Ocean interactions with the base of Amery Ice Shelf, Antarctica


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hhellmer [ at ] awi-bremerhaven.de

Abstract

Using a two-dimensional ocean thermohaline circulation model, the cavity shape beneath Amery Ice Shelf was varied in an attempt to reproduce the 150-m-thick marine ice layer observed at the "G1' ice core site. Most simulations caused melting rates which decrease the ice thickness by as much as 400 m between grounding line and G1, but produce only minor accumulation at the ice core site and closer to the ice front. Changes in the seafloor and ice topographies revealed a high sensitivity of the basal mass balance to water column thickness near the grounding line, to submarine sills, and to discontinuities in ice thickness. Model results showed temperature/salinity gradients similar to observations from beneath other ice shelves where ice is melting into seawater. Modeled outflow characteristics at the ice front are in general agreement with oceanographic data from Prydz Bay. Results concur with Morgan's inference that the G1 core may have been taken in a basal crevasse filled with marine ice. -from Authors



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Published
Eprint ID
3531
DOI https://www.doi.org/10.1029/92jc01856

Cite as
Hellmer, H. H. and Jacobs, S. S. (1992): Ocean interactions with the base of Amery Ice Shelf, Antarctica , Journal of Geophysical Research, 97 (C12), p. 20305 . doi: https://www.doi.org/10.1029/92jc01856


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