Introduction

The Law Dome, previously referred to as the Wilkes local ice cap by Reference BuddBudd (1968,1969,1970) is about 200 km diameter and reaches 1390 m elevation at its summit. The ice cap overlays an irregular bedrock rise which averages about 300 m elevation near the centre where the ice thickness is about 1 100 m. To the north the ice cap runs into the ocean where the bedrock is about 200-400 m below sea-level. To the south the ice flows into a deep bedrock depression joining the Totten and Vanderford Glaciers, and there it merges with the main East Antarctic ice sheet at the bottom of the surface valley (cf. Fig. 1). The Law Dome thus represents an ideal medium-scale ice cap which is conveniently situated near Casey (lat. 66° 16.7' S., long. 1 10° 32.1' E.), about 2 km south of the former station Wilkes.

Fig. 1. Law Dome surface and bedrock elevations are shown with the locations of the bore-hole sites

Following the initial work of the United States glaciologists, Reference Cameron, Cameron, Loken and MolholmCameron and others (1959) and Reference Hollin, Hollin, Cronk and RobertsonHollin and others (1961), the Australian National Antarctic Research Expedition (ANARE) glaciology programs have concentrated on collecting data over the Law Dome and south to the East Antarctic ice sheet towards Vostok. Much of this earlier work has been reported by Reference BuddBudd (1966,1969). A summary of the glaciological work to that date is given by Reference BuddBudd (1970) and of the geophysics by Reference Allen and WhitworthAllen and Whitworth (1970).

Since then the 16 km grid network over the ice cap for elevation and ice thickness has been completed by L. Denham in 1970 using radio-echo profiling and continuous barometric levelling. This has now provided a relatively sound basic set of data over the ice cap for surface and bedrock elevation, ice thickness, and accumulation rate (cf. Figs 1 and 2).

Surface velocities and strain-rates have been measured from the centre to the coast around a large northern triangle and a smaller triangle to the south. The results of these measurements are illustrated in Figure 2.

Fig. 2. Measured net accumulation rates and velocities over Law Dome show a gradient of greatly increased flux from west to east

2. Surface Mean Temperatures

Temperatures to the depth of 10 m in the firn have been measured at many locations over the ice cap. In general the data above 400 m confirm the pattern of variation of mean surface temperature with elevation of approximately 1 deg/100 reported by Reference Cameron and MellorCameron (1964). Below 400 m Cameron indicated that the 10 m temperatures were up to several degrees warmer (than indicated by the above linear relation. Detailed measurements of temperature at eight levels to 16 m reported by Reference Cameron, Bull, Wexler, Wexler, Rubin and CaskeyCameron and Bull (1962) showed that the 10 m temperature at a site 262 m in elevation over a period of two years had a mean 3 deg warmer than the surface, This phenomenon has been observed primarily in regions of ablation where the ice has a dear “blue ice” appearance. Reference Budd and OuraBudd (1967) showed that the differential absorption of solar radiation with depth in blue ice could account for the measured variation in mean annual temperature with depth and the resultant higher 10 m temperatures relative to the surface.

The line from the Dome summit to Cape Folger, some 20 km to the north-cast of Casey seems to reach the ablation zone on the average just beyond the first bore hole at strain grid A of the northern triangle corner where the elevation is 280 m. As a result the measured 10 m temperatures along this line conform closely to the 1 deg/100 m relation.

A certain amount of variability can be expected in 10 m temperatures due to longer-term variations in mean surface temperatures. For example the record of annual mean temperatures for Wilkes-Casey are shown in Figure 3. The similarity of these temperatures with those of Mirny and Dumont d’Urville shown by Reference BuddBudd (1975) suggests that they reflect real, large-scale, changes of amplitude of about 1 deg over a time period of many years. This kind of surface-temperature variation could give rise to variations of amplitude several tenths of a degree at the 10 m level from one year to another. Below 20 m only much longer-term changes are expected to be apparent.

Fig. 3. The record of annual mean temperatures from Wilkes and Casey are shown together with those of the neighbouring stations Mirny and Dumont d’Urville (from Reference BuddBudd, (1975)

3. Tempekature-Depth Gradients

A number of temperature—depth gradients below 20 m from the coast to the interior of Law Dome were measured in 1961 by Budd (cf. Reference BuddBudd 1966). In 1962 A. Battye continued with further gradients to over 60 m depth on Law Dome and extended them inland towards Vostok. These temperature gradients were generally clear linear trends of temperature below 20 m and on Law Dome showed a smooth trend of decrease in gradient from about 3 deg/ too m near the coast to 0.25 deg/100 m 87 km inland. It was shown by Reference BuddBudd (1966) that this trend of the surface gradients could be explained in terms of the heat conduction from the base with the measured ice thickness and accumulation rates and the expected motion of the ice.

