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
收藏
页码：219 / 222
页数：4
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