The puzzling fact that Jakobshavn Isbræ, West Greenland, is flowing very fast but without any significant seasonal velocity changes, despite big amounts of surface-derived meltwater entering the ice stream (Reference Echelmeyer and HarrisonEchelmeyer and Harrison, 1990), has been explained by a combination of different types of measurements. It is now well established from seismic measurements and radio-echo sounding that Jakobshavn Isbræ flows through a deeply eroded subglacial trench that, even 50 km inland of the grounding line, extends as far as 1500 m below sea level (Reference Clarke and EchelmeyerClarke and Echelmeyer, 1996; Reference Legarsky and HuangLegarsky and Huang, 2006). Temperature measurements in boreholes down to 65% of the 2500 m thick ice stream at site B, some 50 km upstream of the calving front (Fig. 1b; Reference Iken, Echelmeyer, Harrison and FunkIken and others, 1993), were used to infer the presence of a substantial layer of temperate ice, the thickness of which was estimated to be at least 300 m by modeling and matching internal layering structures (Reference Funk, Echelmeyer and IkenFunk and others, 1994; Lüthi and others, 2002). The presence of a thick layer of temperate ice under very high driving stress allows for high ice-deformation rates, which contribute substantially to the observed fast flow velocities. Basal motion, while certainly important, seems to be barely influenced by the seasonal meltwater input (Reference Echelmeyer and HarrisonEchelmeyer and Harrison, 1990).
Since the 1990s the geometry of the calving front has changed completely (Reference Podlech and WeidickPodlech and Weidick, 2004). The 15 km long floating tongue, from which kilometer-scale tabular icebergs used to break off, disintegrated in 2002/03. In recent years a smaller floating tongue forms during the winter months and is rapidly removed in spring (Reference Joughin, Das, King, Smith, Howat and MoonJoughin and others, 2008). During most of the summer a substantial part of the calving front is grounded, as is evident from sediments at the bottom of rotated calving icebergs, and the lack of tidal vertical motion (Reference Amundson, Truffer, Lüthi, Fahnestock, West and MotykaAmundson and others, 2008).
The iceberg shown in Figures 1 and 2 is one of many icebergs that displayed intensely blue ice just after calving. The calving event started on 13 July at 04:47:46 UTC (onset of seismic signal registered at a seismometer next to the camera in Fig. 1b) from a retreated front position (red curve in Fig. 1b). The time-lapse photography shown in Figure 3 (color-enhanced due to poor lighting conditions) shows how the berg rotated backwards during calving, with the basal portion being lifted into the flow direction (towards the left in the image). From the distance scale in Figure 3 (discussed below) we can deduce that the initial vertical extent of the iceberg was ∼900 m. After rotating, the iceberg moved at 3.6 ms−1 away from the calving front, as determined by tracking features B1–B4. The trace of point B1 (black dots in Fig. 3) shows that the iceberg was rocking with an under-damped harmonic oscillation of 70 s period, from which an average vertical (initially horizontal) extent of ∼600 m can be calculated (e.g. Reference SommerfeldSommerfeld, 1994, p.40, equation 16).
During calving, this iceberg displayed a zone of intensely blue ice (left in Fig. 1, dark in Fig. 3), which was located close to the bottom before rotation, while the rest of the iceberg was whitish in appearance. Whether the blue ice contained liquid water or was frozen could not be determined. The blue color vanished during the next day, presumably by the action of solar radiation.
Positions of four natural targets on the iceberg were measured by triangulation with two theodolites (Leica TM1800 and Leica T1600), which were mounted on steel survey stands bolted onto bedrock. The theodolites were 250 m apart and at a distance of ∼4 km from the iceberg, and measurements took place within 10 min. From repeated measurements of the natural targets B1–B4 (indicated in Fig. 1) we estimate a position accuracy of better than 15 m in the horizontal, and 3 m in the vertical. The longest distance measured on the iceberg is (B2,B4) = 710 m in the long axis (inset of Fig. 1a), which was nearly vertical before calving. By identification of B2 and B4 in time-lapse pictures taken during the calving event, the approximate distance scale in Figure 3 was obtained. The distance (B2,B3) is 110 m and covers roughly the left (initially lower) half of the blue zone. The maximum elevation above sea level of the iceberg is 147 m at point B2.
From the iceberg dimensions given above, one can estimate a thickness of the blue ice layer of 200–250 m, which is a substantial portion of the calving-front ice thickness of ∼900 m. Water depth in the ice-filled fjord downstream of the calving front is uniformly ∼800 m (Reference Holland, Thomas, de Young, Ribergaard and LyberthHolland and others, 2008), but might be less in the grounding-line area where subglacial sediments are likely accumulated. The height of the ice cliff at the calving front after this calving event was between 100 and 130 m, as measured using the method described above. Our natural targets, B1 and B2, were within 100 m of the bedrock, as can be estimated from Figures 1a and 3, and some sediments are visible at the left in Figure 2 (marked ‘S’). The top ∼200 m broke off during the calving event, as could be determined by analyzing movies and the image sequence (Fig. 3). For the remaining discussion we assume a calving-front thickness of 900 m.
