Experimental procedures

In order to obtain bubble-free samples with a small grain size and without initial deformation features, samples were produced using large-grained bubble-free ice obtained by slow freezing of pure water under vibration that were then exposed to a phase transition at ~300MPa, ~233K. This procedure enables us to produce small-volume samples (cylindrical: ~15–20mm diameter, ~50mm length) with small grain sizes (mean diameter ~0.6mm) due to nucleation/recrystallization processes during the phase change from ice II to ice Ih. In contrast to standard sample production procedures, which usually include pressure sintering, our samples are bubble-free, and do not exhibit deformational microstructures.

Samples were rounded using a lathe. Top and bottom surfaces were cut parallel with a microtome (cylindrical: 13–19mm diameter, and 14–38mm length). The creep machines we used consist of a basal plate, which is situated in a silicon oil bath and a loading stage lead by vertical guide rails. The silicon oil bath is used to prevent the deforming sample from sublimation and to keep the temperature constant during the test. A displacement sensor is attached to the loading stage, which moves down as the sample is compressed, and measures the shortening of the sample. Table 1 gives an overview of all experiments conducted during the study.

Table 1.

Overview of the experimental conditions. Test samples were cylindrical with diameter 13–19mm and length 14–38 mm. Temperatures are means over the duration of the experiment. In some cases it is not clear whether final strain rate is the minimum strain rate

For reference, concurrent annealing of a small section cut from the initial samples was conducted in the same silicon oil bath used for creep experiments.

Observation methods

Thin sections were prepared according to standard procedures, allowing the surfaces to sublimate and reveal (sub)grain boundaries as etch grooves (Reference KipfstuhlKipfstuhl and others, 2006). For each sample, at least two sections, one cut horizontally and the other vertically, were prepared. Microstructures were mapped afterwards with a manual XY-stage and a differential interference microscope (Olympus B × 51 differential interference contrast (DIC), 10× lens). Two to six sectors (~5 mm by 6 mm) of each section, usually chosen close to the centre of the sample and not disturbed by, for example, bad sublimation regions, were photographed with ~25 images to get a representative overview of the sample. Grain size and shape were determined from overview pictures of the whole sample between crossed polarizers (Stereoscope 12, 6× to 64×, 1 × objective).

Measurement methods

Subgrain-boundary statistics were obtained from photomicrographs using digital image analysis. Microstructure maps were assembled from microscopic mosaic images and used to measure total subgrain-boundary length in the grain assemblage presented in the map. This had to be done manually, as subgrain boundaries, in contrast to grain boundaries, appear only as thin faint lines in the images which are difficult to extract automatically. The area of the microstructure map was measured and the subgrainboundary density calculated. Subgrain-boundary density is defined as the sum of all subgrain-boundary lengths per area. Possible interrelations between subgrain-boundary density and the sample cutting scheme (i.e. horizontally or vertically cut) were investigated by systematically changing cutting schemes. These types of observations have not been reported before;this may be because, apart from the time-consuming measurements and analysis processes, standard sample production procedures include pre-deformation due to non-hydrostatic pressure (e.g. Reference Jacka and LileJacka and Lile, 1984; Reference Goldsby and KohlstedtGoldsby and Kohlstedt, 1997) which means deformation microstructures are present in initial samples. Our samples have no such initial deformation features.

Grain parameters were derived from crossed-polarizer pictures which were segmented using an edge filter, revealing the basic network of grain boundaries (Reference Gay and WeissGay and Weiss, 1999). Artefacts were removed manually. The grainboundary network pictures were analyzed with imageprocessing software to obtain grain-size (area, perimeter) data by pixel counting. The software assumes an ellipse of the same area as each grain. Using the length of the major and minor axes of this ellipse, grain-elongation data and the aspect ratio of each grain can be derived.

The ratio of convex perimeter to real perimeter (Fig. 1) called ‘perimeter ratio’ has been adopted to describe the morphology of the grains. This parameter, used here for the first time to describe the grain shape in polycrystalline ice, can be measured using Image-Pro Plus (Media Cybernetics). It was used in a similar way to measure the roughness of grains in unbound aggregates of gneiss forming a base course in road surfaces. A grain with straight boundaries has a perimeter ratio of 1;the value decreases as the irregularity becomes more complex.

Fig. 1.

