Origin and dynamic significance of longitudinal structures ("flow stripes") in the Antarctic Ice Sheet

Longitudinal ice-surface structures in the Antarctic Ice Sheet can be traced continuously down-ice for distances of up to 1200 km. A map of the distribution of ~ 3600 of these features, compiled from satellite images, shows that they mirror the location of fast-flowing glaciers and ice streams that...

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Published in:Earth Surface Dynamics
Main Authors: Glasser, N. F., Jennings, S. J. A., Hambrey, M. J., Hubbard, B.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/esurf-3-239-2015
https://esurf.copernicus.org/articles/3/239/2015/
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spelling ftcopernicus:oai:publications.copernicus.org:esurf26238 2023-05-15T13:54:27+02:00 Origin and dynamic significance of longitudinal structures ("flow stripes") in the Antarctic Ice Sheet Glasser, N. F. Jennings, S. J. A. Hambrey, M. J. Hubbard, B. 2018-09-27 application/pdf https://doi.org/10.5194/esurf-3-239-2015 https://esurf.copernicus.org/articles/3/239/2015/ eng eng doi:10.5194/esurf-3-239-2015 https://esurf.copernicus.org/articles/3/239/2015/ eISSN: 2196-632X Text 2018 ftcopernicus https://doi.org/10.5194/esurf-3-239-2015 2020-07-20T16:24:41Z Longitudinal ice-surface structures in the Antarctic Ice Sheet can be traced continuously down-ice for distances of up to 1200 km. A map of the distribution of ~ 3600 of these features, compiled from satellite images, shows that they mirror the location of fast-flowing glaciers and ice streams that are dominated by basal sliding rates above tens of metres per annum and are strongly guided by subglacial topography. Longitudinal ice-surface structures dominate regions of converging flow, where ice flow is subject to non-coaxial strain and simple shear. They can be traced continuously through crevasse fields and through blue-ice areas, indicating that they represent the surface manifestation of a three-dimensional structure, interpreted as foliation. Flow lines are linear and undeformed for all major flow units described here in the Antarctic Ice Sheet except for the Kamb Ice Stream and the Institute and Möller Ice Stream areas, where areas of flow perturbation are evident. Parcels of ice along individual flow paths on the Lambert Glacier, Recovery Glacier, Byrd Glacier and Pine Island Glacier may reside in the glacier system for ~ 2500 to 18 500 years. Although it is unclear how long it takes for these features to form and decay, we infer that the major ice-flow configuration of the ice sheet may have remained largely unchanged for the last few hundred years, and possibly even longer. This conclusion has implications for our understanding of the long-term landscape evolution of Antarctica, including large-scale patterns of glacial erosion and deposition. Text Antarc* Antarctic Antarctica Byrd Glacier Ice Sheet Kamb Ice Stream Lambert Glacier Möller Ice Stream Pine Island Pine Island Glacier Recovery Glacier Copernicus Publications: E-Journals Antarctic Byrd Byrd Glacier ENVELOPE(160.333,160.333,-80.250,-80.250) Kamb Ice Stream ENVELOPE(-145.000,-145.000,-82.250,-82.250) Lambert Glacier ENVELOPE(67.490,67.490,-73.065,-73.065) Möller Ice Stream ENVELOPE(-63.000,-63.000,-82.000,-82.000) Pine Island Glacier ENVELOPE(-101.000,-101.000,-75.000,-75.000) Recovery Glacier ENVELOPE(-25.500,-25.500,-81.166,-81.166) The Antarctic Earth Surface Dynamics 3 2 239 249
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description Longitudinal ice-surface structures in the Antarctic Ice Sheet can be traced continuously down-ice for distances of up to 1200 km. A map of the distribution of ~ 3600 of these features, compiled from satellite images, shows that they mirror the location of fast-flowing glaciers and ice streams that are dominated by basal sliding rates above tens of metres per annum and are strongly guided by subglacial topography. Longitudinal ice-surface structures dominate regions of converging flow, where ice flow is subject to non-coaxial strain and simple shear. They can be traced continuously through crevasse fields and through blue-ice areas, indicating that they represent the surface manifestation of a three-dimensional structure, interpreted as foliation. Flow lines are linear and undeformed for all major flow units described here in the Antarctic Ice Sheet except for the Kamb Ice Stream and the Institute and Möller Ice Stream areas, where areas of flow perturbation are evident. Parcels of ice along individual flow paths on the Lambert Glacier, Recovery Glacier, Byrd Glacier and Pine Island Glacier may reside in the glacier system for ~ 2500 to 18 500 years. Although it is unclear how long it takes for these features to form and decay, we infer that the major ice-flow configuration of the ice sheet may have remained largely unchanged for the last few hundred years, and possibly even longer. This conclusion has implications for our understanding of the long-term landscape evolution of Antarctica, including large-scale patterns of glacial erosion and deposition.
