Introduction
Arctic ice-shelf research has been concentrated on Ward Hunt Ice Shelf (Fig. 1). It is now generally accepted that the ice shelf originally grew in situ as a thick, fast sea-ice sheet that thickened further by surface accumulation of snow and ice, and by bottom freezing of fresh, brackish or sea ice (Marshall 1955, Hattersley-Smith 1960, Ragle and others 1964, Lyons and others 1971).
The ice shelf is known to act as a floating dam that creates water stratification in Disraeli Fiord (Fig. 1); here, a layer of fresh water, as deep as the draft of the ice shelf (about 44 m), overlies deeper sea-water (Keys 1978, Jeffries and Krouse 1984). On occasion, frazil ice has been observed growing in the fiord at the halocline separating these two water bodies (Keys 1978). It has been suggested that bottom accretion is associated with similar water stratification and frazil-ice growth beneath the ice shelf (Lyons and others 1971, Keys 1978, Jeffries and Krouse 1984). Whereas Lyons and others (1971) and Keys (1978) favoured brackish ice growth associated with water stratification, Jeffries and Krouse (1984) found evidence only for fresh-water ice growth.
Largely because of the logistics problems involved, there have been no direct investigations of water circulation and freezing beneath the ice shelf. Instead, ice-core analysis, which has relied on cores from the south and west areas of the ice shelf only, has been used for indirect investigations (Ragle and others 1964, Lyons and others 1971). Since 1982, we have drilled and analyzed ice cores (Fig. 1) from Ward Hunt Ice Shelf (including the first to be drilled in the east shelf) as part of a study of ice-shelf structure and growth. In this paper we present some results of this study, with particular reference to water circulation and freezing beneath the ice shelf.
General Description of Ward Hunt Ice Shelf and The Oceanography of Disraeli Fiord
The ice shelf has a thickness of 45-50 m and an area of 440. km2. Ward Hunt Island is located at about the centre of the ice shelf, which is loosely divided into three areas: east, west, and south of the island. In 1982-83, a major ice-island calving from the east shelf occurred (Fig. 1). Three deep ice cores drilled into one of these ice islands are the source of most of the data for the east shelf. The ice upper surface is characterized by a distinctive undulating topography of elongated ridges and troughs that are oriented parallel to the shore and to the prevailing coastal winds.
Although much of the ice exposed at the surface is non-saline, there are surface exposures of saline or basement ice (Fig. 1) (Lyons and others 1971) that are generally considered to have accreted at the bottom (base) of the shelf. The exposure of basement ice can be attributed to surface-ice loss and lowering during the past 100-400 years (Crary 1960, Hattersley-Smith and Serson 1970).
As noted in the Introduction, the ice shelf causes fresh-water / sea-water stratification in Disraeli Fiord (Fig. 1). The δl8O values of the fresh-water layer reflect its meteoric origin, i.e. water that was recently involved in atmospheric circulation, whereas the high tritium activities indicate recent fresh-water inflow (Jeffries and Krouse 1984). In spring, the fresh-water layer is 43-44 m deep (Keys 1978, Jeffries and Krouse 1984). Once, when the fresh-water layer was sampled at the end of summer, it was 60 m deep (Crary 1956). The available evidence is not conclusive, but it is likely that the fresh-water layer deepens as melt water flows into the fiord in summer. During the winter it returns to a depth less than or equivalent to the draft of the ice-shelf dam.
Within the deeper sea-water in the fiord, it has been determined that the inflow is at the bottom and towards the south, whereas the outflow is close to the halocline and towards the north (Keys 1978). With regard to circulation and freezing beneath the ice shelf, the following questions remain: from which direction does sea-water flow into the fiord; in which direction does sea-water flow out of the fiord; if excess fresh water from the fiord surface flows out beneath the ice shelf, does it remain as a discrete layer or is it rapidly mixed with sea-water, and what type of ice growth is associated with this flow of water?
