Superplastic deformation of ice: Experimental observations

By D. Goldsby, D. Kohlstedt. 2001

644 citations recorded by the source corpus.

Subfields: Atmospheric Science, Pulmonary and Respiratory Medicine

View Paper: https://www.semanticscholar.org/paper/74cc9df28bb045cc254a9c729c139bc4a2e4a5dc

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Citations in the corpus

Long-Term Stability of a Subsurface Ocean on Enceladus (2007, background): “2a, because ice viscosity is temperaturedependent (Goldsby and Kohlstedt, 2001), and the ice shell will develop a high viscosity lithosphere that is resistant to tidal deformation.”
Interior composition, structure and dynamics of the Galilean satellites (2004, background): “A major complication in the thermal modeling of the water ice-liquid outer layer on Europa is the rheology of ice (Durham and Stern 2001, Durham et al. 1997, 1998, 2001, Goldsby and Kohlstedt 1997, 2001, Stern et al. 1997) both in its control of convection and dissipation.”
Viscous flow features on the surface of Mars: Observations from high‐resolution Mars Orbiter Camera (MOC) images (2003, background): “The rheology of ice-particulate mixtures in the superplastic flow regime [Goldsby and Kohlstedt, 2001] has not been thoroughly investigated (unpublished results of Goldsby and Kohlstedt, however, suggest that ice samples alloyed with 5–10% SiC, with a particle diameter of 5 mm, do not deform…”
RHEOLOGICAL PROPERTIES OF WATER ICE—APPLICATIONS TO SATELLITES OF THE OUTER PLANETS 1 (2001, methodology): “F or p er so na l u se o nl y. P1: FUM March 17, 2001 14:11 Annual Reviews AR125-11 310 DURHAM ¥ STERN map, Goldsby & Kohlstedt (2001) select a value of 181 kJ/mol to describe the flow.”
Microstructural Evidence for Grain Size Sensitive Deformation Mechanisms in Naturally Deformed Peridotites (2002, positive): “grain boundary sliding) and is limited by either this process or the movement of dislocations within grains on the easy slip system [24,8].”
TIDALLY HEATED TERRESTRIAL EXOPLANETS: VISCOELASTIC RESPONSE MODELS (2009, background): “Typical values of G are 90 GPa for (undamaged) rocky material, and 4 GPa for icy material (Goldsby & Kohlstedt 2001).”
Tidally heated convection: Constraints on Europa's ice shell thickness (2003, methodology): “For example, using such a scaling for stagnant lid convection [Solomatov, 1995] and recent laboratory results on ice rheology [Goldsby and Kohlstedt, 1997], McKinnon [1999] showed that ice shells as thin as 10 km would be unstable against convection at their base for melting-point viscosities of…”
Oceans in the icy Galilean satellites of Jupiter (2002, background): “The rheology of ice I and H2O–NH3 ice has been the subject of a number of studies (e.g., Goodman et al., 1981; Kirby et al., 1985; Kargel et al., 1991; Durham et al., 1992, 1993, 1997, 1998; Goldsby and Kohlstedt, 1997, 2001).”
A variational approach to ice stream flow (2006, background): “However, recent work by Goldsby & Kohlstedt (2001) has suggested that a more complex combination of power laws may be a more appropriate description of ice rheology.”
Modeling climate diversity, tidal dynamics and the fate of volatiles on TRAPPIST-1 planets (2017, positive): “At the same temperature and stress conditions, water ice has a viscosity ≤ 1016 Pa s, for grain size lower than 1 mm, based on experimental data (Durham et al. 2001; Durham & Stern 2001; Goldsby & Kohlstedt 2001).”
Rheology of the Earth's mantle: A historical review (2010, background): “An important breakthrough in the study of influence of partial melt on physical properties was made by Stocker and Gordon (1975) who showed that the influence of partial melting onmechanical properties depends critically on the degree of wetting of grain-boundaries by the melt.”
Tropical mountain glaciers on Mars: Altitude-dependence of ice accumulation, accumulation conditions, formation times, glacier dynamics, and implications for planetary spin-axis/orbital history (2007, background): “An important advantage of ice-sheet modeling on Mars is that the theory of glacier flow is well characterized ( Goldsby and Kohlsdedt, 2001; see discussion in Milliken et al., 2003).”