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Scale independence of till rheology

Published online by Cambridge University Press:  08 September 2017

Slawek Tulaczyk*
Affiliation:
Department of Earth Sciences, University of California, Santa Cruz, California 95064, USA E-mail: tulaczyk@pmc.ucsc.edu
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Abstract

Representation of till rheology in glaciological models of ice motion over deformable sediments has, until now, focused largely on two end-member cases: (1) linear, or mildly non-linear, viscous rheology and (2) (nearly) plastic rheology. Most laboratory and in situ experiments support the latter model. Hindmarsh (1997) and Fowler (2002, 2003) proposed that experimental results represent the behavior of small till samples (characteristic length scales of ~0.1 to ~1 m) but that till behaves viscously over length scales that are relevant to determination of ice-flow rates in glaciers and ice sheets (~1 km or more). Observations of short speed-up events on the ice plain of Whillans Ice Stream, West Antarctica, provide an opportunity to compare the in situ rheology of this till, integrated over ~10–100 km, with the rheology of till from beneath the same ice stream determined on small laboratory samples and in local borehole experiments. This comparison indicates that the rheology of the subglacial till beneath Whillans Ice Stream is independent of scale.

Information

Type
Research Article
Copyright
Copyright © International Glaciological Society 2006
Figure 0

Fig. 1. Log–log plot of non-dimensional shear strain rate as a function of non-dimensional shear stress. Clouds of individual points represent measurements performed during three separate triaxial compression tests on three samples of UpB till (Tulaczyk and others, 2000). Solid lines show least-squares fits of Equation (3) to the data. The dashed line illustrates behavior of a linearly viscous rheology. The thick black bar shows the lower bound on the estimate of the shear strain-rate ratio for the ice plain of WIS, with the grey box reflecting the uncertainty caused by the fact that u0 may be <0.1 m h−1.