Measurement of sound speed vs. depth in South Pole ice: pressure waves and shear waves

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 a...

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Main Authors: Collaboration, IceCube, Klein, Spencer
Other Authors: Lawrence Berkeley National Laboratory. Nuclear Science Division.
Format: Article in Journal/Newspaper
Language:English
Published: Lawrence Berkeley National Laboratory 2009
Subjects:
Online Access:https://digital.library.unt.edu/ark:/67531/metadc1013346/
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spelling ftunivnotexas:info:ark/67531/metadc1013346 2023-05-15T18:21:49+02:00 Measurement of sound speed vs. depth in South Pole ice: pressure waves and shear waves Collaboration, IceCube Klein, Spencer Lawrence Berkeley National Laboratory. Nuclear Science Division. 2009-06-04 11 Text https://digital.library.unt.edu/ark:/67531/metadc1013346/ English eng Lawrence Berkeley National Laboratory rep-no: LBNL-3199E grantno: DE-AC02-05CH11231 osti: 983087 https://digital.library.unt.edu/ark:/67531/metadc1013346/ ark: ark:/67531/metadc1013346 Journal Name: Physical review letter Acoustic Detection Acoustics Neutrinos 79 Astronomy And Astrophysics Refraction Velocity Shear Accuracy Explosives Article 2009 ftunivnotexas 2019-03-23T23:08:15Z 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 {approx}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. Article in Journal/Newspaper South pole University of North Texas: UNT Digital Library South Pole
institution Open Polar
collection University of North Texas: UNT Digital Library
op_collection_id ftunivnotexas
language English
topic Acoustic Detection
Acoustics
Neutrinos
79 Astronomy And Astrophysics
Refraction
Velocity
Shear
Accuracy
Explosives
spellingShingle Acoustic Detection
Acoustics
Neutrinos
79 Astronomy And Astrophysics
Refraction
Velocity
Shear
Accuracy
Explosives
Collaboration, IceCube
Klein, Spencer
Measurement of sound speed vs. depth in South Pole ice: pressure waves and shear waves
topic_facet Acoustic Detection
Acoustics
Neutrinos
79 Astronomy And Astrophysics
Refraction
Velocity
Shear
Accuracy
Explosives
description 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 {approx}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.
author2 Lawrence Berkeley National Laboratory. Nuclear Science Division.
format Article in Journal/Newspaper
author Collaboration, IceCube
Klein, Spencer
author_facet Collaboration, IceCube
Klein, Spencer
author_sort Collaboration, IceCube
title Measurement of sound speed vs. depth in South Pole ice: pressure waves and shear waves
title_short Measurement of sound speed vs. depth in South Pole ice: pressure waves and shear waves
title_full Measurement of sound speed vs. depth in South Pole ice: pressure waves and shear waves
title_fullStr Measurement of sound speed vs. depth in South Pole ice: pressure waves and shear waves
title_full_unstemmed Measurement of sound speed vs. depth in South Pole ice: pressure waves and shear waves
title_sort measurement of sound speed vs. depth in south pole ice: pressure waves and shear waves
publisher Lawrence Berkeley National Laboratory
publishDate 2009
url https://digital.library.unt.edu/ark:/67531/metadc1013346/
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_source Journal Name: Physical review letter
op_relation rep-no: LBNL-3199E
grantno: DE-AC02-05CH11231
osti: 983087
https://digital.library.unt.edu/ark:/67531/metadc1013346/
ark: ark:/67531/metadc1013346
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