The acquisition of accurate ice-movement data over the Law Dome made it practical to carry out a more detailed analysis of the temperature profiles. The model developed by Reference BuddBudd (1969) as an extension of the original ideas proposed by Reference Robin.deRobin (1955), accounted for the measured positive gradients on the western side of Law Dome and the negative gradients along the Casey-Vostok route. In addition negative gradients of up to —2 deg/100 m were calculated for a flow line towards Cape Poinsett (cf. Reference BuddBudd, 1970, and Fig. 7). On both sides of the Dome the basal temperatures were calculated to approach melting point towards the coast.

4. Deep Temperature Profiles

Deep core drilling on the Law Dome was commenced in 1969 with a thermal coring drill of a modified CRREL design constructed by Antarctic Division (cf. Reference Bird and BallantyneBird and Ballantyne, 1971). A hole was cored to the depth of 324 m, about 7 km inland from the Cape Folger coast where the ice thickness is about 340 m. An open dry hole was used and severe closure and shear prevented temperature measurements below 224 m. The measured temperature profile is shown in Figure 4, with an extrapolation to pressure melting point at the base. This extrapolation to the base involves a decrease in temperature gradient from 3.5 deg/100 m to 2.8 deg/100 m. Such a reduction is necessary unless an isothermal layer were to exist near the base, which would prevent the geothermal flux penetrating the ice above. As shown in Figure 4, the profile shows a measured maximum gradient equivalent to the combined heat (flux of the geothermal gradient and the internal healing produced by a shear stress of about one bar and a velocity of about 10 m a-¹ The resultant geothermal gradient at the bed is the n compatible with the base gradients inferred from the more stagnant ice above the shear moraine directly inland from Casey.

Fig. 4. The temperature profiles measured in the two CapeFolger bore holes about 3 km apart are shown together with isotherms in the ice. These enable horizontal temperature gradients to be obtained.

The second deep hole cored in 1989 was at the summit of Law Dome to a depth of 380 m. In this case operational difficulties prevented temperature measurements below 320 m. The resultant profile is shown in Figure 5. Except for a slight warming of the upper layers the profile below 200 m is very close to isothermal. This was expected from the high accumulation rates and increased thickness at that location as calculated by Reference BuddBudd (1969, fig. 4.16). The warming in the upper layer could be a result of either a few tenths of a degree climatic warming over the last century or so, or a lowering of the summit of the order of 20 cm a~1’ over the same period, or some combination of both of these effects. The preliminary coarsely spaced ^l6O/¹⁸O isotope profile given by Reference Budd, Morgan and Zinderen Bakker vanBudd and Morgan (1973) supports such a long-term warming except in the top 20 m where errors due to sampling are large. An accurate analysis of this temperature and isotope data is awaiting a clear calibration of the isotope profile for the period of climatic record at Wilkes-Casey of 18 years. On the other hand a general lowering of about the above amount is suggested from both mass-balance and gravity measurements (cf. Reference BuddBudd, 1970).

In 1972 a number of medium-depth holes (50-120 m) were cored in special strategic positions over the Dome. One was near strain grid J, the corner of the triangle inland of Cape Poinsett, to see if the predicted highly negative gradients occurred there. Two other holes were cored at positions p and B, which are about 20 and 40 km respectively up-stream from the hole at A. These holes were cored to obtain isotope profiles up-stream of A and also to confirm the decrease in temperature gradients inland along the flow-line as obtained from the steady-state flow-line calculations.

Fig. 5. The measured temperature profiles are compared with the steady-state profiles computed from the present regime along the two lines from the Law Dome summit to Cape Folger and to Cape Poinsett. The line to Cafe Poinsett shows the development of the large negative temperature depth gradients at the surface in contrast to the high positive gradients on the Folger line

The measured temperature profiles are shown in Figure 5. The results clearly confirm the decrease in surface gradients going inland in a smooth systematic manner. Measurements are now available for deep surface-temperature-depth gradients at seven locations approximately along a flow line from the Dome summit to Cape Folger. These are shown in Table I and Figure 5.

In 1974 the core drilling program was aimed at obtaining an additional core and bore hole to near the bed a few kilometres up-stream from the previous Gape Folger hole with the object of determining in addition to the temperature profile, a velocity-depth profile to cheek measured flow profiles of the ice core with the in situ shear rates of the ice sheet.

The program was reasonably successful. However, high closure rates and shear rates were encountered in the lower part of the hole. The ice thickness was measured as 390 ±10 m by using the radio-echo sounder. Core was obtained to the depth of 350 m. Temperatures were measured to about 320 m. Some inclination and inclination change measurements were also made to this depth and the bore-hole diameter logged to 31 7 m. The bore hole was then filled with fluid in order to maintain the remainder of the hole open for further inclination measurements.

