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Measurement of sound speed vs. depth in South Pole ice for neutrino astronomy

  • R. Abbasi
  • , Y. Abdou
  • , M. Ackermann
  • , J. Adams
  • , J. A. Aguilar
  • , M. Ahlers
  • , K. Andeen
  • , J. Auffenberg
  • , X. Bai
  • , M. Baker
  • , S. W. Barwick
  • , R. Bay
  • , J. L. Bazo Alba
  • , K. Beattie
  • , J. J. Beatty
  • , S. Bechet
  • , J. K. Becker
  • , K. H. Becker
  • , M. L. Benabderrahmane
  • , J. Berdermann
  • P. Berghaus, D. Berley, E. Bernardini, D. Bertrand, D. Z. Besson, M. Bissok, E. Blaufuss, D. J. Boersma, C. Bohm, J. Bolmont, S. Böser, O. Botner, L. Bradley, J. Braun, D. Breder, T. Castermans, D. Chirkin, B. Christy, J. Clem, S. Cohen, D. F. Cowen, M. V. D'Agostino, M. Danninger, C. T. Day, C. De Clercq, L. Demirörs, O. Depaepe, F. Descamps, P. Desiati, G. De Vries-Uiterweerd, T. Deyoung, J. C. Diaz-Velez, J. Dreyer, J. P. Dumm, M. R. Duvoort, W. R. Edwards, R. Ehrlich, J. Eisch, R. W. Ellsworth, O. Engdegrd, S. Euler, P. A. Evenson, O. Fadiran, A. R. Fazely, T. Feusels, K. Filimonov, C. Finley, M. M. Foerster, B. D. Fox, A. Franckowiak, R. Franke, T. K. Gaisser, J. Gallagher, R. Ganugapati, L. Gerhardt, L. Gladstone, A. Goldschmidt, J. A. Goodman, R. Gozzini, D. Grant, T. Griesel, A. Groß, S. Grullon, R. M. Gunasingha, M. Gurtner, C. Ha, A. Hallgren, F. Halzen, K. Han, K. Hanson, Y. Hasegawa, J. Heise, K. Helbing, P. Herquet, S. Hickford, G. C. Hill, K. D. Hoffman, K. Hoshina, D. Hubert, W. Huelsnitz, J. P. Hülß, P. O. Hulth, K. Hultqvist, S. Hussain, R. L. Imlay, M. Inaba, A. Ishihara, J. Jacobsen, G. S. Japaridze, H. Johansson, J. M. Joseph, K. H. Kampert, A. Kappes, T. Karg, A. Karle, J. L. Kelley, P. Kenny, J. Kiryluk, F. Kislat, S. R. Klein, S. Klepser, S. Knops, G. Kohnen, H. Kolanoski, L. Köpke, M. Kowalski, T. Kowarik, M. Krasberg, K. Kuehn, T. Kuwabara, M. Labare, S. Lafebre, K. Laihem, H. Landsman, R. Lauer, H. Leich, D. Lennarz, A. Lucke, J. Lundberg, J. Lünemann, J. Madsen, P. Majumdar, R. Maruyama, K. Mase, H. S. Matis, C. P. McParland, K. Meagher, M. Merck, P. Mészáros, E. Middell, N. Milke, H. Miyamoto, A. Mohr, T. Montaruli, R. Morse, S. M. Movit, K. Münich, R. Nahnhauer, J. W. Nam, P. Nießen, D. R. Nygren, S. Odrowski, A. Olivas, M. Olivo, M. Ono, S. Panknin, S. Patton, C. Pérez De Los Heros, J. Petrovic, A. Piegsa, D. Pieloth, A. C. Pohl, R. Porrata, N. Potthoff, P. B. Price, M. Prikockis, G. T. Przybylski, K. Rawlins, P. Redl, E. Resconi, W. Rhode, M. Ribordy, A. Rizzo, J. P. Rodrigues, P. Roth, F. Rothmaier, C. Rott, C. Roucelle, D. Rutledge, D. Ryckbosch, H. G. Sander, S. Sarkar, K. Satalecka, S. Schlenstedt, T. Schmidt, D. Schneider, A. Schukraft, O. Schulz, M. Schunck, D. Seckel, B. Semburg, S. H. Seo, Y. Sestayo, S. Seunarine, A. Silvestri, A. Slipak, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, G. Stephens, T. Stezelberger, R. G. Stokstad, M. C. Stoufer, S. Stoyanov, E. A. Strahler, T. Straszheim, K. H. Sulanke, G. W. Sullivan, Q. Swillens, I. Taboada, O. Tarasova, A. Tepe, S. Ter-Antonyan, C. Terranova, S. Tilav, M. Tluczykont, P. A. Toale, D. Tosi, D. Turan, N. Van Eijndhoven, J. Vandenbroucke, A. Van Overloop, C. Vogt, B. Voigt, C. Walck, T. Waldenmaier, M. Walter, C. Wendt, S. Westerhoff, N. Whitehorn, C. H. Wiebusch, A. Wiedemann, G. Wikström, D. R. Williams, R. Wischnewski, H. Wissing, K. Woschnagg, X. W. Xu, G. Yodh, S. Yoshida
  • University of Wisconsin-Madison
  • Ghent University
  • German Electron Synchrotron
  • University of Canterbury
  • University of Oxford
  • University of Wuppertal
  • University of Delaware
  • University of California at Irvine
  • University of California at Berkeley
  • Lawrence Berkeley National Laboratory
  • Ohio State University
  • Université libre de Bruxelles
  • TU Dortmund University
  • University of Maryland, College Park
  • University of Kansas
  • RWTH Aachen University
  • Oskar Klein Centre
  • Uppsala University
  • Pennsylvania State University
  • Universite de Mons
  • Swiss Federal Institute of Technology Lausanne
  • Vrije Universiteit Brussel
  • Utrecht University
  • Clark Atlanta University
  • Southern University and A&M College
  • Humboldt University of Berlin
  • Johannes Gutenberg University Mainz
  • Max Planck Institute for Nuclear Physics
  • Chiba University
  • University of Wisconsin-River Falls
  • University of Alaska Anchorage
  • Georgia Institute of Technology
  • University of Alabama

Research output: Contribution to journalArticlepeer-review

26 Scopus citations

Abstract

We have measured the speed of both pressure waves and shear waves as a function of depth between 80 and 500 m depth in South Pole ice with better than 1% precision. The measurements were made using the South Pole Acoustic Test Setup (SPATS), an array of transmitters and sensors deployed in the ice at the South Pole in order to measure the acoustic properties relevant to acoustic detection of astrophysical neutrinos. The transmitters and sensors use piezoceramics operating at ∼5-25 kHz. Between 200 m and 500 m depth, the measured profile is consistent with zero variation of the sound speed with depth, resulting in zero refraction, for both pressure and shear waves. We also performed a complementary study featuring an explosive signal propagating vertically from 50 to 2250 m depth, from which we determined a value for the pressure wave speed consistent with that determined for shallower depths, higher frequencies, and horizontal propagation with the SPATS sensors. The sound speed profile presented here can be used to achieve good acoustic source position and emission time reconstruction in general, and neutrino direction and energy reconstruction in particular. The reconstructed quantities could also help separate neutrino signals from background.

Original languageEnglish
Pages (from-to)277-286
Number of pages10
JournalAstroparticle Physics
Volume33
Issue number5-6
DOIs
StatePublished - 2010

Keywords

  • Acoustics
  • Neutrino astronomy
  • Pressure waves
  • Shear waves
  • Sound speed
  • South Pole

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