format Text
author Glasser, N. F.
Jennings, S. J. A.
Hambrey, M. J.
Hubbard, B.
spellingShingle Glasser, N. F.
Jennings, S. J. A.
Hambrey, M. J.
Hubbard, B.
Origin and dynamic significance of longitudinal structures ("flow stripes") in the Antarctic Ice Sheet
author_facet Glasser, N. F.
Jennings, S. J. A.
Hambrey, M. J.
Hubbard, B.
author_sort Glasser, N. F.
title Origin and dynamic significance of longitudinal structures ("flow stripes") in the Antarctic Ice Sheet
title_short Origin and dynamic significance of longitudinal structures ("flow stripes") in the Antarctic Ice Sheet
title_full Origin and dynamic significance of longitudinal structures ("flow stripes") in the Antarctic Ice Sheet
title_fullStr Origin and dynamic significance of longitudinal structures ("flow stripes") in the Antarctic Ice Sheet
title_full_unstemmed Origin and dynamic significance of longitudinal structures ("flow stripes") in the Antarctic Ice Sheet
title_sort origin and dynamic significance of longitudinal structures ("flow stripes") in the antarctic ice sheet
publishDate 2018
url https://doi.org/10.5194/esurf-3-239-2015
https://esurf.copernicus.org/articles/3/239/2015/
long_lat ENVELOPE(160.333,160.333,-80.250,-80.250)
ENVELOPE(-145.000,-145.000,-82.250,-82.250)
ENVELOPE(67.490,67.490,-73.065,-73.065)
ENVELOPE(-63.000,-63.000,-82.000,-82.000)
ENVELOPE(-101.000,-101.000,-75.000,-75.000)
ENVELOPE(-25.500,-25.500,-81.166,-81.166)
geographic Antarctic
Byrd
Byrd Glacier
Kamb Ice Stream
Lambert Glacier
Möller Ice Stream
Pine Island Glacier
Recovery Glacier
The Antarctic
geographic_facet Antarctic
Byrd
Byrd Glacier
Kamb Ice Stream
Lambert Glacier
Möller Ice Stream
Pine Island Glacier
Recovery Glacier
The Antarctic
genre Antarc*
Antarctic
Antarctica
Byrd Glacier
Ice Sheet
Kamb Ice Stream
Lambert Glacier
Möller Ice Stream
Pine Island
Pine Island Glacier
Recovery Glacier
genre_facet Antarc*
Antarctic
Antarctica
Byrd Glacier
Ice Sheet
Kamb Ice Stream
Lambert Glacier
Möller Ice Stream
Pine Island
Pine Island Glacier
Recovery Glacier
op_source eISSN: 2196-632X
op_relation doi:10.5194/esurf-3-239-2015
https://esurf.copernicus.org/articles/3/239/2015/
op_doi https://doi.org/10.5194/esurf-3-239-2015
container_title Earth Surface Dynamics
container_volume 3
container_issue 2
container_start_page 239
op_container_end_page 249
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