The bore-hole deformation and the ice-core flow and crystallographic properties will be reported elsewhere. An initial examination of the crystallography from the first hole is reported by Reference BuddBudd (1972).

For the moment we turn to the temperature profile shown in Figure 4. Here one of the most interesting features is the slight decrease in the gradient in the lower part of the measured profile. This is supported by the extrapolation to the bedrock at 390 m and pressure melting point. If the base temperature were colder than pressure melting point then the reduction in gradient would need to be even greater. As it stands the gradient decrease from 3.5 deg/ too m to 2.8 deg/100 m can be accounted for by the addition of internal heating. This is brought out more clearly by the modelling analysis of the temperature profiles. It is apparent from the calculations of long-term temperature changes by Reference Budd and YoungBudd and Young (1976) that the effects of the large Ice-Age temperature change would have penetrated well into the bedrock. Hence attention will be primarily given here to steady-state calculations.

5. Mathematical Analysis Of Temperature Profiles

The temperature profiles near Cape Folger have been analysed by a number of models of both the flow-line and column types described by Reference Budd, Budd, Jenssen and RadokBudd and others (1971) and Reference Budd and YoungBudd and Young (1976).

For example consider the column model in which x is the horizontal coordinate in the line of flow, z is the height above the base, u and w are the corresponding velocities then, for the temperature θ at time t

where K, p and c are the ice conductivity, density and capacitance respectively and Q _z is the internal frictional heating at height z.

The heating is given by

where a is the mean surface slope, Z is the ice thickness, and g is the gravitational acceleration. We assume that the flow law is given by a relation of the form

where ξ_o the octahedral shear strain-rate and is a function of the octahedral shear stress T ₀,

the temperature θ* below pressure melting point θ_m, and f which is a factor appropriate for the crystallographic orientation fabric of the ice. From the bore-hole and core data, θ* and f can be prescribed as a function of depth.

When other stresses are negligible this then gives for the horizontal shear strain-rate

These equations for the velocity and temperature profile can be solved simultaneously with the following boundary conditions to give both profiles,

(a) Two temperatures θ₁ and θ₂ at two different levels Z ₁ and z ₂ or a temperature θ at one level z ₁ and a temperature gradient (dθ/dz) at one level z ₂.

(b) The horizontal velocity at the base is taken as zero.

For the vertical velocity we adopt the relation given by Reference Budd and YoungBudd and Young (1976)

where Ū_z is the average velocity to the height z and v is the average velocity through the whole column.

Thus either the average velocity or surface velocity could be provided together with a form of the flow law (containing an arbitrary factor) or the flow law could be prescribed explicitly and the velocity calculated. In most cases the velocities are known more accurately than the flow properties of the ice so that the former procedure is usually adopted.

Fig. 6. For the Cape Folger bore hole the measured profile and a profile computed from the present regime are shown to agree broadly except for a slight warming of the surface and possibly greater internal heating above the base.

A number of theoretical profiles have been scanned using different values of the vertical velocities and the horizontal temperature gradients. Closer fits can be obtained with a number of different possible combinations of these parameters but at this stage we are interested in the closeness of the approximation of this profile to steady-state tinder the present regime Figure 6 shows an example of a calculated profile using values of the input as close as possible to the measured values. The matching is reasonably close over most of the profile but an apparent warming of a few tenths of a degree exists at the surface. As mentioned earlier this warming is noticeable in other profiles around the dome and could be associated with either a climatic change or an elevation lowering. This effect will be treated elsewhere in conjunction with the isotope studies.

6. Flow-Line Profiles

The above column model has also been used with moving coordinates along flow lines to derive a series of temperature profiles, particle paths, and ages to compare with the measured profiles. Figure 5 shows the measured and calculated temperatures along the Dome summit-Gapc Folger line. The agreement in the surface gradients is very striking.

On the eastern side of the northern triangle the regime is remarkably different from the western side as shown in Figures 1 and 2. Along the Dome—Poinsett line the accumulation rates are several times higher. The bedrock is somewhat steeper towards the coast and this results in greater slopes and shear stresses. As a result the horizontal velocities are very much higher. The effect on the temperature profiles is dramatic. Instead of a trend to increasing positive gradients towards the coast the gradients towards Gape Poinsett become increasingly negative to 2 deg/100 m near J. This value agrees closely with the increased gradient there as shown in Figure 5.

As a result the average temperature through the ice for similar elevations and surface temperatures are lower on the eastern side than the western side. This has been further confirmed by the radio-echo strengths measured by D. Carter in 1967 which were generally several decibels higher for equivalent ice thickness and surface temperature on the Dome-Poinsett line compared to the Dome Folger line.

