A compact acoustic calibrator for ultra-high energy neutrino detection

被引：2

作者：

Adrian-Martinez, S. ^{[1
]}

Ardid, M. ^{[1
]}

Bou-Cabo, M. ^{[1
]}

Larosa, G. ^{[1
]}

Llorens, C. D. ^{[1
]}

Martinez-Mora, J. A. ^{[1
]}

机构：

[1] Univ Politecn Valencia, Inst Invest Gestio Integrada Zones Costaneres, Valencia 46730, Spain

来源：

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2013年 / 725卷

关键词：

Underwater neutrino telescopes; Acoustic neutrino detection; Parametric acoustic sources; Underwater acoustic array sensors; SIGNALS; SYSTEM; WATER;

D O I：

10.1016/j.nima.2012.11.142

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

With the aim to optimize and test the method of acoustic detection of ultra-high energy neutrinos in underwater telescopes a compact acoustic transmitter array has been developed. The acoustic parametric effect is used to reproduce the acoustic signature of an ultra-high-energy neutrino interaction. Different R&D studies are presented in order to show the viability of the parametric sources technique to deal with the difficulties of the acoustic signal generation: a very directive transient bipolar signal with 'pancake' directivity. The design, construction and characterization of the prototype are described, including simulation of the propagation of an experimental signal, measured in a pool, over a distance of 1 km. Following these studies, next steps will be testing the device in situ, in underwater neutrino telescope, or from a vessel in a sea campaign. (c) 2012 Elsevier B.V. All rights reserved.

引用

页码：219 / 222

页数：4

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