Schematic illustration of the definition of convex perimeter and real perimeter measured by Image-Pro. The ratio is used as a measure of the irregularity of grains.

Creep data

Experiments were conducted to reach strains of 0.4–8.6% at ~–5°C and 0.5–1.4% at ~–23°C. Greater strains were not attempted as the apparatus was only available for a limited time. Only two of the experiments clearly reached minimum isotropic creep. In the highest-strain experiments, strain rate usually stopped decreasing at ~1–2% strain (Fig. 2).

Fig. 2.

Strain rate vs strain for all experiments.

Grain-size data

Mean grain size increased during almost all our creep tests (Table 1). Comparisons with data derived from grain-growth experiments at –5°C (Reference NishimuraNishimura, 2004) using the same sample type, produced by phase transition, indicate significantly faster increases in grain size when no stress is applied (Fig. 3). A striking difference was found between samples deformed at ~–5°C and at ~–23°C (Fig. 3).

Fig. 3.

Grain-size evolution during creep tests and Reference NishimuraNishimura’s (2004) grain-growth experiment.

Grain-shape data

Elongation, and therefore mean grain aspect ratio, slightly increases with increasing strain (Fig. 4a). At the highest strains a steady aspect ratio of ~1.7 was reached. Importantly, no difference in mean grain aspect ratio could be found between vertically and horizontally cut sections. The orientation of the majority of the grain elongations does not change significantly and no preferred grain-elongation direction could be observed.

Fig. 4.

Microstructural evolution in creep experiments with increasing strain. (a, b) Grain aspect ratio (a); grain perimeter ratio (see Fig. 1 and text for definition) (b). Mean derived from vertical and horizontal sections. (c, d) Subgrain-boundary (sGB) density (c); frequency of parallel-type subgrain boundaries (ratio of the total length of parallel-type subgrain boundaries to total length of all subgrain boundaries) (d). Mean over four to six selected regions (area: ~5mm × ~6 mm) in a section. Bars indicate variability.

We also investigated the detailed irregularity of the grains. Polygonal and regular-shaped grains, isometric with straight grain boundaries and triple-junction angles close to 120°, were observed in samples before deformation and in samples which had been annealed (Fig. 5a). Deformed samples show irregular grains with bulging and curved grain boundaries, extending into neighbouring grains to produce an interlocking texture (Fig. 5b). With increasing strain the grains become increasingly irregular. Perimeter ratio values slightly below 1 are obtained for the highly regular grains in initial and annealed samples. With increasing strain the increasing bulging of the grain boundaries and increasing localized curvature radii decrease the perimeter ratio (Fig. 4b).

Fig. 5.

Composite photomicrographs taken between crossed polarizers. (a) Initial sample. (b, c) After 3 days at –4.9°C: annealing only (b); creep test at 0.52 MPa and 3.58% total strain (c).

Subgrain boundaries and subgrain-boundary density

Reference KipfstuhlKipfstuhl and others (2006) showed that subgrain boundaries are revealed as grooves under controlled sublimation conditions. The dependence of sublimation/thermal grooving on misorientation was described generally by Reference MullinsMullins (1957) and by Reference Saylor and RohrerSaylor and Rohrer (1999) for ceramic polycrystals. Recently Reference Obbard, Baker and IliescuObbard and others (2006a) described a model for preferred sublimation and some special aspects of grain-boundary grooving for ice. As the transition from subgrain boundaries to grain boundaries is gradual, a clear definition or critical value to distinguish between the two is difficult. In materials science the transition is typically taken as between 10° and 15° (see, e.g., Reference Humphreys and HatherlyHumphreys and Hatherly, 2004, p. 92) and in geology as <5° (see, e.g., Reference Passchier and TrouwPasschier and Trouw, 1996, p.265). For ice, Reference Montagnat and DuvalMontagnat and Duval (2000) used 5° as the critical value for the transformation. Preliminary results of X-ray Laue diffractometry (personal communication from A. Miyamoto, 2007) reveal typical misorientations for strong grooves of ~3°. Faint sublimation grooves, although clearly visible, cannot be easily detected by X-ray measurements, indicating a very small misorientation (≪0.5°). Therefore it is probably correct to call some of these sublimation grooves dislocation walls rather than subgrain boundaries. The distinction is not made here, because of the gradual transition from dislocation walls to subgrain boundaries to grain boundaries. High-resolution misorientation measurements can be performed using hard X-ray equipment (Reference Montagnat, Duval, Bastie and HamelinMontagnat and others, 2003), useful for distinguishing these features, but the sample sizes are tiny and neither geometric arrangement nor statistics on substructures can be obtained.

