The positioning system of the ANTARES Neutrino Telescope

S. Adrián-Martínez; M. Ageron; A. Aguilar; I. Al Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; C. Assis Jesus; T. Astraatmadja; J. J. Aubert; B. Baret; S. Basa; V. Bertin; S. Biagi; A. Bigi; C. Bigongiari; C. Bogazzi; M. Bou-Cabo; B. Bouhou; C. Bouwhuis; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Cârloganu; G. Carminati; J. Carr; S. Cecchini; Z. Charif; Ph Charvis; T. Chiarusi; M. Circella; R. Coniglione; H. Costantini; P. Coyle; C. Curtil; G. De Bonis; P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; T. Eberl; U. Emanuele; A. Enzenhöfer; J. P. Ernenwein; S. Escoffier; P. Fermani; M. Ferri; V. Flaminio; F. Folger; U. Fritsch; J. L. Fuda; S. Galatà; P. Gay; G. Giacomelli; V. Giordano; P. Gómez-González; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. Van Haren; J. Hartman; J. Heijboer; Y. Hello; J. Hernández-Rey; B. Herold; J. Höl; C. Hsu; M. De Jong; M. Kadler; O. Kalekin; A. Kappes; U. Katz; O. Kavatsyuk; P. Keller; P. Kooijman; C. Kopper; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; P. Lamare; G. Larosa; D. Lattuada; D. Lefèvre; A. Le Van Suu; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; S. Mangano; M. Marcelin; A. Margiotta; A. Martínez-Mora; A. Meli; T. Montaruli; L. Moscoso; H. Motz; M. Neff; E. Nezri; V. Niess; D. Palioselitis; E. Pavalaş; K. Payet; P. Payre; J. Petrovic; P. Piattelli; N. Picot-Clemente; V. Popa; T. Pradier; E. Presani; C. Racca; D. Real; C. Reed; G. Riccobene; C. Richardt; R. Richter; C. Rivière; A. Robert; K. Roensch; A. Rostovtsev; J. Ruiz-Rivas; M. Rujoiu; V. Russo; F. Salesa; E. Samtleben; F. Schöck; J. P. Schuller; F. Schüssler; T. Seitz; R. Shanidze; F. Simeone; A. Spies; M. Spurio; M. Steijger; Th Stolarczyk; A. Sánchez-Losa; M. Taiuti; C. Tamburini; S. Toscano; B. Vallage; V. Van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; S. Wagner; G. Wijnker; J. Wilms; E. De Wolf; H. Yepes; D. Zaborov; D. Zornoza; J. Zúñiga