Methods
Since 1982, we have drilled cores across the entire ice shelf, including three deep cores drilled in “Hobson’s Ice Island”, 2–3 years after calving (Fig. 1). Core depths and ridge–trough locations are given in Figure 1. Ice density was measured by weighing in air on a triple-beam balance. Specific electrolytic conductivity (SEC) of the ice was measured by conductivity meter. SEC was the basis for the calculation of practical salinity according to the standard relation of UNESCO (1981). The oxygen-isotope abundances are expressed according to the δ18O scale, defined as
where (18O/16/O) is the ratio of the number of l8O to 16O atoms, ‰ is parts per thousand (per mil), subscript s designates the unknown sample and Standard Mean Ocean Water (SMOW; Craig 1961) is the international reference standard.
Tritium analysis of water samples was undertaken by the Isotope Laboratory, Department of Earth Sciences, University of Waterloo, Ontario. Analysis was by direct liquid scintillation counting without prior enrichment.
Tritium activity of each sample was determined to an accuracy of ±8 TU. After 1952, when the first thermonuclear device was tested in the atmosphere, atmospheric-tritium levels rose, and reached a maximum in 1963, when there was an increase of 2–3 orders of magnitude over natural background levels. The latter fall within the range 0–25 TU (Gat 1980).
Results and Discussion
On the basis of differences in the physical properties (salinity–SEC, 180, and density) of ice in 14 ice cores, five different ice-types have been identified in Ward Hunt Ice Shelf. The five ice-types and data summaries for each are shown in Table 1. The discussion of the results is limited to three particular cores (83-1, 85-10, and 86-8) which show that each ice-type tends to be localized within a particular part of the ice shelf. The water circulation and ice accretion below the ice shelf is deduced from the ice-core results.
Ice core 83-1. west Ward Hunt Ice Shelf
This core was the deepest that was drilled in the western ice shelf, but it was not drilled right through to the bottom. Assuming an ice thickness of 45–50 m at the location of core 83-1 (Fig. 1), drilling ceased 13–18 m short of the bottom. Ice salinity and δ18O values show considerable variation and the core is divided into four distinct strata (Fig. 2). Strata I and 3 h ave very low salinities and the δ18O values indicate a meteoric origin. In the case of stratum I, the ice has formed from accumulation of snow and ice at the ice-shelf surface; this type of ice is commonly referred to as iced firn (after Marshall 1955) and is the product of percolation and refreezing of melt water in the snow-pack. Iced firn is quite bubbly, hence the relatively low density compared to saline basement ice (Table I). In contrast to strata 1 and 3, a large part of core 83-1 is saline basement ice (strata 2 and 4) and the δ18O values indicate a sea-water origin, i.e. strata 2 and 4 are sea ice. The brine in saline basement ice would account for the higher density values.
Hattersley-Smith and others (1969) and Prager (unpublished) all had difficulty obtaining good returns during airborne radio echo-sounding of the western ice shelf. In each case it was suggested that the problem arose due to the presence of saline ice, although few ground-truth data were available. Our data confirm the presence of saline ice which, because of low permittivity, undoubtedly gives rise to large dielectric attenuation. Prager (unpublished) obtained faint internal reflections at depths of 15–25 m which were attributed to the transition from freshwater ice to saline ice. Although it is at 10 m depth, the transition from stratum 1 (iced firn) to stratum 2 (saline basement ice) is very abrupt and likely to give rise to an internal reflection.
An interesting phenomenon associated with the drilling of core 83–1 was brine up-welling in the bore hole (Fig. 2). The level to which brine up-welled might represent the maximum hydraulic head and is probably the cause of the high ice salinities in stratum 4B (Fig. 2). Although ice salinities increase in stratum 4B, there is no change in the δ18O values, which remain close to SMOW. However, the increase in salinity is associated with an increase in tritium values. Figure 3 shows that from the surface to 28 m, tritium activities fall within natural background levels. Below 28 m, higher tritium values occur and indicate a source of thermonuclear tritium.
