抄録
The AMADEUS (ANTARES Modules for the Acoustic Detection Under the Sea) system which is described in this article aims at the investigation of techniques for acoustic detection of neutrinos in the deep sea. It is integrated into the ANTARES neutrino telescope in the Mediterranean Sea. Its acoustic sensors, installed at water depths between 2050 and 2300 m, employ piezo-electric elements for the broad-band recording of signals with frequencies ranging up to 125 kHz. The typical sensitivity of the sensors is around -145 dB re 1 V/μPa (including preamplifier). Completed in May 2008, AMADEUS consists of six "acoustic clusters", each comprising six acoustic sensors that are arranged at distances of roughly 1 m from each other. Two vertical mechanical structures (so-called lines) of the ANTARES detector host three acoustic clusters each. Spacings between the clusters range from 14.5 to 340 m. Each cluster contains custom-designed electronics boards to amplify and digitise the acoustic signals from the sensors. An on-shore computer cluster is used to process and filter the data stream and store the selected events. The daily volume of recorded data is about 10 GB. The system is operating continuously and automatically, requiring only little human intervention. AMADEUS allows for extensive studies of both transient signals and ambient noise in the deep sea, as well as signal correlations on several length scales and localisation of acoustic point sources. Thus the system is excellently suited to assess the background conditions for the measurement of the bipolar pulses expected to originate from neutrino interactions.
| 本文言語 | English |
|---|---|
| ページ（範囲） | 128-143 |
| ページ数 | 16 |
| ジャーナル | Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |
| 巻 | 626-627 |
| 号 | 1 |
| DOI | |
| 出版ステータス | Published - 2011 |
| 外部発表 | はい |
ASJC Scopus subject areas
- 核物理学および高エネルギー物理学
- 器械工学
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AMADEUS the acoustic neutrino detection test system of the ANTARES deep-sea neutrino telescope. / Aguilar, J. A.; Al Samarai, I.; Albert, A.; Anghinolfi, M.; Anton, G.; Anvar, S.; Ardid, M.; Assis Jesus, A. C.; Astraatmadja, T.; Aubert, J. J.; Auer, R.; Barbarito, E.; Baret, B.; Basa, S.; Bazzotti, M.; Bertin, V.; Biagi, S.; Bigongiari, C.; Bou-Cabo, M.; Bouwhuis, M. C.; Brown, A.; Brunner, J.; Busto, J.; Camarena, F.; Capone, A.; Cârloganu, C.; Carminati, G.; Carr, J.; Cassano, B.; Castorina, E.; Cavasinni, V.; Cecchini, S.; Ceres, A.; Charvis, Ph; Chiarusi, T.; Chon Sen, N.; Circella, M.; Coniglione, R.; Costantini, H.; Cottini, N.; Coyle, P.; Curtil, C.; De Bonis, G.; Decowski, M. P.; Dekeyser, I.; Deschamps, A.; Distefano, C.; Donzaud, C.; Dornic, D.; Drouhin, D.; Eberl, T.; Emanuele, U.; Ernenwein, J. P.; Escoffier, S.; Fehr, F.; Fiorello, C.; Flaminio, V.; Fritsch, U.; Fuda, J. L.; Gay, P.; Giacomelli, G.; Gómez-Gonázlez, J. P.; Graf, K.; Guillard, G.; Halladjian, G.; Hallewell, G.; Van Haren, H.; Heijboer, A. J.; Heine, E.; Hello, Y.; Hernndez-Rey, J. J.; Herold, B.; Ḧßl, J.; De Jong, M.; Kalantar-Nayestanaki, N.; Kalekin, O.; Kappes, A.; Katz, U.; Keller, P.; Kooijman, P.; Kopper, C.; Kouchner, A.; Kretschmer, W.; Lahmann, R.; Lamare, P.; Lambard, G.; Larosa, G.; Laschinsky, H.; Le Provost, H.; Lefèvre, D.; Lelaizant, G.; Lim, G.; Lo Presti, D.; Loehner, H.; Loucatos, S.; Louis, F.; Lucarelli, F.; Mangano, S.; Marcelin, M.; Margiotta, A.; Martinez-Mora, J. A.; Mazure, A.; Mongelli, M.; Montaruli, T.; Morganti, M.; Moscoso, L.; Motz, H.; Naumann, C.; Neff, M.; Ostasch, R.; Palioselitis, D.; Pǎvǎlaş, G. E.; Payre, P.; Petrovic, J.; Picot-Clemente, N.; Picq, C.; Popa, V.; Pradier, T.; Presani, E.; Racca, C.; Radu, A.; Reed, C.; Riccobene, G.; Richardt, C.; Rujoiu, M.; Ruppi, M.; Russo, G. V.; Salesa, F.; Sapienza, P.; Schöck, F.; Schuller, J. P.; Shanidze, R.; Simeone, F.; Spurio, M.; Steijger, J. J.M.; Stolarczyk, Th; Taiuti, M.; Tamburini, C.; Tasca, L.; Toscano, S.; Vallage, B.; Van Elewyck, V.; Vannoni, G.; Vecchi, M.; Vernin, P.; Wijnker, G.; De Wolf, E.; Yepes, H.; Zaborov, D.; Zornoza, J. D.; Zúñiga, J.