doi:10.1088/1748-0221/7/08/T08002

The positioning system of the ANTARES Neutrino Telescope

S. Adrián-Martínez, M. Ageron, A. Aguilar, I. Al Samarai, A. Albert, M. André, M. Anghinolfi, G. Anton, S. Anvar, M. Ardid, C. Assis Jesus, T. Astraatmadja, J. J. Aubert, B. Baret, S. Basa, V. Bertin, S. Biagi, A. Bigi, C. Bigongiari, C. BogazziM. Bou-Cabo, B. Bouhou, C. Bouwhuis, J. Brunner, J. Busto, F. Camarena, A. Capone, C. Cârloganu, G. Carminati, J. Carr, S. Cecchini, Z. Charif, Ph Charvis, T. Chiarusi, M. Circella, R. Coniglione, H. Costantini, P. Coyle, C. Curtil, G. De Bonis, P. Decowski, I. Dekeyser, A. Deschamps, C. Distefano, C. Donzaud, D. Dornic, Q. Dorosti, D. Drouhin, T. Eberl, U. Emanuele, A. Enzenhöfer, J. P. Ernenwein, S. Escoffier, P. Fermani, M. Ferri, V. Flaminio, F. Folger, U. Fritsch, J. L. Fuda, S. Galatà, P. Gay, G. Giacomelli, V. Giordano, P. Gómez-González, K. Graf, G. Guillard, G. Halladjian, G. Hallewell, H. Van Haren, J. Hartman, J. Heijboer, Y. Hello, J. Hernández-Rey, B. Herold, J. Höl^*, C. Hsu, M. De Jong, M. Kadler, O. Kalekin, A. Kappes, U. Katz, O. Kavatsyuk, P. Keller, P. Kooijman, C. Kopper, A. Kouchner, I. Kreykenbohm, V. Kulikovskiy, R. Lahmann, P. Lamare, G. Larosa, D. Lattuada, D. Lefèvre, A. Le Van Suu, G. Lim, D. Lo Presti, H. Loehner, S. Loucatos, S. Mangano, M. Marcelin, A. Margiotta, A. Martínez-Mora, A. Meli, T. Montaruli, L. Moscoso, H. Motz, M. Neff, E. Nezri, V. Niess, D. Palioselitis, E. Pavalaş, K. Payet, P. Payre, J. Petrovic, P. Piattelli, N. Picot-Clemente, V. Popa, T. Pradier, E. Presani, C. Racca, D. Real, C. Reed, G. Riccobene, C. Richardt, R. Richter, C. Rivière, A. Robert, K. Roensch, A. Rostovtsev, J. Ruiz-Rivas, M. Rujoiu, V. Russo, F. Salesa, E. Samtleben, F. Schöck, J. P. Schuller, F. Schüssler, T. Seitz, R. Shanidze, F. Simeone, A. Spies, M. Spurio, M. Steijger, Th Stolarczyk, A. Sánchez-Losa, M. Taiuti, C. Tamburini, S. Toscano, B. Vallage, V. Van Elewyck, G. Vannoni, M. Vecchi, P. Vernin, S. Wagner, G. Wijnker, J. Wilms, E. De Wolf, H. Yepes, D. Zaborov, D. Zornoza, J. Zúñiga

^*この研究の対応する著者

研究成果: Review article › 査読

53 被引用数 (Scopus)

抄録

The ANTARES neutrino telescope, located 40 km off the coast of Toulon in the Mediterranean Sea at a mooring depth of about 2475 m, consists of twelve detection lines equipped typically with 25 storeys. Every storey carries three optical modules that detect Cherenkov light induced by charged secondary particles (typically muons) coming from neutrino interactions. As these lines are flexible structures fixed to the sea bed and held taut by a buoy, sea currents cause the lines to move and the storeys to rotate. The knowledge of the position of the optical modules with a precision better than 10 cm is essential for a good reconstruction of particle tracks. In this paper the ANTARES positioning system is described. It consists of an acoustic positioning system, for distance triangulation, and a compass-tiltmeter system, for the measurement of the orientation and inclination of the storeys. Necessary corrections are discussed and the results of the detector alignment procedure are described.

本文言語	English
論文番号	T08002
ジャーナル	Journal of Instrumentation
巻	7
号	8
DOI	https://doi.org/10.1088/1748-0221/7/08/T08002
出版ステータス	Published - 2012 8月
外部発表	はい

ASJC Scopus subject areas

器械工学
数理物理学

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10.1088/1748-0221/7/08/T08002

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Adrián-Martínez, S., Ageron, M., Aguilar, A., Al Samarai, I., Albert, A., André, M., Anghinolfi, M., Anton, G., Anvar, S., Ardid, M., Assis Jesus, C., Astraatmadja, T., Aubert, J. J., Baret, B., Basa, S., Bertin, V., Biagi, S., Bigi, A., Bigongiari, C., ... Zúñiga, J. (2012). The positioning system of the ANTARES Neutrino Telescope. Journal of Instrumentation, 7(8), [T08002]. https://doi.org/10.1088/1748-0221/7/08/T08002