The systematic study of subgrain-boundary density during creep tests reveals it evolves with strain (Fig. 4c). Mean subgrain-boundary density increases with strain (Fig. 4c) from ~0.5% up to ~2%. For strains larger than 2–3% the increase stops at a value of ~3.5mm^–1. No systematic difference in subgrain-boundary density or grain size was observed between horizontally and vertically cut sections. Values plotted in Figure 4c are mean values of at least four individual measurements, each determined for one microstructure map (~5mm × 6 mm of a sample surface). Particularly for strains higher than 1%, the individual measurements have a large scatter (bars in Fig. 4c), reflecting a heterogeneous distribution of deformation over the section. Figure 4c shows that the range of variability is approximately similar in all samples, ~3mm^–1 above 1% strain, which indicates that our analysis of four microstructure maps is representative. As experiments at lower temperatures take much longer, only a few data are so far available, though these agree well with the above finding.

Figure 6 illustrates the subgrain-boundary density with final strain rates measured for the experiments. Although a clear correlation cannot yet be shown, subgrain-boundary density seems to increase with strain rate. Further experiments are required to investigate the relation between subgrain evolution and strain rate.

Fig. 6.

Mean subgrain-boundary density against final strain rate. Mean over four to six selected regions (area: ~5 mm × 6 mm) in a section. Further experiments are required.

Subgrain-boundary types

Different subgrain-boundary types classified by shape, and very similar to those found in Antarctic ice (data will be presented elsewhere), have been observed. The appearance of subgrain boundaries is manifold (Fig. 7). Variations occur in shape and intensity (i.e. greyscale value). The subgrainboundary shapes vary from regular straight (rare) to regular bowed (often) and irregular zigzag or step-shaped (very often). The latter sometimes build conspicuous networks. Straight, exactly parallel groups of subgrain boundaries are striking, often appearing faint and light grey.

Fig. 7.

Types of subgrain boundaries in a vertical section (–4.88C, 0.52MPa, 8.56% total strain). GB – grain boundary; p – parallel subgrain boundary; ? – not yet classified subgrain boundary; c – classical polygonization type subgrain boundary.

The shapes of subgrain boundaries have been investigated with respect to crystal orientation using a combination of microstructure mapping and etch-pit analysis (Fig. 8), which enables a more definite classification of three subgrain-boundary types: parallel subgrain boundaries are not only exactly parallel to others in the swarm, but are also parallel to the trace of the basal plane (type p – parallel);zigzag or step-shaped subgrain boundaries usually run in one reticule direction parallel and in the other at a high angle to the basal plane (type z – zigzag);regular, more-or-less straight subgrain boundaries with the classical polygonization orientation (perpendicular to the basal plane) have also been observed (c – classical polygonization type), but almost always change into the zigzag type at one end (Figs 7 and 8). Bowed subgrain boundaries and those without any distinct shape usually do not seem to correspond with the crystal orientation and cannot be classified.

Fig. 8.

Combination of microstructure mapping and etch-pit method. Example of vertical section (–4.8°C, 0.35 MPa, 1.22% strain). (a) Sublimated surface showing grain boundaries (GB) and different types of subgrain boundaries (p – parallel; z – zigzag; c – classical polygonization type; ? – not identified). (b) Etch pits produced on same sector as (a). Short white bars indicate trace of basal plane in cutting surface according to etch-pit shape. Note: parallel type is parallel to basal plane trace; classical polygonization type is perpendicular to basal plane trace.

Due to the striking and easily recognizable nature of parallel subgrain boundaries, statistics on their occurrence have been calculated (Fig. 4d). The fraction of the length of parallel subgrain boundaries over total subgrain boundaries, and the variability, is highest in undeformed samples, because the few subgrain boundaries occurring in initial samples are often parallel. In slightly deformed samples (up to 1% strain) the parallel type represents ~20–30% of the total subgrain-boundary length, but for strains above 2% this frequency decreases rapidly to only several per cent.