Although core 83-1 was not drilled to the bottom of the ice shelf, the high tritium values in saline ice, with δ18O values that remain close to SMOW, indicate recent ice accretion from sea-water below the western ice shelf. Seismic sounding (Crary 1956) and hydrographie surveys (Crary 1956, personal communication from R. McDougall) indicate that a deep (900 m) trench, oriented west–east, lies below the western ice shelf. It is probable that the trench channels sea-water into Disraeli Fiord. The great thickness (>l2m) of stratum 4 alone suggests that the flow of sea-water and the associated ice accretion has occurred over a long period below west Ward Hunt Ice Shelf. However, the non-saline basement ice (Table I) of stratum 3 (Fig. 2) suggests that the western ice shelf was underlain by fresh water at least once in the past. This will be discussed further with reference to the eastern ice shelf.
Ice core 85-10, east Ward Hunt Ice Shelf
This ice core was drilled right through to the water below the ice. Salinity and δ18O profiles (Fig. 4) show none of the stratigraphie variation evident in core 83-1 (Fig. 2). Ice core 85-10 has a very low salinity and the δ18O values indicate fresh-water ice of meteoric origin. This ice core is composed entirely of non-saline basement ice (Table I).
The absence of saline ice in the eastern shelf would account for the greater success of radio echo-sounding in this area. Hattersley-Smith and others (1969) obtained thicknesses of 30–40m, whereas Prager (unpublished) obtained 45–50 m. The thickness of “Hobson’s Ice Island” (Fig. 1) varies between 41 and 43.5 m (personal communication from R. Verrall), confirming the greater reliability of radio echo-sounding of the eastern shelf.
As in core 83–1, much of the ice from “Hobson’s Ice Island” has low, background levels of tritium (Fig. 3). In core 85-10, however, tritium values in the lowermost 5 m of ice are as much as twice those in core 83-1. It is possible that the highest value (71 TU at 40 m) is related to the 1963 atmospheric-tritium maximum. The high tritium values in 180-depleted ice at the bottom of core 85-10 must be the result of recent bottom-ice accretion from fresh or meteoric water.
The source of the fresh water below the eastern ice shelf is probably Disraeli Fiord. Hamblin and Carmack (1978) showed that in the Northern Hemisphere the Coriolis force causes water flowing into lakes to be deflected to the right. By analogy, we expect the tidally driven sea-water outflow from Disraeli Fiord to be deflected to the right, beneath the eastern ice shelf. It has been suggested before that fresh water from Disraeli Fiord also flows out beneath the ice shelf, albeit as a brackish water layer from which brackish ice grows (Lyons and others 1971, Keys 1978). Our ice-core evidence suggests that the fresh water does not mix with sea-water to form brackish water. Instead, it appears that fresh-water / sea-water stratification with associated fresh/meteoric ice accretion is extensive beneath the eastern shelf.
The chronology of tritium inputs to the atmosphere is well established, as is subsequent fallout in precipitation. The presence of tritium at the bottom of core 85–10 means that the ice has accreted quite recently, and that the data can also be used to determine the accretion rate. The thickness of the tritiated ice layer suggests a mean annual accretion rate of 95 mm a−1 since 1963. This may be compared to the mean annual surface-ice loss of about 100 mm −1 since the early 1960s (Hattersley-Smith and Serson 1970, Serson 1979). Therefore, if climatic conditions are invariant, a situation would exist in which surface-ice loss is nearly balanced by bottom accretion, resulting in a complete replacement of ice from below. This process of vertical–upward ice movement would account for the eastern ice shelf being composed entirely of non-saline basement ice. If a maximum ice thickness of 45 m is assumed, this process would require about 450 years of overall negative mass balance. Evidence for this long period of negative mass balance has been found in the form of sponges and plant material in the basement ice around Ward Hunt Island (Fig. 1). Crary (1960) obtained 14C ages of 400–500 years for the organic material and suggested that this was the time required for it to reach the surface after being frozen in at the bottom.
