001. https://doi.org/10.1088/1748-0221/18/02/T02001

@article{b351b33c84354e978e16fdbb598c17af,

title = "KM3NeT broadcast optical data transport system",

abstract = "The optical data transport system of the KM3NeT neutrino telescope at the bottom of the Mediterranean Sea will provide more than 6000 optical modules in the detector arrays with a point-to-point optical connection to the control stations onshore. The ARCA and ORCA detectors of KM3NeT are being installed at a depth of about 3500 m and 2500 m, respectively and their distance to the control stations is about 100 kilometers and 40 kilometers. In particular, the two detectors are optimised for the detection of cosmic neutrinos with energies above about 1 TeV (ARCA) and for the detection of atmospheric neutrinos with energies in the range 1 GeV-1 TeV (ORCA). The expected maximum data rate is 200 Mbps per optical module. The implemented optical data transport system matches the layouts of the networks of electro-optical cables and junction boxes in the deep sea. For efficient use of the fibres in the system the technology of Dense Wavelength Division Multiplexing is applied. The performance of the optical system in terms of measured bit error rates, optical budget are presented. The next steps in the implementation of the system are also discussed.",

keywords = "Large detector systems for particle and astroparticle physics, Cherenkov detectors, Optics, Data Processing",

author = "S. Aiello and A. Albert and {Alves Garre}, S. and Z. Aly and A. Ambrosone and F. Ameli and M. Andre and M. Anghinolfi and M. Anguita and M. Ardid and S. Ardid and J. Aublin and C. Bagatelas and L. Bailly-Salins and B. Baret and {Basegmez du Pree}, S. and Y. Becherini and M. Bendahman and F. Benfenati and E. Berbee and V. Bertin and S. Biagi and M. Boettcher and {Bou Cabo}, M. and J. Boumaaza and M. Bouta and M. Bouwhuis and C. Bozza and H. Branzas and R. Bruijn and J. Brunner and R. Bruno and E. Buis and R. Buompane and J. Busto and B. Caiffi and D. Calvo and S. Campion and A. Capone and F. Carenini and V. Carretero and P. Castaldi and S. Celli and L. Cerisy and M. Chabab and N. Chau and A. Chen and {Cherkaoui El Moursli}, R. and S. Cherubini and Miroslav Filipovic and {et al.}",

note = "Publisher Copyright: {\textcopyright} 2023 The Author(s)",

year = "2023",

month = feb,

day = "1",

doi = "10.1088/1748-0221/18/02/T02001",

language = "English",

volume = "18",

journal = "Journal of Instrumentation",

issn = "1748-0221",

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Aiello, S, Albert, A, Alves Garre, S, Aly, Z, Ambrosone, A, Ameli, F, Andre, M, Anghinolfi, M, Anguita, M, Ardid, M, Ardid, S, Aublin, J, Bagatelas, C, Bailly-Salins, L, Baret, B, Basegmez du Pree, S, Becherini, Y, Bendahman, M, Benfenati, F, Berbee, E, Bertin, V, Biagi, S, Boettcher, M, Bou Cabo, M, Boumaaza, J, Bouta, M, Bouwhuis, M, Bozza, C, Branzas, H, Bruijn, R, Brunner, J, Bruno, R, Buis, E, Buompane, R, Busto, J, Caiffi, B, Calvo, D, Campion, S, Capone, A, Carenini, F, Carretero, V, Castaldi, P, Celli, S, Cerisy, L, Chabab, M, Chau, N, Chen, A, Cherkaoui El Moursli, R, Cherubini, S, Filipovic, M & et al. 2023, 'KM3NeT broadcast optical data transport system', Journal of Instrumentation, vol. 18, no. 2, T02001. https://doi.org/10.1088/1748-0221/18/02/T02001

TY - JOUR

T1 - KM3NeT broadcast optical data transport system

AU - Aiello, S.

AU - Albert, A.

AU - Alves Garre, S.

AU - Aly, Z.

AU - Ambrosone, A.

AU - Ameli, F.

AU - Andre, M.

