Introduction
Conditions necessary for large-scale ice-sheet formation during Pleistocene glacial periods are not well documented because deep-sea and terrestrial records lack directly relevant atmospheric, oceanic, and geodynamic variables. It is difficult to envision, for example, how subtle changes in solar-radiation distribution culminates in the formation of ice sheets 3–4 km thick in 10 ka. Perhaps the most perplexing element of ice-sheet formation concerns marine ice-sheet inception on the continental shelves of West Antarctica and northern Eurasia (Reference Denton, Hughes, Denton and HughesDenton and Hughes, 1981). Marine ice sheets are grounded on sub-sea-level platforms and must maintain sufficient thickness to avoid floating and losing the basal friction necessary to maintain their large mass and domed elevation profile. During inception, however, those parts of marine ice sheets which form through consolidation and thickening of a floating ice cover must do so without the advantage of basal friction. Horizontal ice divergence and iceberg calving make this initial growth far more difficult than if the ice sheet were originally situated on a land surface. The formation of a marine ice sheet can thus be characterized as a competition between divergent ice-shelf flow and the ability of the atmosphere and ocean to deliver ice mass to a confined marine location.
In the present study, we examine this competition as it may have influenced the development of the present marine-based West Antarctic ice sheet. We use a time-dependent numerical model which calculates ice-shelf mass balance and flow (Reference Lindstrom and MacAyealLindstrom and MacAyeal, 1986) to simulate the evolution of an initially thin ice cover over West Antarctica as it would appear if the present glacial load were removed and the sea bed allowed to rebound as shown in Figures 1 and 2. The ice is floating where the isostatically adjusted bed is below sea-level and is grounded where the bed is above sea-level. Atmospheric and oceanic conditions, and ice fluxes into the West Antarctic region from adjacent ice in East Antarctica, are varied throughout a number of independent simulations. The results delimit circumstances under which parts of the initial floating ice cover will ground on the sea bed. Our study is intended to illustrate glaciological issues involved in marine ice-sheet formation as well as provide hypothetical scenarios to test should the geologic record permit.
Mass Balance and Water-Bucket Analogy
To form a marine ice sheet from a floating ice cover, more mass must be delivered to the ice cover by surface accumulation, basal freezing, and flux from adjacent ice sheets than is lost by basal melting and ice-front calving. Grounding is difficult to attain because horizontal ice velocity and mass advection through the seaward ice-front increase as the ice cover thickens.
The process is analogous to filling a leaky water bucket. If initially water is poured into the bucket faster than it leaks out, the water level will rise. As the level rises, however, the leakage rate may increase to a point balancing water input. If a balanced condition is reached before the water level reaches the top of the bucket, it will never completely fill.
The analogy between West Antarctic marine ice-sheet formation and the leaky water bucket is useful in describing geographic and glaciological factors that must be overcome for the ice cover to ground substantially. As shown in Figure 1, the West Antarctic continental shelf is configured as a channel extending from the Weddell Sea to the Ross Sea. The border with East Antarctica is mountainous. Gaps in this border allow the East Antarctic ice sheet (which presumably formed prior to the possibly multiple ice-sheet formation events in West Antarctica, but see Reference HughesHughes (1982)) to spill over into the West Antarctic channel, The other side of the channel facing the South Pacific Ocean, and the two ends in the Weddell and Ross Seas, are predominantly open to the sea and would permit significant ice leakage into the ocean. One fundamental advantage the West Antarctic continental shelf has over the leaky bucket is the potential for ice grounding to plug gaps and leaks. Once the ice exceeds a critical thickness of approximately 500 m, grounding on shallow sea-bed regions around the continental shelf’s periphery reduces the net floating ice-front exposure by approximately one-half. Sealing these leaks provides the key which allows the marine ice sheet to form.
Methods of Simulating West Antarctic Ice-Sheet Formation
The basic features of the finite-element model used in this study have been described by Reference Lindstrom and MacAyealLindstrom and MacAyeal (1986) and are summarized in the flow chart of Figure 3. Major assumptions and simplifications are listed in Table I. As indicated in the Flow chart (Fig. 3), stress-equilibrium and mass-conservation equations are solved to yield the instantaneous (depth-independent) velocity distribution u(x, y, t) and the ice-thickness H(x, y, t) evolution with time. The shallow ice approximation (Reference HutterHutter, 1983; see also Reference Muszynski and BirchfieldMuszynski and Birchfield, 1987) is applied to simplify stress-equilibrium conditions. Under this simplification, vertical shear stress may be disregarded and horizontal velocity may be treated as depth-independent, and the vertical stress T zz is glaciostatic.
