We present development work aiming towards a large scale ice-based hybrid detector including acoustic sensors for the detection of neutrinos in the GZK range. A facility for characterization and calibration of acoustic sensors in clear (bubble-free) ice has been developed and the first measurements done at this facility are presented. Further, a resonant sensor intended primarily for characterization of the ambient noise in the ice at the South Pole has been developed and some data from its performance are given. (C) 2010 Elsevier B.V. All rights reserved
For the planned high-energy extension of the IceCube Neutrino Observatory in the glacial ice at the ...
We have measured the speed of both pressure waves and shear waves as a function of depth between 80 ...
Neutrino astronomy is a new field of astroparticle physics that uses neutrino detectors to observe a...
The feasibility and design of an acoustic neutrino detection array in the South Pole ice depend on t...
The South Pole Acoustic Test Setup consists of four strings, each instrumented with seven acoustic s...
The detection of extraterrestrial EHE neutrinos requires detection volumes at least one order of mag...
In order to detect the small neutrino fluxes expected at ultra-high energies, large volumes of ma...
Due to the low flux of ultrahigh energetic neutrinos induced in interactions of cosmic rays with the...
When high-energy particles interact in dense media to produce a particle shower, most of the shower ...
The detection of acoustic signals from ultra-high energy neutrino interactions is a promising method...
The detection of acoustic signals from ultra-high energy neutrino interactions is a promising method...
The South Pole Acoustic Test Setup (SPATS) was built to evaluate the acoustic characteristics of the...
Abstract: Astrophysical neutrinos in the EeV range (particularly those generated by the interaction ...
We have measured the speed of both pressure waves and shear waves as a function of depth between 80 ...
Over the last few decades, several dedicated neutrino telescopes have been built to detect high ener...
For the planned high-energy extension of the IceCube Neutrino Observatory in the glacial ice at the ...
We have measured the speed of both pressure waves and shear waves as a function of depth between 80 ...
Neutrino astronomy is a new field of astroparticle physics that uses neutrino detectors to observe a...
The feasibility and design of an acoustic neutrino detection array in the South Pole ice depend on t...
The South Pole Acoustic Test Setup consists of four strings, each instrumented with seven acoustic s...
The detection of extraterrestrial EHE neutrinos requires detection volumes at least one order of mag...
In order to detect the small neutrino fluxes expected at ultra-high energies, large volumes of ma...
Due to the low flux of ultrahigh energetic neutrinos induced in interactions of cosmic rays with the...
When high-energy particles interact in dense media to produce a particle shower, most of the shower ...
The detection of acoustic signals from ultra-high energy neutrino interactions is a promising method...
The detection of acoustic signals from ultra-high energy neutrino interactions is a promising method...
The South Pole Acoustic Test Setup (SPATS) was built to evaluate the acoustic characteristics of the...
Abstract: Astrophysical neutrinos in the EeV range (particularly those generated by the interaction ...
We have measured the speed of both pressure waves and shear waves as a function of depth between 80 ...
Over the last few decades, several dedicated neutrino telescopes have been built to detect high ener...
For the planned high-energy extension of the IceCube Neutrino Observatory in the glacial ice at the ...
We have measured the speed of both pressure waves and shear waves as a function of depth between 80 ...
Neutrino astronomy is a new field of astroparticle physics that uses neutrino detectors to observe a...