In spite of some irregularities due to the rough bedrock profiles, there is a tendency for the base temperatures along each line to approach pressure melting point towards the coast and also in deep hollows of the bedrock, as shown in Figure 7.

7. Conclusions

The temperature profiles measured in the Law Dome conform closely to the profiles calculated from steady-state under the present regime except for a slight warming in the firn zone near the surface of a few tenths of a degree. This warming could be caused by some combination of climatic warming during the last century or so, or slight lowering of (he ice sheet.

The calculated temperature profiles from steady-state provide a sound basis for calculating the flow parameters of the ice from the measured surface velocities. These flow properties need also lo be studied in association with the ice-crystal orientations.

The high bore-hole closure rates prevent much deeper drilling with the present open-hole system. It is important to obtain deeper profiles of temperature and inclination change. The development of melt-sonde probes and ice drills operating in fluid-filled holes will be required for this.

Fig. 7. The calculated temperature profiles are shown for the lines from the Law Dome summit to Cape Folger (above) and to ' Cape Poinsett (below) superimposed on the surface and bedrock profiles. The basal temperatures tend to approach melting point towards the coast and in the deeper bedrock hollows

Acknowledgements

The results presented here have been obtained over many years with support provided by Antarctic Division personnel in the field and in Australia. In particular Mr I, G. Bird has been responsible for the development of the drilling equipment and bore-hole instrumentation, Mr R. Anderson for the drilling at Casey in 1969 and Messrs D. S. Russell and K. W. Gooley for the field program of 1974- The authors express their appreciation for the contribution of all these colleagues.

Discussion

W. D. Harrison: Could the failure of the measured and calculated temperatures to match some distance above the bed be due to enhanced deformation (and hence heating) from bed irregularities? If the ice were sliding over a sinusoidal bed, for example, this distance would be about 1/k where k is the wave number.

W. F. Budd: The difference seems to be the other way, i.e. somewhat less heat than required to increase the gradient from the base to the measured level. Thus, it seems the lower part of the ice could be less mobile than expected.

L. Lliboutry: Owing to lateral differences in ice temperatures, the direction of flow may differ from the direction of the steepest surface slope. Have you observed such an effect on the northern side of your ice cap?

Budd: Inclination measurements made in the 1974 bore hole have been repeated over only a short interval. These suggest there may be some divergence of the flow at depth towards the west, but at this stage these results are still tentative.

M. M. Miller: Geologists versus physicists may view the concept of steady state in different time frames. Will you explain what are the parameters of your definition of a glacio-thermal steady slate in terms of the boundary limits involved, the constancy or inconstancy of temperature at given levels, and lastly in terms of the other key factors affecting the regime of the total system.

Budd: A steady-state ice cap is an abstract concept which considers a model for which all its properties, such as its temperature and velocity distributions as well as the boundary conditions, are all constant with time. This concept is useful for comparing the properties of such a model with a real ice cap in order to study how the real one may have changed with time.

T. J. Hughes: The effect of ice fabric on steady-state creep rates is quite important. You reported a three-fold increase between random and single-maximum fabrics for separate ice-core specimens tested in simple shear at 0.5 bar and —6°C I found an eight-fold increase when an initially random ice fabric was deformed in simple shear at 1.0 bar and – 3° C until a strong single-maximum ice fabric developed in the same specimen. But when a similar ice specimen was tested the same way at 0.5 bar, there was no significant recrystallizalion after eight months and I could not be sure that transient creep still was not important.

How do you assess the effect of stress and temperature on the time needed to reach a stable ice fabric and steady-state creep? Have you been able to quantify these effect?

Budd: The time required depends strongly on temperature. We did some recrystallization studies on core ice at 0.2°C for several months; quite strong fabrics developed. But at —2°C, over six months, the recrystallization was very small.

J. W. Glen: What was the method of conducting a simple shear test?

Budd: We cut a to cm diameter core into sections of thickness small compared with the diameter. We fit plates to the top and bottom and run these plates parallel in bearings which keep the separation constant. We do see end effects in polarized light but we believe that the bulk of the sample is in simple shear.

C. F. Raymond: Did you check whether reloading of core samples produced any structural changes in them?

Budd: The low-temperature, low-stress test samples remaining in steady state have been examined and found to show no noticeable crystal size or fabric changes. Special recrystallization experiments however show that strong recrystallization fabrics develop after several months at —0.2°C for 1 to 2 bars loading. During this time the strain-rates go beyond the initial steady state to a higher tertiary-state creep rate.

W. S. B. Patfrson: Have you measured temperatures in fluid-filled holes and if so, have you any guidance as to whether they are perturbed by convection in the fluid?

BUDD: NO. We have only recently filled the new Folger bore hole with fluid. This will be an interesting Future study there.