The two horizontal stress-equilibrium equations may be written in terms of the horizontal velocity components and flow-law parameters using the method of weighted residuals (Reference Lapidus and PinderLapidus and Pinder, 1982)
and
where x and y are horizontal coordinates (with ê x and ê y as unit vectors in the x and y directions), the domain of area integrals in the entire region of floating ice, ┌ is the ice-front contour in the horizontal plane (with outward normal n ), R(x, y) and S(x, y) are arbitrary weighting functions, u and v are the x- and y-velocity components, respectively, g equals 9.81 m s−2, ρi equals 917 kg m−3, and ρw equals 1027 kg m–3. The depth-average effective viscosity is designed to represent Glen’s flow law
where e, the second invariant of the strain-rate tensor (simplified by the above approximations), is given by
B Z (Pa s1/n ) is the proportionality between strain-rate and stress, and n is the flow-law exponent taken to be 3 in this study. For simplification, we treat B Z , ρi and ρw as constants. This treatment eliminates thermo-mechanical coupling and the firn layer, which can be examined in a future study. Boundary conditions applied to Equations (1) and (2) are velocity (usually zero, see below) at ice-shelf/grounded-ice junctions and stress at the seaward ice front, and sloping underside (as shown on the right-hand sides of Equations (1) and (2).
The mass-balance equation is likewise expressed using the method of weighted residuals
where Ȧ is the snow-accumulation rate (basal melting is assumed zero), ┌’ is the grounding line (with outward-pointing normal n ′), P(x, y) is an arbitrary weighting function, and Q is the ice-volume flux specified at ice-shelf/grounded-ice boundaries. The second term on the left-hand side of Equation (5) specifies that flux through the ice front is to be passed freely into the ocean. This requirement assumes that the ice front ┌ remains constant in time, which is specified as shown in Figure 2. In contrast with the ice front, the grounding line ┌’ is allowed to advance into the ice-shelf region as the simulation proceeds. This is done by designating ice-shelf elements to be grounded when their average thickness exceeds [ρw/ρi]H b, where H b(x, y) is the sea-bed depth shown in Figure 2. Under most simulations conducted, Q is specified as zero (consistent with our assumption that grounded ice during initial stages of ice-sheet formation is stagnant). Q is specified according to regional mass-balance estimates in tests where the effects of influx from East Antarctica are considered.
Ice-shelf regions that ground during the course of ice-sheet formation are treated as stagnant ice platforms that slowly thicken with the snow-accumulation rate. These stagnant regions initially appear as ice rises within the ice-shelf domain. Their presence causes reduced seaward ice-shelf flow and catalyzes further ice-shelf grounding. In tests where East Antarctic influx is specified, Q is specified along those parts of the grounding line that border the East Antarctic ice sheet, but is zero along other grounding lines.
The validity of our simple treatment of grounded ice is tested by monitoring the magnitude of driving stress τ d over the entire grounded-ice/floating-ice domain (Reference Whillans, Veen and OerlemansWhillans, 1987)
where α is the surface slope. This test allows us to evaluate the stress level which would have driven grounded-ice flow had we chosen to treat it explicitly in our model.
Driving stress is the primary catalyst for glacial motion and is derived from gravitational forces (Reference Whillans, Veen and OerlemansWhillans, 1987). Present driving-stress values for the grounded part of the West Antarctic ice sheet range from 20 to 100 kPa (Reference DrewryDrewry, 1983, sheet 5; Reference Whillans, Veen and OerlemansWhillans, 1987). Treating grounded ice as stagnant, then, is valid so long as the driving stress remains significantly below this range (ice streams are an exception in that they flow with great speed at low driving-stress values, but they probably do not exist during the initial stages of ice-sheet formation). The areal average driving stress for the entire region originally covered by floating ice is calculated diagnostically from model output at each time step. We display the average driving stress as a function of time in Figure 4 for a number of representative simulations described below (Table II). In all simulations displayed, except those with a precipitation rate of 0.4 m a–1, the driving stress remains less than 20 kPa throughout the 3–4 ka necessary to ground the majority of the ice shelf. We conclude from this a posteriori test that grounded-ice flow dynamics, had we treated them explicitly, would have contributed little to the initial nucleation of the marine ice sheet. This conclusion does not apply to the grounded-ice dynamics that control influx from the East Antarctic ice sheet. This influx is shown by our experiments to have a significant impact on the West Antarctic ice-sheet formation. Beyond 4 ka, however, driving-stress values over grounded regions become significantly large as the ice cover thickens due to surface accumulation.
