Acoustic properties of glacial ice for neutrino detection and the Enceladus Explorer
K. Helbing (1), R. Hoffmann (1), U. Naumann (1), D. Eliseev (2), D., Heinen (2), F. Scholz (2), C. Wiebusch (2), S. Zierke (2) ((1) Dept. of, Physics, University of Wuppertal, (2) III. Physikalisches Institut, RWTH, Aachen University)

TL;DR
This paper investigates the acoustic properties of glacial ice for neutrino detection and explores the use of acoustics in the Enceladus Explorer for subsurface exploration and extraterrestrial life detection.
Contribution
It provides new measurements of ice acoustics at various sites and discusses applications for neutrino detection and extraterrestrial exploration using acoustic systems.
Findings
Measured attenuation and sound speed in ice at multiple sites.
Analyzed frequency response and directional dependencies of acoustic signals.
Developed acoustic transducer systems for ice exploration and neutrino detection.
Abstract
Ultra high energy neutrinos may be observed in ice by the emission of acoustic signals. The SPATS detector has investigated the possibility of observing GZK-neutrinos in the clear ice near the South Pole at the IceCube detector site. To explore other potential detection sites glacial ice in the Alps and in Antarctica has been surveyed for its acoustical properties. The purpose of the Enceladus Explorer (EnEx), on the other hand, is the search for extraterrestrial life on the Saturn moon Enceladus. Here acoustics is used to maneuver a subsurface probe inside the ice by trilateration of signals. A system of acoustic transducers has been developed to study both applications. In the south polar region of the moon Enceladus there are secluded crevasses. These are filled with liquid water, probably heated by tidal forces due to the short distance to Saturn. We intend to take a sample of water…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Cryospheric studies and observations