Adrián-Martínez, S, Ageron, M, Aguilar, A, Al Samarai, I, Albert, A, André, M, Anghinolfi, M, Anton, G, Anvar, S, Ardid, M, Assis Jesus, C, Astraatmadja, T, Aubert, JJ, Baret, B, Basa, S, Bertin, V, Biagi, S, Bigi, A, Bigongiari, C, Bogazzi, C, Bou-Cabo, M, Bouhou, B, Bouwhuis, C, Brunner, J, Busto, J, Camarena, F, Capone, A, Cârloganu, C, Carminati, G, Carr, J, Cecchini, S, Charif, Z, Charvis, P, Chiarusi, T, Circella, M, Coniglione, R, Costantini, H, Coyle, P, Curtil, C, De Bonis, G, Decowski, P, Dekeyser, I, Deschamps, A, Distefano, C, Donzaud, C, Dornic, D, Dorosti, Q, Drouhin, D, Eberl, T, Emanuele, U, Enzenhöfer, A, Ernenwein, JP, Escoffier, S, Fermani, P, Ferri, M, Flaminio, V, Folger, F, Fritsch, U, Fuda, JL, Galatà, S, Gay, P, Giacomelli, G, Giordano, V, Gómez-González, P, Graf, K, Guillard, G, Halladjian, G, Hallewell, G, Van Haren, H, Hartman, J, Heijboer, J, Hello, Y, Hernández-Rey, J, Herold, B, Höl, J, Hsu, C, De Jong, M, Kadler, M, Kalekin, O, Kappes, A, Katz, U, Kavatsyuk, O, Keller, P, Kooijman, P, Kopper, C, Kouchner, A, Kreykenbohm, I, Kulikovskiy, V, Lahmann, R, Lamare, P, Larosa, G, Lattuada, D, Lefèvre, D, Le Van Suu, A, Lim, G, Lo Presti, D, Loehner, H, Loucatos, S, Mangano, S, Marcelin, M, Margiotta, A, Martínez-Mora, A, Meli, A, Montaruli, T, Moscoso, L, Motz, H, Neff, M, Nezri, E, Niess, V, Palioselitis, D, Pavalaş, E, Payet, K, Payre, P, Petrovic, J, Piattelli, P, Picot-Clemente, N, Popa, V, Pradier, T, Presani, E, Racca, C, Real, D, Reed, C, Riccobene, G, Richardt, C, Richter, R, Rivière, C, Robert, A, Roensch, K, Rostovtsev, A, Ruiz-Rivas, J, Rujoiu, M, Russo, V, Salesa, F, Samtleben, E, Schöck, F, Schuller, JP, Schüssler, F, Seitz, T, Shanidze, R, Simeone, F, Spies, A, Spurio, M, Steijger, M, Stolarczyk, T, Sánchez-Losa, A, Taiuti, M, Tamburini, C, Toscano, S, Vallage, B, Van Elewyck, V, Vannoni, G, Vecchi, M, Vernin, P, Wagner, S, Wijnker, G, Wilms, J, De Wolf, E, Yepes, H, Zaborov, D, Zornoza, D & Zúñiga, J 2012, 'The positioning system of the ANTARES Neutrino Telescope', Journal of Instrumentation, vol. 7, no. 8, T08002. https://doi.org/10.1088/1748-0221/7/08/T08002

@article{c94092a9de2244d6b70ea162e0f15919,

title = "The positioning system of the ANTARES Neutrino Telescope",

abstract = "The ANTARES neutrino telescope, located 40 km off the coast of Toulon in the Mediterranean Sea at a mooring depth of about 2475 m, consists of twelve detection lines equipped typically with 25 storeys. Every storey carries three optical modules that detect Cherenkov light induced by charged secondary particles (typically muons) coming from neutrino interactions. As these lines are flexible structures fixed to the sea bed and held taut by a buoy, sea currents cause the lines to move and the storeys to rotate. The knowledge of the position of the optical modules with a precision better than 10 cm is essential for a good reconstruction of particle tracks. In this paper the ANTARES positioning system is described. It consists of an acoustic positioning system, for distance triangulation, and a compass-tiltmeter system, for the measurement of the orientation and inclination of the storeys. Necessary corrections are discussed and the results of the detector alignment procedure are described.",