Model Experiments and Parameter Values
Twelve separate model experiments were made to test how different combinations of surface-accumulation rates, sea-level, mass input from the East Antarctic ice sheet, and B Z values affect West Antarctic ice-sheet formation. A summary of parameter values used for each run and the primary objective each run addresses is presented in Table II.
Realistic parameter values were specified for all runs except run number 1, which monitors development assuming non-deformable ice. Surface and basal temperatures of −20° C and −1.7° C, respectively, were used throughout because they closely correspond to average Antarctic ice-shelf surface temperatures (Reference Budd, Budd, Mclnnes, Jenssen, Smith, Veen and OerlemansBudd and others, 1987, table 3) and the pressure melting-point temperature at the ice-shelf base.
The average accumulation rate over present Antarctic ice shelves is approximately 0.2 m a–1 (Reference Giovinetto and BentleyGiovinetto and Bentley, 1985). This value was used over the entire region for most simulations. Runs were also made with accumulation rates of 0.1 and 0.4 m a–1, which represent reasonable variations from different atmospheric and oceanic circulation patterns. Run number 3 investigates the effect of using a non-uniform precipitation rate over the entire region. A physically reasonable variable accumulation-rate pattern over the ice shelf, shown in Figure 5, was devised under the constraint that the net mass falling on the entire ice shelf be equivalent to the 0.2 m a–1 value used in run number 2. Results of run numbers 2 and 3 vary only slightly from one another, so we conclude that the geographic pattern of snow accumulation is generally irrelevant to the issue of ice-sheet formation.
Reference Denton, Hughes, Denton and HughesDenton and Hughes (1981) suggested that West Antarctic marine ice-sheet formation is locked in phase with northern ice-sheet development through their control on eustatic sea-level. We test this hypothesis by performing a number of experiments where sea-level is instantaneously lowered by 50 m and 100 m (equivalent to the ice volume of moderately and fully developed glacial periods, respectively). Sea-level is varied in the model by specifying uniformly decreased bed depths beneath the ice shelf.
In the final three runs, we simulate ice flow into the shelf from East Antarctica and from ice which grounds adjacent to East Antarctica by imposing a non-zero ice flux at the grounding line. Flux into West Antarctica was roughly divided into three drainage systems shown in Figure 6. Initial velocities of 500, 100, and 50 m a–1 were specified at the grounding lines for the basins of Figure 6 with fluxes of 0.05, 0.03, and 0.13 Tm3 a–1 (where T = 1012), respectively. We apply these velocities arbitrarily based on current velocity conditions at ice-sheet/ice-shelf junctions and on the geographic confinement of the border through which the East Antarctic ice is discharged. The 500 m a–1 discharge velocity, for example, is specified at the narrow border presently occupied by Byrd Glacier, whereas the 50m a−1 value is specified along the lengthy boundary extending along the Weddell Sea sector.
The 124 MN m−2 s1/3 B Z value used for most runs was calculated following the method of Reference Thomas and MacAyealThomas and MacAyeal (1982) for an ice shelf having a linear temperature-depth profile with surface and basal temperatures of −20° C and −1.7° C, respectively. Run numbers 8 and 9 investigate the response to raising and lowering this value. These simulations test the influence of: (i) different atmospheric temperatures, (ii) inaccuracy of the assumed linear temperature-depth profile, and (iii) uncertainties in the flow law.
Ice-Sheet Formation
Each simulation was run for 5900 years with a 50 year time step. This was sufficiently long for the ice shelf still remaining after the simulation to attain a steady state, where the absolute values of net mass input and output are equal, except for run numbers 1, 10, and 12 of Table II. Owing to the artificial elimination of ice flow, run number 1 never reaches a steady state. Run numbers 10 and 12, however, were close to a steady-state condition, with mass loss to gain ratios of 0.97 and 0.98, respectively. The percentage of the original ice-shelf area which had grounded at the end of each run is listed in Table II. Figure 7 shows the percentage of ice shelf remaining for run numbers 2, 5, 10, and 12 as a function of time.
