Dynamics of stick–slip motion, Whillans Ice Stream, Antarctica
Document Type
Article
Department or Administrative Unit
Geological Sciences
Publication Date
5-15-2011
Abstract
The stick–slip motion and associated seismic emissions of Whillans Ice Stream (WIS), West Antarctica are two of the many recent observations of unexpected ice sheet behavior that are challenging traditional models of rapid glacier motion. Here we find that the WIS slip events repeatedly nucleate from a sticky-spot located in the middle of the ice stream, acting similar to an asperity in traditional models of earthquake physics. This region shows less motion than surrounding areas during the inter-slip periods, thus, concentrating stress and producing a pulse of seismic energy at the onset of slip. The propagating rupture breaks through an additional asperity in the northern part of the ice stream, producing another pulse of seismic energy 6–12 min after initiation. Both asperities are regions of higher hydraulic potential than surrounding regions, suggesting they may have greater bed friction due to reduced water lubrication. Tidal pacing of the stress accumulation combined with fault healing controls the applied stress at failure, with higher stress giving faster propagation of the rupture front and higher slip velocities; these differences are reflected in the timing of the teleseismic arrivals. Our results highlight both the great sensitivity of large ice streams to small changes in external forcing and the importance of limited regions of the subglacial bed in controlling their motion, as well as providing insights to the mechanics of repeating earthquakes.
Recommended Citation
Winberry, J. P., Anandakrishnan, S., Wiens, D. A., Alley, R. B., & Christianson, K. (2011). Dynamics of stick–slip motion, Whillans Ice Stream, Antarctica. Earth and Planetary Science Letters, 305(3–4), 283–289. https://doi.org/10.1016/j.epsl.2011.02.052
Journal
Earth and Planetary Science Letters
Rights
Copyright © 2011 Elsevier B.V. All rights reserved.
Comments
This article was originally published in Earth and Planetary Science Letters. The full-text article from the publisher can be found here.
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