keywords = "Detector alignment and calibration methods (lasers, Detector control systems (detector and experiment monitoring and slow-control systems, Detector modelling and simulations II (electric fields, Timing detectors, algorithms, architecture, charge transport, databases), electron emission, etc), hardware, multiplication and induction, particle-beams), pulse formation, sources",

author = "S. Adri{\'a}n-Mart{\'i}nez and M. Ageron and A. Aguilar and {Al Samarai}, I. and A. Albert and M. Andr{\'e} and M. Anghinolfi and G. Anton and S. Anvar and M. Ardid and {Assis Jesus}, C. and T. Astraatmadja and Aubert, {J. J.} and B. Baret and S. Basa and V. Bertin and S. Biagi and A. Bigi and C. Bigongiari and C. Bogazzi and M. Bou-Cabo and B. Bouhou and C. Bouwhuis and J. Brunner and J. Busto and F. Camarena and A. Capone and C. C{\^a}rloganu and G. Carminati and J. Carr and S. Cecchini and Z. Charif and Ph Charvis and T. Chiarusi and M. Circella and R. Coniglione and H. Costantini and P. Coyle and C. Curtil and {De Bonis}, G. and P. Decowski and I. Dekeyser and A. Deschamps and C. Distefano and C. Donzaud and D. Dornic and Q. Dorosti and D. Drouhin and T. Eberl and U. Emanuele and A. Enzenh{\"o}fer and Ernenwein, {J. P.} and S. Escoffier and P. Fermani and M. Ferri and V. Flaminio and F. Folger and U. Fritsch and Fuda, {J. L.} and S. Galat{\`a} and P. Gay and G. Giacomelli and V. Giordano and P. G{\'o}mez-Gonz{\'a}lez and K. Graf and G. Guillard and G. Halladjian and G. Hallewell and {Van Haren}, H. and J. Hartman and J. Heijboer and Y. Hello and J. Hern{\'a}ndez-Rey and B. Herold and J. H{\"o}l and C. Hsu and {De Jong}, M. and M. Kadler and O. Kalekin and A. Kappes and U. Katz and O. Kavatsyuk and P. Keller and P. Kooijman and C. Kopper and A. Kouchner and I. Kreykenbohm and V. Kulikovskiy and R. Lahmann and P. Lamare and G. Larosa and D. Lattuada and D. Lef{\`e}vre and {Le Van Suu}, A. and G. Lim and {Lo Presti}, D. and H. Loehner and S. Loucatos and S. Mangano and M. Marcelin and A. Margiotta and A. Mart{\'i}nez-Mora and A. Meli and T. Montaruli and L. Moscoso and H. Motz and M. Neff and E. Nezri and V. Niess and D. Palioselitis and E. Pavala{\c s} and K. Payet and P. Payre and J. Petrovic and P. Piattelli and N. Picot-Clemente and V. Popa and T. Pradier and E. Presani and C. Racca and D. Real and C. Reed and G. Riccobene and C. Richardt and R. Richter and C. Rivi{\`e}re and A. Robert and K. Roensch and A. Rostovtsev and J. Ruiz-Rivas and M. Rujoiu and V. Russo and F. Salesa and E. Samtleben and F. Sch{\"o}ck and Schuller, {J. P.} and F. Sch{\"u}ssler and T. Seitz and R. Shanidze and F. Simeone and A. Spies and M. Spurio and M. Steijger and Th Stolarczyk and A. S{\'a}nchez-Losa and M. Taiuti and C. Tamburini and S. Toscano and B. Vallage and {Van Elewyck}, V. and G. Vannoni and M. Vecchi and P. Vernin and S. Wagner and G. Wijnker and J. Wilms and {De Wolf}, E. and H. Yepes and D. Zaborov and D. Zornoza and J. Z{\'u}{\~n}iga",

year = "2012",

month = aug,

doi = "10.1088/1748-0221/7/08/T08002",

language = "English",

volume = "7",

journal = "Journal of Instrumentation",

issn = "1748-0221",

publisher = "IOP Publishing Ltd.",

number = "8",

}

TY - JOUR

T1 - The positioning system of the ANTARES Neutrino Telescope

AU - Adrián-Martínez, S.

