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Decadal-scale variations in ice flow along Whillans Ice Stream and its tributaries, West Antarctica

Published online by Cambridge University Press:  08 September 2017

Leigh A. Stearns
Affiliation:
Byrd Polar Research Center and Department of Geological Sciences, The Ohio State University, 1090 Carmack Road, Columbus, Ohio 43210-1002, USA E-mail: leigh.stearns@maine.edu
Kenneth C. Jezek
Affiliation:
Byrd Polar Research Center and Department of Geological Sciences, The Ohio State University, 1090 Carmack Road, Columbus, Ohio 43210-1002, USA E-mail: leigh.stearns@maine.edu
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 E-mail: leigh.stearns@maine.edu
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Abstract

We investigate velocity changes occurring along Whillans Ice Stream (WIS) by comparing velocities derived from repeat aerial photographs acquired in 1985-89 (average date of 1987) to interferometric satellite radar (InSAR) velocities collected in 1997. Three different analysis methods are applied to the velocity data. First, temporal and spatial changes in velocities are correlated to identifiable features (flowlines, shear margins, bed features) visible on the 1997 RADARSAT Antarctic Mapping Project mosaic. Second, we relate velocity gradients to stresses via the flow law and, along with surface topography and ice-thickness data, apply the force-budget technique to determine the relative importance of driving stress, side drag and basal drag over time. Finally, the mass balance of the main part of WIS is determined for 1987 and 1997. Our results are consistent with previous studies that show an overall deceleration resulting in downstream thickening of the ice stream (Whillans and others, 2001; Joughin and others, 2002).

Information

Type
Research Article
Copyright
Copyright © International Glaciological Society 2005
Figure 0

Fig. 1. The locations of photogrammetric velocity data points (black dots) overlain on a portion of the RAMP mosaic. The transects used in this study are shown in white.

Figure 1

Fig. 2. InSAR velocities for WIS and VIS. Velocities <50ma_1 are white, and areas with no data are speckled. Thick black lines spanning the ice stream represent transects used in this study (labeled in Fig. 1). Thin black lines trending down the ice stream are flowlines traced from the RAMP mosaic.

Figure 2

Fig. 3. Spatial and temporal changes in velocity (m a_1) along WIS. The dotted line is the difference between the 1997 InSAR velocities and the 1987 photoblock velocities, plotted at the same scale. There are no photoblock data across transects G0n and G0s.

Figure 3

Fig. 4. Shear stress variations (kPa) across WIS, calculated from Equation (1). The 1987 shear stress is derived from the photoblock velocities, and the 1997 shear stress from InSAR velocities (as shown in Fig. 3).

Figure 4

Table 1. Force budget along WIS in 1987 and 1997

Figure 5

Fig. 5. The distribution of driving stress along WIS and VIS based on the OSU DEM and BEDMAP. The value above represents the mean driving stress for each area with a 2σ error, at an average date of 1999.

Figure 6

Fig. 6. Basal drag (italic labels in the center of the ice stream) and weighted shear stress values for 1987 (regular type) and 1997 (bold type).

Figure 7

Table 2. Values of parameters used in Equation (7)

Figure 8

Fig. 7. Rate of thickness change, 1987_97, along WIS. The circles represent data from 1987, and the triangles data from 1997. Isolated stars are thinning rates estimated by Spikes and others (2003), using repeat laser altimetry (from 1997 and 1999) for an area slightly upstream of the study area.

Figure 9

Fig. 8. Rate of thickness change, 1987_97, along VIS and the trunk of WIS. The circles represent data from 1987, and the triangles data from 1997. Isolated stars are thinning rates estimated by Spikes and others (2003), using repeat laser altimetry from 1997 and 1999.

Figure 10

Table A1. Photoblock mass-balance variables. Fi is the flux in through the upstream gate, S is the surface area in between the two flux gates, b is the area-averaged accumulation rate, Fs is the flux through the ice surface (accumulation rate times the surface area), Fin is the sum of Fi and Fs, Fout is the flux out of the downstream gate, and dH/dt is the rate of thickness change. The north tributary refers to the Whillans Ice Stream; the south tributary refers to Van der Veen Ice Stream; ‘all’ refers to the sum of both Ice Streams

Figure 11

Table A2. InSAR mass-balance variables