Distribution of subgrain boundaries within grains

Subgrain boundaries are not randomly distributed within the grain. They accumulate along grain boundaries, i.e. they usually start somewhere along a grain boundary and fade out towards the crystal core. However, the distribution along the grain boundaries is not homogeneous. Accumulation of subgrain boundaries in some regions of grains, preferentially at edges or necks, has been observed (Fig. 9). The heterogeneous distribution can be described as a ‘core and mantle’ structure (Reference KipfstuhlKipfstuhl and others, 2006);a mantle describing the rim of the crystal with high subgrain-boundary density and the core defined by low subgrain-boundary density in the middle of a grain. This description holds for most grains.

Fig. 9.

Distribution of subgrain boundaries (marked as lines). Most subgrain boundaries are attached or close to a grain boundary (black), forming a subgrain-boundary-free core (approximately indicated by ellipses), which is not sharply defined. (a) Horizontal section (–4.88C, 0.35MPa, 1.22% total strain). (b) Horizontal section (–4.98C, 0.35MPa, 0.44% total strain). Note: Distribution inside grain is highly heterogeneous, e.g. areas of higher subgrainboundary density (top of (a)).

Detailed measurements of subgrain-boundary density give values two to five times higher near to grain boundaries (1–36mm^–1; see Fig. 10), compared to the mean subgrain-boundary density (3 and 6 mm^–1; see Fig. 4c). This difference clearly indicates the heterogeneity of the subgrain-boundary distribution within grains. Detailed subgrain-boundary density was measured choosing curved grain boundaries. An additional observation was that the majority of curved grain boundaries have more subgrain boundaries on their convex side than on the concave side (Fig. 10b).

Fig. 10.

Subgrain-boundary density in the vicinity of curved grain boundaries (–4.88C, 0.52MPa, 8.56% total strain). (a) Schematic showing how subgrain-boundary density was determined with measured areas, subgrain boundaries and curvatures. Numbers refer to the measurement. (b) Curvatures against subgrain-boundary densities. Areas on convex (●) and concave (▴) sides of the curve are shown separately.

Creep behaviour and substructure evolution

At ~2% strain (i.e. at minimum strain rate;Fig. 2) a steady value of mean subgrain-boundary density is reached (Fig. 4c). This finding indicates that strain hardening during primary creep corresponds to the evolution of the substructure of the crystal. Reference Duval, Ashby and AndermanDuval and others (1983) suggest the decrease in creep rate during this stage is due to two different hardening processes: kinematic hardening and isotropic hardening. Kinematic hardening is evidenced by partly recoverable deformation during transient strain, due to non-uniform distribution of long-range internal stresses caused by different orientations of grains which favour or hinder basal slip in the individual grain.

Isotropic hardening is the non-reversible component of strain during transient creep ascribed by Reference Duval, Ashby and AndermanDuval and others (1983) to a period of zero strain rate during stress-drop experiments. The processes leading to isotropic strain hardening can be observed directly using subgrain-boundary density data. Dislocations which accomplish plastic creep (e.g. Reference Duval, Arnaud, Brissaud, Montagnat and de la ChapelleDuval and others, 2000; Reference Montagnat and DuvalMontagnat and Duval, 2000, Reference Montagnat and Duval2004) form dislocation walls and subgrain boundaries. The synchrony of achievement of minimum strain rate and steady subgrain-boundary density suggests that the cause for this part of strain hardening is the production of obstacles which hinder the motion of dislocations. The most common obstacles for dislocations in ice are dislocation walls and subgrain boundaries. As the production of such obstacles and the prevention of dislocation motion is increased, the deformation rate keeps decreasing until a steady density of obstacles is reached. This coincides with attaining the maximum value of the subgrain-boundary density.