AU - Ageron, M.

AU - Aguilar, A.

AU - Al Samarai, I.

AU - Albert, A.

AU - André, M.

AU - Anghinolfi, M.

AU - Anton, G.

AU - Anvar, S.

AU - Ardid, M.

AU - Assis Jesus, C.

AU - Astraatmadja, T.

AU - Aubert, J. J.

AU - Baret, B.

AU - Basa, S.

AU - Bertin, V.

AU - Biagi, S.

AU - Bigi, A.

AU - Bigongiari, C.

AU - Bogazzi, C.

AU - Bou-Cabo, M.

AU - Bouhou, B.

AU - Bouwhuis, C.

AU - Brunner, J.

AU - Busto, J.

AU - Camarena, F.

AU - Capone, A.

AU - Cârloganu, C.

AU - Carminati, G.

AU - Carr, J.

AU - Cecchini, S.

AU - Charif, Z.

AU - Charvis, Ph

AU - Chiarusi, T.

AU - Circella, M.

AU - Coniglione, R.

AU - Costantini, H.

AU - Coyle, P.

AU - Curtil, C.

AU - De Bonis, G.

AU - Decowski, P.

AU - Dekeyser, I.

AU - Deschamps, A.

AU - Distefano, C.

AU - Donzaud, C.

AU - Dornic, D.

AU - Dorosti, Q.

AU - Drouhin, D.

AU - Eberl, T.

AU - Emanuele, U.

AU - Enzenhöfer, A.

AU - Ernenwein, J. P.

AU - Escoffier, S.

AU - Fermani, P.

AU - Ferri, M.

AU - Flaminio, V.

AU - Folger, F.

AU - Fritsch, U.

AU - Fuda, J. L.

AU - Galatà, S.

AU - Gay, P.

AU - Giacomelli, G.

AU - Giordano, V.

AU - Gómez-González, P.

AU - Graf, K.

AU - Guillard, G.

AU - Halladjian, G.

AU - Hallewell, G.

AU - Van Haren, H.

AU - Hartman, J.

AU - Heijboer, J.

AU - Hello, Y.

AU - Hernández-Rey, J.

AU - Herold, B.

AU - Höl, J.

AU - Hsu, C.

AU - De Jong, M.

AU - Kadler, M.

AU - Kalekin, O.

AU - Kappes, A.

AU - Katz, U.

AU - Kavatsyuk, O.

AU - Keller, P.

AU - Kooijman, P.

AU - Kopper, C.

AU - Kouchner, A.

AU - Kreykenbohm, I.

AU - Kulikovskiy, V.

AU - Lahmann, R.

AU - Lamare, P.

AU - Larosa, G.

AU - Lattuada, D.

AU - Lefèvre, D.

AU - Le Van Suu, A.

AU - Lim, G.

AU - Lo Presti, D.

AU - Loehner, H.

AU - Loucatos, S.

AU - Mangano, S.

AU - Marcelin, M.

AU - Margiotta, A.

AU - Martínez-Mora, A.

AU - Meli, A.

AU - Montaruli, T.

AU - Moscoso, L.

AU - Motz, H.

AU - Neff, M.

AU - Nezri, E.

AU - Niess, V.

AU - Palioselitis, D.

AU - Pavalaş, E.

AU - Payet, K.

AU - Payre, P.

AU - Petrovic, J.

AU - Piattelli, P.

AU - Picot-Clemente, N.

AU - Popa, V.

