%0 Generic %1 Boeser2008 %A Boeser, S. %A Bohm, C. %A Descamps, F. %A Fischer, J. %A Hallgren, A. %A Heller, R. %A Hundertmark, S. %A Krieger, K. %A Nahnhauer, R. %A Pohl, M. %A Price, P. B. %A Sulanke, K.-H. %A Tosi, D. %A Vandenbroucke, J. %D 2008 %J arXiv %K high-energy DESY southpole acoustic icecube neutrino spats %T Feasibility of acoustic neutrino detection in ice: Design and performance of the South Pole Acoustic Test Setup (SPATS) %U http://arxiv.org/PS_cache/arxiv/pdf/0807/0807.4676v1.pdf %X The South Pole Acoustic Test Setup (SPATS) has been built to evaluate the acoustic characteristics of the South Pole ice in the 10 to 100 kHz frequency range so that the feasibility and specific design of an acoustic neutrino detection array at South Pole can be evaluated. SPATS consists of three vertical strings that were deployed in the upper 400 meters of the South Pole ice cap in January 2007, using the upper part of IceCube holes. The strings form a triangular array with the longest baseline 421 meters. Each of them has 7 stages with one transmitter and one sensor module. Both are equipped with piezoelectric ceramic elements in order to produce or detect sound. Analog signals are brought to the surface on electric cables where they are digitized by a PC-based data acquisition system. The data from all three strings are collected on a master-PC in a central facility, from which they are sent to the northern hemisphere via a satellite link or locally stored on tape. A technical overview of the SPATS detector and its performance is presented.

@electronic{Boeser2008, abstract = {The South Pole Acoustic Test Setup (SPATS) has been built to evaluate the acoustic characteristics of the South Pole ice in the 10 to 100 kHz frequency range so that the feasibility and specific design of an acoustic neutrino detection array at South Pole can be evaluated. SPATS consists of three vertical strings that were deployed in the upper 400 meters of the South Pole ice cap in January 2007, using the upper part of IceCube holes. The strings form a triangular array with the longest baseline 421 meters. Each of them has 7 stages with one transmitter and one sensor module. Both are equipped with piezoelectric ceramic elements in order to produce or detect sound. Analog signals are brought to the surface on electric cables where they are digitized by a PC-based data acquisition system. The data from all three strings are collected on a master-PC in a central facility, from which they are sent to the northern hemisphere via a satellite link or locally stored on tape. A technical overview of the SPATS detector and its performance is presented.}, added-at = {2009-03-11T17:32:05.000+0100}, archiveprefix = {arXiv}, author = {Boeser, S. and Bohm, C. and Descamps, F. and Fischer, J. and Hallgren, A. and Heller, R. and Hundertmark, S. and Krieger, K. and Nahnhauer, R. and Pohl, M. and Price, P. B. and Sulanke, K.-H. and Tosi, D. and Vandenbroucke, J.}, biburl = {https://www.bibsonomy.org/bibtex/2d7a75d932ec3ae60cbe29af4f3d29467/jfischer}, eprint = {0807.4676}, interhash = {d63d0538298c5c0ddd94a61a4cc16b09}, intrahash = {d7a75d932ec3ae60cbe29af4f3d29467}, journal = {arXiv}, keywords = {high-energy DESY southpole acoustic icecube neutrino spats}, primaryclass = {astro-ph}, slaccitation = {%%CITATION = 0807.4676;%%}, timestamp = {2009-03-11T17:32:05.000+0100}, title = {Feasibility of acoustic neutrino detection in ice: Design and performance of the South Pole Acoustic Test Setup (SPATS)}, url = {http://arxiv.org/PS_cache/arxiv/pdf/0807/0807.4676v1.pdf}, year = 2008 }