Abstract

AbstractWe use seismic refraction data to investigate the firn structure across a suture zone on the Amery Ice Shelf, East Antarctica, and the possible role of glacier dynamics in firn evolution. In the downstream direction, the data reveal decreasing compressional-wave velocities and increasing penetration depth of the propagating wave in the firn layer, consistent with$\sim$1 m firn thickening every 6 km. The boundary between the Lambert Glacier unit to the west and a major suture zone and the Mawson Escarpment Ice Stream unit to the east, is marked by differences in firn thicknesses, compressional-wave velocities and seismic anisotropy in the across-flow direction. The latter does not contradict the presence of a single-maximum crystal orientation fabric oriented 45–$90^{\circ }$away from the flow direction. This is consistent with the presence of transverse simple shear governing the region's underlying ice flow regime, in association with elevated strain along the suture zone. The confirmation and quantification of the implied dynamic coupling between firn and the underlying ice requires integration of future seismic refraction, coring and modelling studies. Because firn is estimated to cover$\sim$98% of the Antarctic continent any such coupling may have widespread relevance to ice-sheet evolution and flow.

Highlights

  • Firn is a porous, intermediate layer of polar ice sheets that exists between freshly accumulated snow and the underlying glacial ice (Cuffey and Paterson, 2010, Ch. 2)

  • We demonstrate the complex physical structure of the firn layer on the Amery Ice Shelf by analysing first arrival travel times of a seismic dataset, which reveals clear trends along and across a major ice shelf suture zone

  • Orthogonal profiles at each of the 11 survey sites permit the analysis of directional changes of seismic velocity at each site and relative seismic velocity changes between the survey sites

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Summary

Introduction

Intermediate layer of polar ice sheets that exists between freshly accumulated snow and the underlying glacial ice (Cuffey and Paterson, 2010, Ch. 2). For ice core climatological records, firn models are essential to determine the age difference between the ice matrix and the age of gases trapped within (e.g. Parrenin and others, 2012). In both cases the accuracy of model estimates is limited by our understanding of firn densification and structural evolution. Viscoplastic deformation due to increasing overburden pressure drives the third densification stage until pore close-off is reached at 830 kg m−3 (Maeno and Ebinuma, 1983), i.e. when air entrapped in the firn forms discrete bubbles within the polycrystalline ice matrix. A fourth stage of slow density increase, up to 917 kg m−3, is associated with compression of these air bubbles (Lipenkov and others, 1997)

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