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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Lawrence Berkeley National Laboratory
2009
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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 |
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University of North Texas: UNT Digital Library |
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ftunivnotexas |
language |
English |
topic |
Acoustic Detection Acoustics Neutrinos 79 Astronomy And Astrophysics Refraction Velocity Shear Accuracy Explosives |
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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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1766201139476299776 |