In: Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Vol. 626-627, No. 1, 2011, p. 128-143.研究成果: Article › 査読
}
TY - JOUR
T1 - AMADEUS the acoustic neutrino detection test system of the ANTARES deep-sea neutrino telescope
AU - Aguilar, J. A.
AU - Al Samarai, I.
AU - Albert, A.
AU - Anghinolfi, M.
AU - Anton, G.
AU - Anvar, S.
AU - Ardid, M.
AU - Assis Jesus, A. C.
AU - Astraatmadja, T.
AU - Aubert, J. J.
AU - Auer, R.
AU - Barbarito, E.
AU - Baret, B.
AU - Basa, S.
AU - Bazzotti, M.
AU - Bertin, V.
AU - Biagi, S.
AU - Bigongiari, C.
AU - Bou-Cabo, M.
AU - Bouwhuis, M. C.
AU - Brown, A.
AU - Brunner, J.
AU - Busto, J.
AU - Camarena, F.
AU - Capone, A.
AU - Cârloganu, C.
AU - Carminati, G.
AU - Carr, J.
AU - Cassano, B.
AU - Castorina, E.
AU - Cavasinni, V.
AU - Cecchini, S.
AU - Ceres, A.
AU - Charvis, Ph
AU - Chiarusi, T.
AU - Chon Sen, N.
AU - Circella, M.
AU - Coniglione, R.
AU - Costantini, H.
AU - Cottini, N.
AU - Coyle, P.
AU - Curtil, C.
AU - De Bonis, G.
AU - Decowski, M. P.
AU - Dekeyser, I.
AU - Deschamps, A.
AU - Distefano, C.
AU - Donzaud, C.
AU - Dornic, D.
AU - Drouhin, D.
AU - Eberl, T.
AU - Emanuele, U.
AU - Ernenwein, J. P.
AU - Escoffier, S.
AU - Fehr, F.
AU - Fiorello, C.
AU - Flaminio, V.
AU - Fritsch, U.
AU - Fuda, J. L.
AU - Gay, P.
AU - Giacomelli, G.
AU - Gómez-Gonázlez, J. P.
AU - Graf, K.
AU - Guillard, G.
AU - Halladjian, G.
AU - Hallewell, G.
AU - Van Haren, H.
AU - Heijboer, A. J.
AU - Heine, E.
AU - Hello, Y.
AU - Hernndez-Rey, J. J.
AU - Herold, B.
AU - Ḧßl, J.
AU - De Jong, M.
AU - Kalantar-Nayestanaki, N.
AU - Kalekin, O.
AU - Kappes, A.
AU - Katz, U.
AU - Keller, P.
AU - Kooijman, P.
AU - Kopper, C.
AU - Kouchner, A.
AU - Kretschmer, W.
AU - Lahmann, R.
AU - Lamare, P.
AU - Lambard, G.
AU - Larosa, G.
AU - Laschinsky, H.
AU - Le Provost, H.
AU - Lefèvre, D.
AU - Lelaizant, G.
AU - Lim, G.
AU - Lo Presti, D.
AU - Loehner, H.
AU - Loucatos, S.
AU - Louis, F.
AU - Lucarelli, F.
AU - Mangano, S.
AU - Marcelin, M.
AU - Margiotta, A.
AU - Martinez-Mora, J. A.
AU - Mazure, A.
AU - Mongelli, M.
AU - Montaruli, T.
AU - Morganti, M.
AU - Moscoso, L.
AU - Motz, H.
AU - Naumann, C.
AU - Neff, M.
AU - Ostasch, R.
AU - Palioselitis, D.
AU - Pǎvǎlaş, G. E.
AU - Payre, P.
AU - Petrovic, J.
AU - Picot-Clemente, N.
AU - Picq, C.
AU - Popa, V.
AU - Pradier, T.
AU - Presani, E.
AU - Racca, C.
AU - Radu, A.
AU - Reed, C.
AU - Riccobene, G.
