Abstract. Grain growth can modify the microstructure of natural ice, including the
grain size and crystallographic preferred orientation (CPO). To better
understand grain-growth processes and kinetics, we compared microstructural
data from synthetic and natural ice samples of similar starting grain sizes
that were annealed at the solidus temperature (0 ∘C) for
durations of a few hours to 33 d. The synthetic ice has a homogeneous
initial microstructure characterized by polygonal grains, little
intragranular distortion, few bubbles, and a near-random CPO. The natural
ice samples were subsampled from ice cores acquired from the Priestley
Glacier, Antarctica. This natural ice has a heterogeneous microstructure
characterized by a considerable number of air bubbles, widespread
intragranular distortion, and a CPO. During annealing, the average grain
size of the natural ice barely changes, whereas the average grain size of
the synthetic ice gradually increases. These observations demonstrate that
grain growth in natural ice can be much slower than in synthetic ice and
therefore that the grain-growth law derived from synthetic ice cannot be
directly applied to estimate the grain-size evolution in natural ice with a
different microstructure. The microstructure of natural ice is characterized
by many bubbles that pin grain boundaries. Previous studies suggest that
bubble pinning provides a resisting force that reduces the effective driving
force of grain-boundary migration and is therefore linked to the inhibition
of grain growth observed in natural ice. As annealing progresses, the number
density (number per unit area) of bubbles on grain boundaries in the natural
ice decreases, whilst the number density of bubbles in the grain interiors
increases. This observation indicates that some grain boundaries sweep
through bubbles, which should weaken the pinning effect and thus reduce the
resisting force for grain-boundary migration. Some of the Priestley ice
grains become abnormally large during annealing. We speculate that the
contrast of dislocation density amongst neighbouring grains, which favours
the selected growth of grains with low dislocation densities, and
bubble pinning, which inhibits grain growth, are tightly associated with
abnormal grain growth. The upper 10 m of the Priestley ice core has a weaker
CPO and better-developed second maximum than deeper samples. The similarity
of this difference to the changes observed in annealing experiments suggests
that abnormal grain growth may have occurred in the upper 10 m of the
Priestley Glacier during summer warming.