AU - Anghinolfi, M.

AU - Anguita, M.

AU - Ardid, M.

AU - Ardid, S.

AU - Aublin, J.

AU - Bagatelas, C.

AU - Bailly-Salins, L.

AU - Baret, B.

AU - Basegmez du Pree, S.

AU - Becherini, Y.

AU - Bendahman, M.

AU - Benfenati, F.

AU - Berbee, E.

AU - Bertin, V.

AU - Biagi, S.

AU - Boettcher, M.

AU - Bou Cabo, M.

AU - Boumaaza, J.

AU - Bouta, M.

AU - Bouwhuis, M.

AU - Bozza, C.

AU - Branzas, H.

AU - Bruijn, R.

AU - Brunner, J.

AU - Bruno, R.

AU - Buis, E.

AU - Buompane, R.

AU - Busto, J.

AU - Caiffi, B.

AU - Calvo, D.

AU - Campion, S.

AU - Capone, A.

AU - Carenini, F.

AU - Carretero, V.

AU - Castaldi, P.

AU - Celli, S.

AU - Cerisy, L.

AU - Chabab, M.

AU - Chau, N.

AU - Chen, A.

AU - Cherkaoui El Moursli, R.

AU - Cherubini, S.

AU - Filipovic, Miroslav

AU - et al., null

PY - 2023/2/1

Y1 - 2023/2/1

N2 - The optical data transport system of the KM3NeT neutrino telescope at the bottom of the Mediterranean Sea will provide more than 6000 optical modules in the detector arrays with a point-to-point optical connection to the control stations onshore. The ARCA and ORCA detectors of KM3NeT are being installed at a depth of about 3500 m and 2500 m, respectively and their distance to the control stations is about 100 kilometers and 40 kilometers. In particular, the two detectors are optimised for the detection of cosmic neutrinos with energies above about 1 TeV (ARCA) and for the detection of atmospheric neutrinos with energies in the range 1 GeV-1 TeV (ORCA). The expected maximum data rate is 200 Mbps per optical module. The implemented optical data transport system matches the layouts of the networks of electro-optical cables and junction boxes in the deep sea. For efficient use of the fibres in the system the technology of Dense Wavelength Division Multiplexing is applied. The performance of the optical system in terms of measured bit error rates, optical budget are presented. The next steps in the implementation of the system are also discussed.

AB - The optical data transport system of the KM3NeT neutrino telescope at the bottom of the Mediterranean Sea will provide more than 6000 optical modules in the detector arrays with a point-to-point optical connection to the control stations onshore. The ARCA and ORCA detectors of KM3NeT are being installed at a depth of about 3500 m and 2500 m, respectively and their distance to the control stations is about 100 kilometers and 40 kilometers. In particular, the two detectors are optimised for the detection of cosmic neutrinos with energies above about 1 TeV (ARCA) and for the detection of atmospheric neutrinos with energies in the range 1 GeV-1 TeV (ORCA). The expected maximum data rate is 200 Mbps per optical module. The implemented optical data transport system matches the layouts of the networks of electro-optical cables and junction boxes in the deep sea. For efficient use of the fibres in the system the technology of Dense Wavelength Division Multiplexing is applied. The performance of the optical system in terms of measured bit error rates, optical budget are presented. The next steps in the implementation of the system are also discussed.

KW - Large detector systems for particle and astroparticle physics

KW - Cherenkov detectors

KW - Optics

KW - Data Processing

UR - https://hdl.handle.net/1959.7/uws:74391

UR - http://www.scopus.com/inward/record.url?scp=85147796736&partnerID=8YFLogxK

U2 - 10.1088/1748-0221/18/02/T02001

DO - 10.1088/1748-0221/18/02/T02001

M3 - Article

SN - 1748-0221

VL - 18

JO - Journal of Instrumentation

JF - Journal of Instrumentation

IS - 2

M1 - T02001

ER -

KM3NeT broadcast optical data transport system

Abstract

Bibliographical note

Open Access - Access Right Statement

Keywords

Access to Document

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