When an obstacle is encountered, dislocations cannot move freely and stress must accumulate. It is plausible that this stress accumulation leads to locally increased dislocation production due to sources for dislocations at nodes or steps formed by obstacles in the glide plane (Reference Ahmad, Ohtomo and WhitworthAhmad and others, 1986) and increased subgrain-boundary formation by dislocation pile-up. Three observations indeed reveal significant deformation inhomogeneity inside the sections and even inside the grains: (i) the high variability of single measurements (bars in Fig. 4c); (ii) the qualitatively observable heterogeneous distribution of subgrain boundaries (Fig. 9);and (iii) the difference between mean subgrain-boundary densities (up to ~5.5mm^–1; see Fig. 4c) and the locally measured subgrain-boundary density (up to 36 mm^–1; see Fig. 10). Not only is the internal stress of the non-uniform state due to resistance to creep between basal and other planes (Reference Duval, Arnaud, Brissaud, Montagnat and de la ChapelleDuval and others, 1983), but also the deformation within the grains is not homogeneous. This finding is in general accordance with strain gradients in ice described by Reference Montagnat, Duval, Bastie and HamelinMontagnat and others (2003) and interpreted, following Reference AshbyAshby (1970), as being associated with the storage of geometrically necessary dislocations.

Subgrain-boundary obstacles lead to a higher strain-energy accumulation than expected under the assumption that dislocations cross the whole grain, reach grain boundaries and are absorbed by them (Reference Pimienta and DuvalPimienta and Duval, 1987). This non-uniform state of strain energy within grains can be studied in the vicinity of grain-boundary curves. These areas are chosen because the existence of ‘bulges’ indicates a difference in energy across the boundary (e.g. Reference Duval, Ashby and AndermanDuval and others, 1983; Reference Barber, Barber and MeredithBarber, 1990).

The energy change, ΔE, across a migrating grain boundary is given by

where ΔE _GB is due to grain-boundary area change, ΔE _sGB is due to subgrain-boundary area change and ΔE _dis is a consequence of removal of dislocations by the passage of grain boundaries.

This energy change exerts a driving stress, P on the grain boundary:

The driving pressure on the convex side of the curved grain boundary, P _GB = (2_γGB)/R, is acting against motion to the convex side and is therefore subtracted. The grain-boundary energy, γ_GB, is ~10^–2Jm^–2 (4.2 × 10^–2Jm^–2: Reference Petrenko and WhitworthPetrenko and Whitworth, 1999;6.5 × 10^–2Jm^–2: Reference Ketcham and HobbsKetcham and Hobbs, 1969; Reference HobbsHobbs, 1974). The curvature radii, R (~0.05–0.3 mm; Fig. 10), are significantly smaller than values usually considered, which use mean grain size for such estimations.

Driving stress due to subgrain-boundary removal by sweep of grain boundaries is P_SGB = γ_SGB Δ_SGB, with γ_SGB being the subgrain-boundary energy (~γ_GB/10;Reference Humphreys and HatherlyHumphreys and Hatherly, 2004) and γ_sGB the subgrain-boundary density difference across the grain boundary.

P_GB and P_sGB can be calculated using data shown in Figure 10. Values for P_sGB (Fig. 11a) are negative or positive depending on the subgrain boundary frequency on the convex and concave sides of the grain boundary. Although P_sGB is usually positive, P_GB reaches much higher values (by two orders of magnitude) due to the very small curvature radii compared to the maxima of ^P sGB. This estimate shows that the internal strain energy contributed by the subgrain boundaries is not enough to produce the observed curvature radii. Grain-boundary motion is not affected by subgrain boundaries themselves, although frequently observed pinning of grain boundaries at intersections with subgrain boundaries (Fig. 12) indicates there are exceptions. As dislocations collected in subgrain boundaries or dislocation walls do not provide enough internal strain energy to produce the observed curvatures, internal energy exerted by more randomly distributed dislocations must be operating (also estimated in Fig. 11a). Thus subgrain-boundary occurrence indicates a higher dislocation density accumulated around them by acting as obstacles.

Fig. 11.

(a) Driving pressures on the convex sides of the curved grain boundaries calculated from curvature radii (P _GB) and subgrain-boundary density measurements (P _sGB) (Fig. 10). Minimum driving pressures by dislocations to keep these curvature radii are also given (P _dis). Note the second y axis with a larger scale for (P_sGB). (b) Minimum dislocation density excess which has to be larger on the convex side for the radius of curvature to remain stable, estimated from minimum driving pressures by dislocations.

Fig. 12.

Extensive interaction of subgrain boundaries with grain boundaries. (a) The geometry indicates pinning of a moving grain boundary by the subgrain boundary (–4.5°C, 0.35 MPa, 2.8% total strain). (b) Conceptual model; the grain boundary is moving towards the top of the picture (arrows indicate direction of movement) and the subgrain boundary pins it where they meet, in a similar way to particle-pinning of grain boundaries.