The outflow of fresh water from Disraeli Fiord has been traced by ice-core drilling and analysis of the eastern ice shelf. However, the non-saline basement ice of stratum 3 (Table I; Fig. 2) suggests that water stratification and associated fresh-water ice growth once occurred below the western ice shelf. Jeffries and Krouse (1984) suggested that this could have occurred during an exceptionally warm climatic period when the volume of fresh water flowing into and out of Disraeli Fiord was far greater than it is today. Alternatively, there could have been a pulse of water from the land to the west of Cape Alexandra (Fig. 1).
Core 86-8, south Ward Hunt Ice Shelf
Brackish ice was found to interfinger with sea ice in two deep cores drilled south-west of Ward Hunt Island (Fig. 1) (Lyons and others 1971). Core 86-8 was drilled in the same area and although it is only a 10 m core, the salinity and δ18O data set is much larger than that of Lyons and co-workers. Salinity and δ18O are plotted on an x–y graph (Fig. 5).
Salinity and δ18O are linearly related (Fig. 5) and the δ18O data show that the core contains fresh-water/meteoric ice in addition to brackish ice and sea ice. The brackish ice salinity and δ18O values of Lyons and others (1971) are also plotted for the purposes of comparison. Since ice core 86-8 contains a combination of fresh, brackish, and sea ice it is termed “combination basement ice” (Table I).
Combination basement ice appears to be restricted to an area south of Ward Hunt Island, a location that lies between the western ice shelf with inflowing sea-water and the eastern ice shelf with outflowing sea-water and fresh water. The salinity and δ18O values of the ice are evidence of accretion from fresh, brackish, or sea-water. The greater and more frequent variability of ice properties suggests that water stratification in this area is less common than below the eastern ice shelf. The variability of water properties below the ice must be related to variations in the degree of fresh-water / sea-water mixing that may be due to the influence of local sea-floor topography or under-ice topography.
Conclusion
On the basis of ice-core drilling and analysis we have attempted to determine water circulation and freezing below Ward Hunt Ice Shelf, and their relationship to the inflow and outflow of water to/from Disraeli Fiord. Our interpretation is summarized in Figurefig 6. Sea-water flows into Disraeli Fiord beneath the west shelf and, apart from one known interruption, the ice has grown directly from sea-water. Sea-water flow out of the fiord occurs beneath the east shelf, but includes a discrete layer of fresh water directly below the ice shelf. Ice growth (probably frazil) from this fresh water, in balance with surface melting, has led to the complete removal of any sea ice that once grew east of Ward Hunt Island. South of Ward Hunt Island, due to local geometry that remains to be delineated, considerable water mixing occurs. Water strata there are subject to greater and more frequent mixing, which is reflected in the growth of fresh, brackish, or sea ice. The ice cores contain a proxy record of variations in water circulation beneath the Ward Hunt Ice Shelf. Now there is a need for an extended time series of direct measurements through the deployment of current meters, tide gauges, and CTDs below the ice shelf.
Acknowledgements
Martin O Jeffries acknowledges the support of the following: Department of Geography, University of Calgary, PCSP (Director, G D Hobson), Defence Research Establishment Pacific, the Arctic Institute of North America, Gulf Canada, Dome Petroleum and Petro-Canada. H Roy Krouse acknowledges NSERC Canada funding of the stable-isotope laboratory at the University of Calgary. The ice-island project at the Geophysical Institute, University of Alaska, is funded by the U.S. Department of Energy (Morgantown Energy Technology Center). Our thanks to Dr G Holdsworth for his help with drilling ice core 83-1 and to the P.U.N.S. Expedition (1985–86) to Ward Hunt Ice Shelf (leader. Sir Ranulph Fiennes) for drilling four 10 m ice cores. We also thank the Resolute Bay weather station (AES Canada) for allowing us to store the ice cores in one of their freezers. Dr W F Weeks kindly read the manuscript before submission.