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Published August 2016 | Published + Supplemental Material
Journal Article Open

The role of ice stream dynamics in deglaciation

Abstract

Since the mid-Pleistocene transition, deglaciation has occurred only after ice sheets have grown large while experiencing several precession and obliquity cycles, indicating that large ice sheets are more sensitive to Milankovitch forcing than small ice sheets are. Observations and model simulations suggest that the development of ice streams in the Laurentide Ice Sheet played an as yet unknown role in deglaciations. In this study, we propose a mechanism by which ice streams may enhance deglaciation and render large ice sheets more sensitive to Milankovitch forcing. We use an idealized configuration of the Parallel Ice Sheet Model that permits the formation of ice streams. When the ice sheet is large and ice streams are sufficiently developed, an upward shift in equilibrium line altitude, commensurate with Milankovitch forcing, results in rapid deglaciation, while the same shift applied to an ice sheet without fully formed ice streams results in continued ice sheet growth or slower deglaciation. Rapid deglaciation in ice sheets with significant streaming behavior is caused by ice stream acceleration and the attendant enhancement of calving and surface melting at low elevations. Ice stream acceleration is ultimately the result of steepening of the ice surface and increased driving stresses in ice stream onset zones, which come about due to the dependence of surface mass balance on elevation. These ice sheet simulations match the broad features of geomorphological observations and add ice stream dynamics that are missing from previous model studies of deglaciation.

Additional Information

© 2016 American Geophysical Union. Issue online: 13 September 2016; Version of record online: 31 August 2016; Accepted manuscript online: 9 August 2016; Manuscript Accepted: 4 August 2016; Manuscript Revised: 18 July 2016; Manuscript Received: 3 May 2016. This work has been supported by the NSF grant AGS-1303604. E.T. thanks the Weizmann Institute for its hospitality during parts of this work. A.R. has been supported by the NSF Graduate Research Fellowship. We thank Christian Schoof, Jim Rice, Jerry Mitrovica, and Richard Hindmarsh for useful suggestions and helpful conversations during the completion of this work. Special thanks go to the PISM team at the University of Alaska Fairbanks for providing timely model support. Development of PISM is supported by NASA grants NNX13AM16G and NNX13AK27G. All model results used to produce the figures in this study are available from the corresponding author upon request from robel@caltech.edu.

Attached Files

Published - Robel_et_al-2016-Journal_of_Geophysical_Research__Earth_Surface.pdf

Supplemental Material - jgrf20583-sup-0001-supplementary.pdf

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jgrf20583-sup-0001-supplementary.pdf
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Additional details

Created:
August 22, 2023
Modified:
October 23, 2023