The driving pressure caused by removal of dislocations other than those which comprise dislocation walls or subgrain boundaries is P_dis = 0.5Δp_disGb² (e.g. Duval, 1985; Reference Humphreys and HatherlyHumphreys and Hatherly, 2004), where Δp_dis is the minimum dislocation density excess which has to be larger on the convex side for the radius of curvature to remain stable, G is the shear modulus (35.2 × 10⁸Nm^–2; Reference Petrenko and WhitworthPetrenko and Whitworth, 1999) and b is the Burgers vector of a perfect dislocation in the basal plane (~0.5 nm;Reference Hondoh and HondohHondoh, 2000). Considering motion of the grain boundary to the convex side as indicated by the bulging, P in Equation (2) must be positive (P > 0). ∆p_dis can then be estimated (Fig. 11b). Minimum dislocation densities reach values of 10¹²m^–2, one to two orders of magnitude higher than previously estimated (Duval, 1985) or modelled (Reference Montagnat and DuvalMontagnat and Duval, 2000) for bulk ice samples. Dislocation densities locally increased by subgrain boundaries acting as obstacles can produce enough internal energy to initiate strain-induced grainboundary migration during the early stages of creep.

Grain-growth reduction during deformation

The parabolic growth law which describes the grain growth of ice crystals in firn (Reference GowGow, 1969), and which is widely applied to ice in ice sheets,

can be applied to grain-growth experiments with no applied stress (k ≈ 5.1 × 10²mm²a^–1; Fig. 3). The growth rate, k, is temperature-dependent.

Grain-size data from creep experiments indicate that grains grow during deformation, but growth is significantly slower than during grain growth with no loading at the same temperature (Fig. 3). We observe an influence of temperature on grain-size evolution during primary/secondary creep (Fig. 3). Reference Jacka and LiJacka and Li (1994) suggest the dependence of grain-size evolution on stress during steady-state tertiary creep is largely independent of temperature. Although creep clearly reduces grain growth during creep tests, we cannot find an explicit dependence on stress. An explanation might be that due to the fact that our experiments do not represent the tertiary creep stage, the measured grain sizes can be regarded as intermediate stages moving towards the steady-state crystal size described by Reference Jacka and LiJacka and Li (1994). Creep experiments at conditions chosen here indicate both temperature and stress dependence of grain-size evolution. This suggests that primary and secondary creep provide a transition between the dependence of grain size on temperature and its dependence on stress.

During experiments which take place at annealing conditions, static grain growth influences grain size and grains can grow according to the grain-growth constant, k, for a given temperature following Equation (4). Additional processes affecting grain size take place during creep (Reference Gow and WilliamsonGow and Williamson, 1976). Whether these effects compete with or support normal grain growth probably depends on initial grain size, and possibly on other factors such as stress and, eventually, strain rate. Our experimental conditions enable processes which reduce grain-growth rates. As grain size moves towards a stress-dependent tertiary steady-state value, the reducing effect of deformation on grain growth is expected to be small with small stress (fig. 3 in Reference Jacka and LiJacka and Li, 1994). Experiments conducted at 0.18MPa clearly show the reduction of grain growth by creep (Fig. 3). However, further experiments are required to clarify whether a threshold stress is needed for the competing processes in grain growth at very small stresses (i.e. <0.18 MPa).

In the following we consider three micro-processes that could be responsible for the grain-growth reduction: (1) effects of soluble and insoluble impurities on mobility of grain boundaries and driving stresses; (2) splitting of grains by subgrain-rotation recrystallization (polygonization);and (3) migration recrystallization by locally very high grainboundary migration rates and/or by nucleation of new strain-free grains.

• (1) The inhibition of grain growth by impurities and particles that is often seen (Reference Alley, Perepezko and BentleyAlley and others, 1986; Reference Thorsteinsson, Kipfstuhl, Eicken, Johnsen and FuhrerThorsteinsson and others, 1995) can be excluded here, because pure-water ice has been used to produce the samples. Therefore the grain-growth reduction, observed in these experiments, must be caused by deformation, even though only low total strains are reached.