AU - Richardt, C.
AU - Rujoiu, M.
AU - Ruppi, M.
AU - Russo, G. V.
AU - Salesa, F.
AU - Sapienza, P.
AU - Schöck, F.
AU - Schuller, J. P.
AU - Shanidze, R.
AU - Simeone, F.
AU - Spurio, M.
AU - Steijger, J. J.M.
AU - Stolarczyk, Th
AU - Taiuti, M.
AU - Tamburini, C.
AU - Tasca, L.
AU - Toscano, S.
AU - Vallage, B.
AU - Van Elewyck, V.
AU - Vannoni, G.
AU - Vecchi, M.
AU - Vernin, P.
AU - Wijnker, G.
AU - De Wolf, E.
AU - Yepes, H.
AU - Zaborov, D.
AU - Zornoza, J. D.
AU - Zúñiga, J.
N1 - Funding Information: The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat à l’énergie atomique et aux énergies alternatives (CEA), Agence National de la Recherche (ANR), Commission Européenne (FEDER fund and Marie Curie Program), Région Alsace (contrat CPER), Région Provence-Alpes-Côte d’Azur, Département du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium für Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Ciencia e Innovacion (MICINN), Prometeo of Generalitat Valenciana (GVA) and MULTIDARK, Spain. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities.
PY - 2011
Y1 - 2011
N2 - The AMADEUS (ANTARES Modules for the Acoustic Detection Under the Sea) system which is described in this article aims at the investigation of techniques for acoustic detection of neutrinos in the deep sea. It is integrated into the ANTARES neutrino telescope in the Mediterranean Sea. Its acoustic sensors, installed at water depths between 2050 and 2300 m, employ piezo-electric elements for the broad-band recording of signals with frequencies ranging up to 125 kHz. The typical sensitivity of the sensors is around -145 dB re 1 V/μPa (including preamplifier). Completed in May 2008, AMADEUS consists of six "acoustic clusters", each comprising six acoustic sensors that are arranged at distances of roughly 1 m from each other. Two vertical mechanical structures (so-called lines) of the ANTARES detector host three acoustic clusters each. Spacings between the clusters range from 14.5 to 340 m. Each cluster contains custom-designed electronics boards to amplify and digitise the acoustic signals from the sensors. An on-shore computer cluster is used to process and filter the data stream and store the selected events. The daily volume of recorded data is about 10 GB. The system is operating continuously and automatically, requiring only little human intervention. AMADEUS allows for extensive studies of both transient signals and ambient noise in the deep sea, as well as signal correlations on several length scales and localisation of acoustic point sources. Thus the system is excellently suited to assess the background conditions for the measurement of the bipolar pulses expected to originate from neutrino interactions.
AB - The AMADEUS (ANTARES Modules for the Acoustic Detection Under the Sea) system which is described in this article aims at the investigation of techniques for acoustic detection of neutrinos in the deep sea. It is integrated into the ANTARES neutrino telescope in the Mediterranean Sea. Its acoustic sensors, installed at water depths between 2050 and 2300 m, employ piezo-electric elements for the broad-band recording of signals with frequencies ranging up to 125 kHz. The typical sensitivity of the sensors is around -145 dB re 1 V/μPa (including preamplifier). Completed in May 2008, AMADEUS consists of six "acoustic clusters", each comprising six acoustic sensors that are arranged at distances of roughly 1 m from each other. Two vertical mechanical structures (so-called lines) of the ANTARES detector host three acoustic clusters each. Spacings between the clusters range from 14.5 to 340 m. Each cluster contains custom-designed electronics boards to amplify and digitise the acoustic signals from the sensors. An on-shore computer cluster is used to process and filter the data stream and store the selected events. The daily volume of recorded data is about 10 GB. The system is operating continuously and automatically, requiring only little human intervention. AMADEUS allows for extensive studies of both transient signals and ambient noise in the deep sea, as well as signal correlations on several length scales and localisation of acoustic point sources. Thus the system is excellently suited to assess the background conditions for the measurement of the bipolar pulses expected to originate from neutrino interactions.
KW - AMADEUS
KW - ANTARES
KW - Acoustic neutrino detection
KW - Neutrino telescope
KW - Thermo-acoustic model
UR - http://www.scopus.com/inward/record.url?scp=79251595181&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=79251595181&partnerID=8YFLogxK
U2 - 10.1016/j.nima.2010.09.053
DO - 10.1016/j.nima.2010.09.053
M3 - Article
AN - SCOPUS:79251595181
VL - 626-627
SP - 128
EP - 143
JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
SN - 0168-9002
IS - 1
ER -