1992
DOI: 10.1017/s0022143000003658
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Flow-law hypotheses for ice-sheet modeling

Abstract: ABSTRACT. Ice-flow modeling requires a flow law relating strain rates to stresses in situ, but a flow law cannot be measured directly in ice sheets. Microscopic processes such as dislocation glide and boundary diffusion control both the flow law for ice and the development of physical properties such as grain-size and c-axis fabric. These microscopic processes can be inferred from observations of the physical properties, and the flow law can then be estimated from the microscopic processes.A review of availabl… Show more

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Cited by 271 publications
(197 citation statements)
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“…We expect that the NGG can take place along the whole Guliya core as the recrystallization is the same at all depths of the EPICA DML core [5]. This is different from the classical tripartite paradigm of the polar ice [8,15,[42][43][44][45][46] which includes the NGG, the polygonization/rotation recrystallization (RRX), and the migration recrystallization (SIBM) from the top to the bottom down each core.…”
Section: Grain Growthmentioning
confidence: 85%
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“…We expect that the NGG can take place along the whole Guliya core as the recrystallization is the same at all depths of the EPICA DML core [5]. This is different from the classical tripartite paradigm of the polar ice [8,15,[42][43][44][45][46] which includes the NGG, the polygonization/rotation recrystallization (RRX), and the migration recrystallization (SIBM) from the top to the bottom down each core.…”
Section: Grain Growthmentioning
confidence: 85%
“…Within 10-101 m depth of the Guliya core, which possibly reflects periods of climatic warming and cooling (the grain diameter are evidently large at 44.0-51.0 m and 81.0-91.0 m, and distinctly small at 101.0 m in Figure 2) is consistent with the analysis of Lipenkov et al [23] for the Vostok3G-1 core and Faria et al [41] for the EPICA DML core, respectively. However, that the grain size of the Ice Age is significantly smaller than that of Holocene ice [8,27,30] has not been identified by the measurement of the Guliya ice core [22]. This can be explained by grains growing with age reaching a limited size where polygonization counteracts grain growth for the Holocene part of the EPICA DML core [20] and, by that, the grain growth of the North GRIP core for the last~2 ka is seen to be linear with time, while the grains older than 2 ka merely approach a constant area (Figure 2), which is probably a result of polygonization [17].…”
Section: Grain Growthmentioning
confidence: 96%
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