• (2) Although significant fabric change and intense grain rotation are not expected at these low strains (Reference Azuma and HigashiAzuma and Higashi, 1985), subgrain-boundary formation takes place;it is the first stage of splitting of grains by subgrain-rotation recrystallization. Unfortunately fabric data could not be obtained systematically due to the small sample size with relatively small crystal numbers per thin section after tests and problems with application of the etch-pit method. However, the extent to which subgrain boundaries contribute to grain-growth reduction depends on the development into high-angle grain boundaries. Further rotation of subgrains and therefore further deformation is needed. Additionally, removal of subgrain boundaries by grain-boundary migration needs to be considered. Providing a first stage of polygonization, subgrain boundaries contribute to grain-growth reduction. However, a direct correlation between higher subgrain-boundary density and smaller grain size during or after deformation cannot be shown.

• (3) Migration recrystallization is described typically as the nucleation of new strain-free grains and the fast migration of grain boundaries (e.g. Reference Duval and CastelnauDuval and Castelnau, 1995), including two phenomena (strain-induced grainboundary migration (SIGBM) and recrystallization with nucleation) whose main characteristics are alike in that internal strain energy and relatively high temperatures are needed. Nucleation easily decelerates grain growth by production of small grains. However, this explanation is unlikely because true nucleation textures or grain nucleation near grain boundaries, which are visible in high-resolution microstructure maps of sublimation features, are not observed in our experiments. The spontaneous nucleation process is difficult to achieve, requiring very high internal strain energies and high temperatures and, possibly, preferably oriented nucleation seeds. If one of these conditions is not adequately fulfilled, dynamic recrystallization always starts with SIGBM. Although usually described as causing high mean grain size due to the very high grain-boundary migration rate, SIGBM can reduce grain growth. SIGBM is evidenced by irregular grains (Fig. 5) with curves of grain boundaries producing interlocking textures (Reference Duval and CastelnauDuval and Castelnau, 1995; Reference Goldsby and KohlstedtGoldsby and Kohlstedt, 2002). The bulging grain-boundary curves can be cut off from the parent grain by further grain-boundary motion, to build a new, small grain with a similar orientation to the parent (Reference Humphreys and HatherlyHumphreys and Hatherly, 2004, p.251). Additionally, SIGBM can lead to apparent grain-growth reduction by three-dimensional duplication effects (studied in detail by Reference Nishida and NaritaNishida and Narita, 1996) emerging only with interlocking textures: a single grain appears plurally in one section due to its multiple protuberances. It is inevitably counted and measured as two or more grains and therefore significantly decreases the measured mean grain size (also discussed by Reference GowGow, 1969; Reference Alley and WoodsAlley and Woods, 1996). The occurrence of SIGBM is measured in creep samples using the perimeter ratio (Fig. 4b) and has been shown by estimates of local dislocation densities and observations of bulging grain boundaries. Irregularity is dependent on strain and indicates that the contribution of SIGBM to the deceleration of grain growth during deformation is important in these strain regimes.

Implications for subgrain-boundary-formation processes

It is known from other materials that the orientation of subgrain boundaries depends on the orientation of slip systems of dislocations accumulating in the grain (Tre´pied and others, 1980). As the dominant slip system in ice lies in the basal plane and other slip systems contribute much less to ice deformation (Reference Hondoh and HondohHondoh, 2000), the different orientations and arrangements of subgrain boundaries give insights into basic considerations about how they are formed. Clearly these thoughts need to be inspected in more detail using full crystal orientation measurements, which are now becoming available (Reference Montagnat, Duval, Bastie and HamelinMontagnat and others, 2003; Reference Miyamoto, Shoji, Hori, Hondoh, Clausen and WatanabeMiyamoto and others, 2005; Reference Obbard, Baker and SiegObbard and others, 2006b).

The type-c subgrain boundary (straight and basal plane orthogonal) can be explained by considering the classical, and so far only, formation process described in ice (Reference NakayaNakaya, 1958). A tilt boundary is built by pile-up and alignment of edge dislocations gliding on the basal plane during bending of the crystal.

