Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10787
Authors: Winter, Anna* 
Steinhage, Daniel* 
Arnold, Emily J.* 
Blankenship, Donald D.* 
Cavitte, Marie G. P.* 
Corr, Hugh F. J.* 
Paden, John D.* 
Urbini, Stefano* 
Young, Duncan A.* 
Eisen, Olaf* 
Title: Radio-echo sounding measurements and ice-core synchronization at Dome C, Antarctica
Issue Date: 2017
Series/Report no.: /11 (2017)
DOI: 10.5194/tc-2016-147
URI: http://hdl.handle.net/2122/10787
Abstract: We present a compilation of radio-echo sounding (RES) measurements of five radar systems (AWI, BAS, CReSIS, INGV and UTIG) around the EPICA Dome C (EDC) drill site, East Antarctica. The aim of our study is to investigate the differences of the various systems in their resolution of internal reflection horizons (IRHs) and bedrock topography, penetration depth, and quality of imaging the basal layer. We address the questions of the compatibility of existing radar data for common interpretation, and the 5 suitability of the individual systems for Oldest Ice reconnaissance surveys.We find that the most distinct IRHs and IRH patterns can be identified and transferred between most data sets. Considerable differences between the RES systems exist in range resolution and depiction of the basal layer. Considering both aspects, which we judge as crucial factors in the search for old ice, the CReSIS and the UTIG systems are the most valuable ones. In addition to the RES data set comparison we calculate a synthetic radar trace from EDC density and conductivity profiles.We identify ten common IRHs in the measured 10 RES data and the synthetic trace. The reflection-causing conductivity sections are determined by sensitivity studies with the synthetic trace. In this way, we accomplish an accurate two-way travel time to depth conversion for the reflectors, without having to use a precise velocity-depth function that would accumulate depth uncertainties with increasing depth. The identified IRHs are assigned with the AICC2012 time scale age. Due to the isochronous character of these conductivity-caused IRHs, they are a means to extend the Dome C age structure by tracing the IRHs along the RES profiles.
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