A layering structure is apparent in the blue ice in Figure 2. The layer labeled ‘BF’ appears to be folded, with the hinge line indicated (‘H’) in Figure 2. Especially striking is a green-grayish layer (‘G’) ∼50 m thick in the middle of the blue zone, and separated at the lower end by a straight plane (labeled ‘P’ in Fig. 2). The origin of the green-grayish color is unknown, but it is difficult to imagine an origin from organic sources, as has been observed elsewhere (e.g. Reference Warren, Roesler, Morgan, Brandt, Goodwin and AllisonWarren and others, 1993). A possible cause of the altered color could be a high dust content, as measured in ice from the late Wisconsin period on the Greenland Icecore Project (GRIP) and Greenland Ice Sheet Project 2 (GISP2) ice cores (e.g. Reference De Angelis, Steffensen, Legrand, Clausen and HammerDe Angelis and others, 1997). The straight boundary plane (‘P’) between greenish and blue ice could be an overthrust fault. Active overthrusting at the transition between Holocene and Wisconsin ice was inferred from erratic ice motion at a drill site, D, 50 km upstream of the terminus and just outside the ice-stream trunk (Lüthi and others, 2003).
We interpret the blue and white colors of parts of the iceberg as indicators of their thermal state. The white ice (on the right in Figs 1a and 3) likely belongs to the layer of very cold (−22°C) ice that has been found in all upstream boreholes. We think that the intensely blue color on the left of Figure 1a indicates ice that was at the pressure-melting point, and that contained liquid water. This interpretation, based on appearance, relies on the idea that cold sedimentary ice contains a high density of air bubbles, and that the presence of meltwater alters bubble density and the optical properties of the ice. Observations and measurements of absorption spectra show that clear, bubble-free ice absorbs red light and therefore appears blue, while air bubbles scatter light at all wavelengths and lead to a white opaque appearance (Reference BohrenBohren, 1983; Reference Warren, Roesler, Morgan, Brandt, Goodwin and AllisonWarren and others, 1993; Reference Warren and BrandtWarren and Brandt, 2008).
If the above interpretation is correct, one can estimate the thickness of the temperate layer upstream of the grounding line. There, the temperate layer has to be considerably thicker than the 200–250 m deduced from Figure 1a. Ice thickness in the center of the ice stream some 50 km inland (e.g. at drill site B (Fig. 1b)) is ∼2500 m (Reference Clarke and EchelmeyerClarke and Echelmeyer, 1996) and diminishes to 900 m or 35% at the calving front. If vertical strain is evenly distributed throughout the ice column, the assumed 200–250 m of temperate ice at the terminus would correspond to 600–750 m at site B, and even more if the temperate ice experiences over-proportional vertical stretching.
An independent estimate of the thickness of the temperate layer in the center of the ice stream can be obtained by comparison of temperature profiles from sites A, B and D (from Reference Iken, Echelmeyer, Harrison and FunkIken and others, 1993; Lüthi and others, 2002). In these publications a comparison with relative depths, and with internal layering structure, was attempted. Matching the temperature profiles in the cold zone by uniformly stretching the depth scale gives surprisingly good agreement. In Figure 4 the measured temperature profiles are shown on a relative depth scale, such that the transition between cold and temperate ice is at relative depth 1. Since the ice between the lower end of the cold zone and bedrock has to be temperate, one can estimate the thickness of that layer. For site D this leads to the observed 38 m of temperate ice, and 720 m for site B.
Both of the above estimates for the thickness of the temperate layer at site B agree. Given the uncertainties involved, this value should be taken with care. If the blue ice observed on many icebergs is indeed at the melting point, a temperate layer of at least 200 m exists near the terminus, and is likely much thicker upstream.
This short note demonstrates the potential of using rotated icebergs to explore the vertical structure of Jakobshavn Isbræ. Such observations would otherwise be only possible with great logistical effort by drilling through very thick and cold ice.
Acknowledgements
The collaboration with R. Motyka, J. Amundson and J. Brown is gratefully acknowledged. Comments by R. Motyka, R. LeB. Hooke, S. Warren and an anonymous reviewer helped improve the clarity of presentation. Logistics support was provided by VECO Polar Resources. Funding was provided by NASA’s Cryospheric Sciences Program (NNG06GB49G), the US National Science Foundation (ARC0531075), the Swiss National Science Foundation (200021-113503/1) and theComer Science and Education Foundation.
19 March 2009