Type-p subgrain boundaries (regular, straight and parallel to the basal plane) cannot be formed by bending of basal planes, but might be explained by analogy with the tilt boundary, i.e. as pile-up and accumulation of screw dislocations (Reference Weertman and WeertmanWeertman and Weertman, 1992). The occurrence of this dislocation type in ice was shown by Reference Montagnat, Duval, Bastie and HamelinMontagnat and others (2003). A second possible interpretation for p-type subgrain boundaries might be micro-shear zones, which have been observed by Reference Bons and JessellBons and Jessell (1999) in a rock-analogue material. In shear zones (of micrometres to kilometres) observed in rocks, a distinct package of material undertakes a high portion of the total strain of the bulk sample. In contrast to normal slip on basal planes accomplished by dislocations, a wider region of atomic layers consisting of several tens of layers is deformed while the bulk above and below the shear zone remains relatively undeformed. In our experimentally deformed samples, this type of subgrain boundary is quite unlikely, because a distinct grain geometry is needed for micro-shear zones (Reference Bons and JessellBons and Jessell, 1999). However it has been observed in Antarctic ice (S. H. Faria and others, http://www.mis.mpg.de/preprints/2006/prepr2006_33.html).

Type-z subgrain boundaries (zigzag or step-like) probably consist of tilt boundaries formed by edge dislocations on basal and non-basal planes. As most grains are not oriented to preferably build one type of dislocation, they probably form several dislocation types which align to type-z subgrain boundaries. However, motion of dislocations in many directions (climb and glide) is necessary to obtain sections of relatively pure tilt or twist boundary. Preliminary X-ray Laue measurements confirm the existence of tilt and twist boundaries (personal communication from Reference Miyamoto, Shoji, Hori, Hondoh, Clausen and WatanabeA. Miyamoto, 2007).

The rapidly decreasing frequency of type-p subgrain boundaries (Fig. 4d) shows that they are not produced under our conditions and suggests that it is the other types (c and z) that are produced in our experiments.

Outlook: similarity of high- and low-stress microstructures

Experiments have been conducted at stresses between 0.18 and 0.52 MPa. Compared with the polar ice sheets, where driving stresses are typically <0.1 MPa, measured deformation rates are very high. It is interesting, then, that observed ice substructures are very similar in deformed artificial ice and ice from deep Antarctic ice cores, especially as the experiments reached only secondary creep whereas polar ice deforms, predominantly, in near-steady-state tertiary creep.

As mentioned above, the typical shapes and arrangements of subgrain-boundary types found in the experimentally deformed ice have been characterized in an Antarctic ice core (EDML;data will be presented elsewhere). Due to this observation and the high mechanical anisotropy of ice it can be assumed that these structures are, indeed, characteristic traces of deformation processes displaying the material’s response to creep. The similarity between the subgrainboundary types can be explained by the preponderance of internal dislocation slip for the deformation of polar and artificial ice (Reference Duval, Ashby and AndermanDuval and others, 1983; Reference Montagnat and DuvalMontagnat and Duval, 2000). A difference might be found in the fraction of the different subgrain-boundary types. In our experiments the fraction of parallel-type subgrain boundaries decreases rapidly with strain, yet this is the most common kind found throughout the deep ice core. This finding suggests further studies are necessary to learn about the activity of dislocation types in low- and high-stress regimes. Furthermore, distributions of subgrain boundaries inside grains are very similar. In both cases, substructures are observed close to grain boundaries forming a ‘core and mantle’ structure. The accumulation at protruding parts of grains strikingly indicates that strain accumulation is the rule rather than the exception in deforming ice in general. The preponderance of subgrain boundaries on the convex side of grainboundary curves (Fig. 10) has also been observed in ice sheets, suggesting that local dislocation-density peaks can also occur in ice at low stresses. Most surprising is that mean subgrain-boundary density is of the same order in high-stress experiments Ị~4mm^–1; see Fig. 4c) and in the EDML ice core (~2 mm^–1). The slightly lower values in ice deformed at low stresses can be explained by recovery processes which can act with the prolonged duration of creep.

Alongside other similarities in substructure observed in experiments and in ice cores, the evolution of grain growth and especially its dependence on creep should be investigated. This requires further examination of strain-rate effects, impurity effects and other possible factors. In experiments the grain-growth reduction is already significant at low strains. At the higher strains in polar ice it is possible that strain inhomogeneities in layers of the ice sheet lead to significant differences in grain size;further work is required to clarify this. However, deformation needs to be considered as a possible cause for grain-size variation in ice cores.