Design and performance of the South Pole Acoustic Test Setup
Yasser Abdou, Karl-Heinz Becker, Jens Berdermann, Martin Bissok,, Christian Bohm, Sebastian Boeser, Martin Bothe, Michael Carson, Freija, Descamps, Jan-Hendrik Fischer-Wolfarth, Leif Gustafsson, Allan Hallgren, Dirk, Heinen, Klaus Helbing, Reinhart Heller, Stephan Hundertmark

TL;DR
The paper describes the design, deployment, and initial performance results of SPATS, an acoustic array in the South Pole ice, aimed at evaluating its suitability for detecting ultra-high-energy neutrinos via acoustic signals.
Contribution
It presents the design, deployment, and technical performance of SPATS, a novel acoustic detection setup in the South Pole ice for neutrino astronomy.
Findings
SPATS successfully detected and generated acoustic signals in ice.
The system's noise levels and signal transmission characteristics were characterized.
Preliminary data support the feasibility of acoustic neutrino detection at the South Pole.
Abstract
The South Pole Acoustic Test Setup (SPATS) was built to evaluate the acoustic characteristics of the South Pole ice in the 10 kHz to 100 kHz frequency range, for the purpose of assessing the feasibility of an acoustic neutrino detection array at the South Pole. The SPATS hardware consists of four vertical strings deployed in the upper 500 m of the South Pole ice cap. The strings form a trapezoidal array with a maximum baseline of 543 m. Each string has 7 stages equipped with one transmitter and one sensor module. Sound is detected or generated by piezoelectric ceramic elements inside the modules. Analogue signals are sent to the surface on electric cables where they are digitized by a PC-based data acquisition system. The data from all strings are collected on a central computer in the IceCube Laboratory from where they are send to a central data storage facility via a satellite link or…
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