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Premelting increases the rate of regelation by an order of magnitude

Published online by Cambridge University Press:  23 May 2019

ALAN W. REMPEL*
Affiliation:
Department of Earth Sciences, University of Oregon, Eugene, OR, USA
COLIN R. MEYER
Affiliation:
Department of Earth Sciences, University of Oregon, Eugene, OR, USA
*
Correspondence: Alan W. Rempel <rempel@uoregon.edu>
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Abstract

Glacier sliding over small obstacles relies on melting on their upstream sides and refreezing downstream. Previous treatments have appealed to ‘pressure melting’ as the cause of the spatial variations in melting temperature that drive this regelation process. However, we show that typical liquid pressure variations across small obstacles are negligible and therefore variations in ice pressure closely approximate variations in effective stress. For a given change in effective stress, the equilibrium melting temperature changes by an order of magnitude more than when the pressure of ice and liquid both change by an equal amount. In consequence, the temperature gradients that drive heat flow across small obstacles are larger than previously recognized and the rate of regelation is faster. Under typical conditions, the transition wavelength at which ice deformation and regelation contribute equally is of m-scale, several times longer than previous predictions, which have been reported to underestimate field inferences.

Information

Type
Letter
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
Copyright © The Author(s) 2019
Figure 0

Fig. 1. Generalized Clapeyron conditions for regelation. (a) Schematic of regelation past a bump. (b) Gibbs free energy per molecule of ice and liquid water. The ice lines are more shallow because ice has a lower specific entropy than liquid. Separate lines for a given substance correspond to different pressures. Intersections of ice and liquid lines correspond to phase equilibria. Consider the intersection of the two green lines (e.g. at the pressure conditions on the downstream side of a bump): at temperatures below the phase equilibrium temperature, ice has the lower free energy, and above the melting temperature, liquid prevails due to its lower free energy. The red lines show the free energy in each phase when pressure is elevated as labeled. If the ice and liquid pressures both increase by the same amount, the melting temperature decreases along the Clapeyron slope with the intersection between the dashed and the dot-dashed red lines. If, however, the ice and liquid pressures are perturbed by different amounts (e.g. at the pressure conditions on the upstream side of a bump), the melting temperature decrease can be much larger, as shown by the intersection of the two dot-dashed red lines.

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