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Acoustic in-ice positioning in the Enceladus Explorer project

Published online by Cambridge University Press:  26 July 2017

Dmitry Eliseev
Affiliation:
III. Physikalisches Institut, RWTH Aachen University, Aachen, Germany E-mail: heinen@physik.rwth-aachen.de
Dirk Heinen
Affiliation:
III. Physikalisches Institut, RWTH Aachen University, Aachen, Germany E-mail: heinen@physik.rwth-aachen.de
Klaus Helbing
Affiliation:
Department of Physics, University of Wuppertal, Wuppertal, Germany
Ruth Hoffmann
Affiliation:
Department of Physics, University of Wuppertal, Wuppertal, Germany
Uwe Naumann
Affiliation:
Department of Physics, University of Wuppertal, Wuppertal, Germany
Franziska Scholz
Affiliation:
III. Physikalisches Institut, RWTH Aachen University, Aachen, Germany E-mail: heinen@physik.rwth-aachen.de
Christopher Wiebusch
Affiliation:
III. Physikalisches Institut, RWTH Aachen University, Aachen, Germany E-mail: heinen@physik.rwth-aachen.de
Simon Zierke
Affiliation:
III. Physikalisches Institut, RWTH Aachen University, Aachen, Germany E-mail: heinen@physik.rwth-aachen.de
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Abstract

The Enceladus Explorer project is a preparatory study for a future space mission to Saturn’s moon, Enceladus. Its ultimate goal is to probe liquid-water pockets below the ice surface of Enceladus for signatures of life. A probe could be based on the IceMole concept, which melts curved trajectories through the ice. In the Enceladus Explorer project, a specialized IceMole probe for a terrestrial test scenario is in development. The goal of this exploratory study is to probe water from a liquid crevasse close to Blood Falls at Taylor Glacier, Antarctica. To navigate such a probe it is essential to be able to determine its position and monitor its trajectory. Part of the navigation system is the in-ice acoustic positioning system. For this, the head of the IceMole is equipped with acoustic sensors, which receive signals from synchronized acoustic emitters situated at the ice surface. Based on the measured propagation times, the speed of sound in ice and the positions of the emitters at the surface, the position of the IceMole can be determined by trilateration techniques. Here we present the developed acoustic positioning system, which is designed to track the in-ice melting probe up to distances of 100 m in glacier ice. Results from full-system tests in water and a first field test on Morteratschgletscher, Switzerland, are discussed.

Information

Type
Research Article
Copyright
Copyright © International Glaciological Society 2014
Figure 0

Fig. 1.Photograph of the plumes in the south polar region of Enceladus. Image credit: NASA/Jet Propulsion Laboratory (JPL)/SSI.

Figure 1

Fig. 2.Principle of the APS. The absolute position of the IceMole is determined by trilateration of ultrasonic pulses from several emitters.

Figure 2

Fig. 3.Scheme of the APS data-acquisition microcontroller.

Figure 3

Fig. 4.Flow chart of the APS, showing all essential parts of the system. CTU: central transducer unit; FTU: front-end transducer unit; emPC: embedded PC; DAQ: data-acquisition system.

Figure 4

Fig. 5.Waveforms of different measurements, and schema of the test site of the APS proof of principle. The schema shows the top view of the melted holes with the corresponding distances between the holes. The waveforms were recorded while the receivers were in hole 0 and the transducer in hole 2, 5 or 6. Note the different scales on the y-axis.

Figure 5

Fig. 6.Sketch of the set-up for the full-system tests in water. IceMole is scaled by a factor of 2.

Figure 6

Fig. 7.Angular sensitivity pattern of the IceMole measured during a full-system test in water. 0° is in front of the IceMole.

Figure 7

Fig. 8.Reconstructed IceMole positions (circles with errors) in comparison with the position of the raft (diamonds). The errors represent the uncertainties of the trilateration algorithm.

Figure 8

Fig. 9.Signal from one transducer recorded by a receiver within the IceMole head during the field test in summer 2013 on Morteratschgletscher. The horizontal dashed lines mark the signal detection thresholds. The arrival time was determined to 3.7 ms, which corresponds to a distance of ∼13 m using a measured speed of sound of 3600 m s−1.

Figure 9

Fig. 10.Reconstructed 20 m long trajectory recorded during the field test on Morteratschgletscher in summer 2013. The dashed line is a crevasse.