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Bed radar reflectivity across the north margin of Whillans Ice Stream, West Antarctica, and implications for margin processes

Published online by Cambridge University Press:  08 September 2017

C.F. Raymond
Affiliation:
Department of Earth and Space Sciences, Box 351310, University of Washington, Seattle, Washington 98195-1310, USA. E-mail: charlie@ess.washington.edu
Ginny A. Catania
Affiliation:
Department of Earth and Space Sciences, Box 351310, University of Washington, Seattle, Washington 98195-1310, USA. E-mail: charlie@ess.washington.edu Institute for Geophysics, University of Texas, Austin, Texas 78759, USA
Nadine Nereson
Affiliation:
Department of Earth and Space Sciences, Box 351310, University of Washington, Seattle, Washington 98195-1310, USA. E-mail: charlie@ess.washington.edu Philips Medical Systems Ultrasound, 22100 Bothell Everett Highway, Bothell, Washington 98021-8434, USA
C.J. Van Der Veen
Affiliation:
Byrd Polar Research Center and Department of Geological Sciences, The Ohio State University, 1090 Carmack Road, Columbus, Ohio 43210-1002, USA
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Abstract

Surface-based ice-penetrating radar profiles were made across the active north margin (the Snake) of the upper part of Whillans Ice Stream (formerly Ice Stream B, branch B2), West Antarctica, at three locations. Low frequency (about 2 MHz) and the ground deployment of the radar allowed penetration through the near-surface zone of fracturing to detect internal layering and bed reflection characteristics on continuous profiles spanning from the slow-moving ice of Engelhardt Ridge well into the chaotic zone of the shear margin. Internal layers were tracked beneath the chaotic zone, where they are warped but remain continuous. The energy returned from internal layers showed no systematic changes associated with the transition from the undisturbed surface of the slow-moving ice into the fractured surface of the shear margin, thus indicating little effect from the surface crevasses on the penetration of the radar signal. Based on this calibration of the near-surface effects and corrections for path length, spreading and attenuation, we examine the spatial variation of bed reflectivity. Low bed reflectivity found under Engelhardt Ridge extends under the chaotic zone of the margin into fast-moving ice. We argue that the fast motion in a band along the margin is mediated by processes other than deformation of thick dilated till that is the source of lubrication allowing fast motion in the interior of the ice stream.

Information

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

Fig. 1. (a) Location of field area in Antarctica. (b) SAR image of Engelhardt Ridge (ER) and bounding Whillans and Kamb Ice Streams taken from the RADARSAT-1 Antarctic Mapping Project (RAMP) mosaic (Jezek, 1999). Lines indicate the approximate paths of ground-based, low-frequency radar profiles collected on parts of ER in the last decade (Nereson and Raymond, 2001; Catania and others, 2003 and unpublished information; this paper). White lines show profiles at approximately 2 MHz used in this paper. Black lines show other profiles not used because of higher frequency (nominally 5–7 MHz) over rough bed areas or instrumental artifacts complicating analysis of power return. Dashed lines are specific profiles from Catania and others (2003) mentioned in the text. White box shows the location of (c). (c) Large-scale image of the WIS margin (Snake) with precise locations (white lines) of three profiles shown in Figure 2. Coordinates are polar stereographic projection in units of km. Horizontal axis is polar stereographic x, and vertical is polar stereographic y

Figure 1

Fig. 2. Radar profiles across the Snake at three locations (Fig. 1b) separated by about 8 km along the direction of flow of WIS: (a) East profile (83.3042° S, 138.3697° W to 83.2667° S, 138.4764° W); (b) Camp profile (83.318° S, 138.976° W to 83.2831 º S, 139.0662° W); and (c) West profile (83.345° S, 139.547° W to 83.2883° S, 139.6608° W). Profiles are aligned with 0 distance at the approximate outer edge of the zone of arcuate crevasses. Shaded vertical bar indicates the possible range in location of maximum strain rate. The disturbance at +1 km in the Camp profile results from scattering from a radio antenna and other objects in the camp. The panel beneath each profile shows relative power return from the bed (BRPR; heavy curve) and interior (IRPN; light curve) as described in the text. Curves of BRPR and IRPN are not smoothed. Curve for IRPN is shifted by 1 to separate it from BRPR.

Figure 2

Fig. 3. Power returned from bed BRP and interior IRP vs two-way travel time to the bed, ttb, for local profiles East, Camp and West (Fig. 1c) including the extension of Camp profile across the divide of ER (Fig. 1b). Different symbols distinguish measurements from ER and those from the Snake. The solid curve represents a function BRP = Ғ(ttb) fit to data from the ER parts of profiles.

Figure 3

Table 1. Statistics of relative bed return power variations

Figure 4

Table 2. Statistics of normalized internal return power variations

Figure 5

Fig. 4. Power returned from the bed BRP scaled to power from the interior IRP vs the corresponding two-way travel time to the bed, ttb, for profiles collected with approximately 2MHz impulse radar. Different symbols indicate source of data. ER local and Snake are from BRP and IRP in Figure 3. SDM are from Siple Dome (Fig. 1b) using data from Jacobel and others (1996) and Gades and others (2000).