For the purpose of describing ice-sheet formation, we arbitrarily require 35% or more of the original floating ice-covered region to ground before accepting the run as generating a marine ice sheet. Four reasons for specifying this criterion are: (i) the present grounded part of the West Antarctic ice sheet covers 35% of our original ice-shelf area, (ii) 35% grounding is sufficient to form a substantial central grounded core instead of only isolated grounded patches, (iii) the original ice shelf is broken up into a number of separate and unconnected ice shelves, and (iv) this requirement is simple.
To display the range of parameters which permit 35% grounding, we plot in Figure 8 parameter values of all runs having a B Z value of 124 MN m−2 s–1/3 on a coordinate system with axes representing: (1) ice flux from the East Antarctic ice sheet, (ii) surface-accumulation rate, and (iii) sea-level. The boundary separating parameter ranges in which the ice sheet does or does not form in our simulations is plotted as a planar surface.
Grounded Pattern After 5900 Years
The shaded pattern of Figure 9a shows regions of the ice shelf which are presently grounded. Figure 9b–i shows the final grounding of configurations for run numbers 2, 10, 4, 6, 5, 7, 11, and 12, respectively. The heavy lines enclose regions of the original ice-shelf area which have grounded and the dashed line shows the current ice-front positions for the Ross and Filchner-Ronne Ice Shelves. These figures show that (i) the Ronne Ice Shelf region grounds very easily; (ii) the Filchner Ice Shelf grounds under conditions where the sea-level is lowered and there is ice flux from the East Antarctic ice sheet; and (iii) the Thwaites Glacier and Ross Ice Shelf regions are difficult to ground.
The Ronne Ice Shelf bed is shallow, so grounding is sensitive to changes in sea-level (Fig. 9e–g, h–i). Grounding in the region occurs most readily between the Henry and Korff Ice Rises and Berkner Island (Fig. 9c–d). A number of isolated ice rises and rumples exist in this region today (Reference DrewryDrewry, 1983, sheet 2). The Filchner Ice Shelf is much harder to ground because of its greater bed depth. Ice influx from the East Antarctic ice sheet and an increase in the accumulation rate by themselves have no influence on the grounding pattern (Fig. 9c–d), and lowering sea-level by itself has only a limited effect (Fig. 9f). A combination of ice flux from the East Antarctic ice sheet and lower sea-level, however, grounds the entire region, even if the accumulation rate is lowered (Fig. 9h, i).
The area drained by Thwaites Glacier did not ground for any simulations other than run number 1 because of its deep bed and proximity to the calving front. The bed depth allows ice to become very thick and the ice-front proximity promotes a large surface-elevation gradient. These two conditions produce a large driving stress (Equation (6)), which removes ice from the region before it has a chance to ground. We propose that grounding occurs up-stream of Thwaites Glacier today because driving stresses of adjacent grounded ice have flushed large amounts of ice into previously ungrounded regions.
The Ross Ice Shelf is hard to ground because of its moderately large bed depths and long ice-shelf front. Glacial geologic studies (Reference Stuiver, Stuiver, Denton, Hughes, Fastook, Denton and HughesStuiver and others, 1981) and sea-core sedimentological analyses (Reference Kellogg, Kellogg, Truesdale and OstermanKellogg and others, 1979), however, indicate ice was grounded in the Ross Sea basin to the continental shelf 18 ka BP. This grounding must have occurred by processes similar to those which we speculate caused grounding up-stream of Thwaites Glacier.
Ice-shelf Development Through Time
Histories of mass balance, fraction of original ice-shelf front remaining, average thickness, volume, average velocity, and fraction of original ice shelf remaining are presented as functions of time in Figures 10–14 and Figure 7, respectively, for run numbers 2, 5, 10, and 12. These runs were chosen because they represent varying degrees of final ice-shelf grounding.
As demonstrated by the histories of area-average thickness and ice volume, ice-shelf build-up generally proceeds rapidly through the first 1500 years. Following this, the build-up slows as steady-state conditions are approached. From roughly 1500 to 3000 years, average ice-shelf thickness and volume decrease for run number 12. This decrease can be attributed to selective removal of the thickest parts of the ice shelf. Smaller humps and irregularities of the curves result from small-scale regional grounding and from thickening of ice-shelf segments cut off from the ocean by surrounding grounded ice.