AU - Pradier, T.

AU - Presani, E.

AU - Racca, C.

AU - Real, D.

AU - Reed, C.

AU - Riccobene, G.

AU - Richardt, C.

AU - Richter, R.

AU - Rivière, C.

AU - Robert, A.

AU - Roensch, K.

AU - Rostovtsev, A.

AU - Ruiz-Rivas, J.

AU - Rujoiu, M.

AU - Russo, V.

AU - Salesa, F.

AU - Samtleben, E.

AU - Schöck, F.

AU - Schuller, J. P.

AU - Schüssler, F.

AU - Seitz, T.

AU - Shanidze, R.

AU - Simeone, F.

AU - Spies, A.

AU - Spurio, M.

AU - Steijger, M.

AU - Stolarczyk, Th

AU - Sánchez-Losa, A.

AU - Taiuti, M.

AU - Tamburini, C.

AU - Toscano, S.

AU - Vallage, B.

AU - Van Elewyck, V.

AU - Vannoni, G.

AU - Vecchi, M.

AU - Vernin, P.

AU - Wagner, S.

AU - Wijnker, G.

AU - Wilms, J.

AU - De Wolf, E.

AU - Yepes, H.

AU - Zaborov, D.

AU - Zornoza, D.

AU - Zúñiga, J.

PY - 2012/8

Y1 - 2012/8

N2 - The ANTARES neutrino telescope, located 40 km off the coast of Toulon in the Mediterranean Sea at a mooring depth of about 2475 m, consists of twelve detection lines equipped typically with 25 storeys. Every storey carries three optical modules that detect Cherenkov light induced by charged secondary particles (typically muons) coming from neutrino interactions. As these lines are flexible structures fixed to the sea bed and held taut by a buoy, sea currents cause the lines to move and the storeys to rotate. The knowledge of the position of the optical modules with a precision better than 10 cm is essential for a good reconstruction of particle tracks. In this paper the ANTARES positioning system is described. It consists of an acoustic positioning system, for distance triangulation, and a compass-tiltmeter system, for the measurement of the orientation and inclination of the storeys. Necessary corrections are discussed and the results of the detector alignment procedure are described.

AB - The ANTARES neutrino telescope, located 40 km off the coast of Toulon in the Mediterranean Sea at a mooring depth of about 2475 m, consists of twelve detection lines equipped typically with 25 storeys. Every storey carries three optical modules that detect Cherenkov light induced by charged secondary particles (typically muons) coming from neutrino interactions. As these lines are flexible structures fixed to the sea bed and held taut by a buoy, sea currents cause the lines to move and the storeys to rotate. The knowledge of the position of the optical modules with a precision better than 10 cm is essential for a good reconstruction of particle tracks. In this paper the ANTARES positioning system is described. It consists of an acoustic positioning system, for distance triangulation, and a compass-tiltmeter system, for the measurement of the orientation and inclination of the storeys. Necessary corrections are discussed and the results of the detector alignment procedure are described.

KW - Detector alignment and calibration methods (lasers

KW - Detector control systems (detector and experiment monitoring and slow-control systems

KW - Detector modelling and simulations II (electric fields

KW - Timing detectors

KW - algorithms

KW - architecture

KW - charge transport

KW - databases)

KW - electron emission

KW - etc)

KW - hardware

KW - multiplication and induction

KW - particle-beams)

KW - pulse formation

KW - sources

UR - http://www.scopus.com/inward/record.url?scp=84865267586&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84865267586&partnerID=8YFLogxK

U2 - 10.1088/1748-0221/7/08/T08002

DO - 10.1088/1748-0221/7/08/T08002

M3 - Review article

AN - SCOPUS:84865267586

SN - 1748-0221

VL - 7

JO - Journal of Instrumentation

JF - Journal of Instrumentation

IS - 8

M1 - T08002

ER -

The positioning system of the ANTARES Neutrino Telescope

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ASJC Scopus subject areas

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