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AMADEUS-The Acoustic Neutrino Detection Test System of the Deep-Sea ANTARES Neutrino Telescope
Content Provider | Semantic Scholar |
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Author | Aguilar, Jose A. Samarai, Imen Al Albert, Andreas Anghinolfi, Marco Anton, Gisela Anvar, Shebli Ardid, Miguel Jesus, Ana Carolina Assis Astraatmadja, Tri L. Aubert, J-J. Auer, Ralf Barbarito, Ed Baret, Bruny Basa, Stéphane Bertin, V. Bigongiari, Ciro Bou-Cabo, Manuel Bouwhuis, Mieke Brown, Alan Brunner, J. Busto, J. Camarena, Francisco Cecchini, Sébastien Circella, M. Coniglione, R. Costantini, Heide Curtil, Christian Bonis, Giuseppe D. De Dekeyser, Ivan Donzaud, Corinne Dornic, Damien Drouhin, Doriane Eberl, Thomas Fritsch, Ulf G'omez-Gonz'alez, J. P. Guillard, Goulven Halladjian, G. Hallewell, Gregory Heijboer, A. J. Herold, Björn Hößl, Juergen Jong, Mathijs De Kretschmer, Wolfgang Lamare, Pierre-Olivier Lambard, Guillaume Lefèvre, Dominique Lucarelli, Franco |
Copyright Year | 2019 |
Abstract | The AMADEUS system described in this article is integrated i nto the ANTARES neutrino telescope in the Mediterranean Sea and aims at the inve st gation of techniques for acoustic detection of neutrinos in the deep sea. Installed a t water depths between 2000 and 2400 m, its acoustic sensors employ piezo-electric elem ents for the broad-band recording of signals with frequencies ranging up to 125 kHz with typ ical sensitivities around −145 dB re. 1V/ μPa (including preamplifier). Completed in May 2008, AMADEUS consists of six “acoustic clusters”, each comprising six acous tic sensors that are arranged at distances of roughly 1 m from each other. Three acoustic clus ters each are installed along two vertical mechanical structures (so-called lines) of th e ANTARES detector at a horizontal distance of 240 m. Vertical spacings within a line range f rom 15 m to 125 m. Each cluster contains custom-designed electronics boards to amplify an d digitise the acoustic data from the sensors. The data transmission to shore is done via optic al fibres, using the TCP/IP protocol. An on-shore computer cluster, currently consisting of four dedicated servers, is used to process, filter and store the selected data. The daily volu me of recorded data is about 10 – 20 GByte. The system is operating continuously and automat ically, requiring only little human intervention. AMADEUS allows for extensive studies o f b th transient signals and ambient noise in the deep sea as well as signal correlations o n several length scales and localisation of acoustic point sources. Thus the system is e xcellently suited to assess the background conditions that affect the measurement of bipol ar pulses expected to originate from neutrino interactions. This in turn allows for feasibi lity studies of a future large-scale acoustic neutrino telescope in the Mediterranean Sea. |
File Format | PDF HTM / HTML |
Alternate Webpage(s) | http://hal.in2p3.fr/in2p3-00474914/document |
Language | English |
Access Restriction | Open |
Content Type | Text |
Resource Type | Article |