The leaky bucket analogy of marine ice-sheet formation described earlier is clearly evident in the histories of ice-shelf area and ice-front length, As the ice-shelf thickness builds up, and the ratio of net ice discharge to accumulation increases, the seaward ice-front length within the West Antarctic basin is shortened. This is accomplished by ice-shelf grounding in gaps between islands which enclose the West Antarctic basin and at isolated sea-bed bumps in the Ross and Weddell Seas. For those runs which are successful in forming a marine ice sheet, the ice-front length is shortened by a substantial amount, up to 30–40%. This confirms the tendency for ice-shelf grounding to seal leaks that otherwise would prevent build-up of a marine ice sheet.
Possible Scenario for the West Antarctic Ice-Sheet Development
We propose the following scenario of West Antarctic ice-sheet development based on our numerical simulation results. Ice-sheet development begins after an interglacial period where grounded ice has collapsed in regions below sea-level and isostatic adjustment of the bed has occurred, as in Figures 1 and 2.
At the early stages of the glacial period, before enough ice has accumulated in the Northern Hemisphere to lower significantly sea-level, an ice cover over West Antarctica similar to that of Figure 9c develops, with limited grounding in: (i) the central sector except up-stream of Thwaites Glacier, (ii) the Ronne Ice Shelf between Henry and Korff Ice Rises and Berkner Island, and (iii) the isolated shallow bed region up-stream of the present Ross Ice Shelf grounding line.
As sea-level falls with Northern Hemisphere ice build-up, additional grounding occurs over the Ronne Ice Shelf and in the central sector, as shown in Figure 9e. When the Northern Hemisphere’s ice sheets are near their maximum size, a grounded distribution similar to that of Figure 9i exists. Eventually, as the grounded parts develop significant driving stresses, regions up-stream of Thwaites Glacier and the Ross Ice Shelf also ground by the flux of grounded ice into the ice shelf.
Summary
Our results address answers to several questions raised concerning: (i) whether the West Antarctic ice sheet could have re-established itself if it collapsed during the Sangamon Interglacial 125 ka BP (Reference MercerMercer, 1968), (ii) what climatic conditions will be needed and how long it will take the West Antarctic ice sheet to re-establish itself if it collapses within the next millennium from atmospheric trace gas and CO2 increases (Reference MercerMercer, 1978; Reference Manabe and StoufferManabe and Stouffer, 1979; Reference Ramanathan, Ramanathan, Lian and CessRamanathan and others, 1979), and (iii) the relative importances of ice-shelf thickening (Reference WexlerWexler, 1961; Reference HughesHughes, 1982) and grounded ice flux (Reference Bentley and OstensoBentley and Ostenso, 1961) in initiating the West Antarctic ice sheet.
For the first two questions, our study has shown that a precursor to the West Antarctic ice sheet can form within several thousand years under realistic environmental conditions once sea-level is lowered in association with a Northern Hemisphere glaciation. Our result is consistent with the view that glacial events in the Southern Hemisphere are phase-locked with those of the Northern Hemisphere through eustatic sea-level (Reference HollinHollin, 1962). Flux of ice from the East Antarctic ice sheet and the accumulation rate are also significant factors, but not as important as sea-level changes.
In the third case, our results shows that all parts of the West Antarctic ice sheet can form through ice-shelf thickening alone except up-stream of Thwaites Glacier and in the Ross Sea region. Grounding up-stream of Thwaites Glacier and in the Ross Sea region occurs only after neighboring grounded ice has developed a driving stress large enough to force more ice mass into these areas. We are currently refining our model so that it can treat grounded-ice dynamics and isostatic adjustments of the bed.
Acknowledgements
This work was supported by U.S. National Science Foundation grant DPP-8401016. We thank K. Bryan, Jr, M.M. Monaghan, R.G. Grumbine, A. Ziegler, T.J. Hughes, G.H. Denton, T.B. Kellogg, B. Stauffer, and an anonymous referee for helpful suggestions and criticisms throughout the span of this project. Finally, we wish to acknowledge and dedicate this paper to John Mercer, who pioneered the study of West Antarctic ice-sheet stability.