Antarctic ice shelf thickness change from multimission lidar mapping

We calculate rates of ice thickness change and bottom melt for ice shelves in West Antarctica and the Antarctic Peninsula from a combination of elevation measurements from NASA–CECS Antarctic ice mapping campaigns and NASA Operation IceBridge corrected for oceanic processes from measurements and mod...

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Published in:The Cryosphere
Main Authors: Sutterley, Tyler C., Markus, Thorsten, Neumann, Thomas A., Broeke, Michiel, Wessem, J. Melchior, Ligtenberg, Stefan R. M.
Format: Text
Language:English
Published: 2019
Subjects:
Online Access:https://doi.org/10.5194/tc-13-1801-2019
https://tc.copernicus.org/articles/13/1801/2019/
id ftcopernicus:oai:publications.copernicus.org:tc71184
record_format openpolar
spelling ftcopernicus:oai:publications.copernicus.org:tc71184 2023-05-15T13:55:28+02:00 Antarctic ice shelf thickness change from multimission lidar mapping Sutterley, Tyler C. Markus, Thorsten Neumann, Thomas A. Broeke, Michiel Wessem, J. Melchior Ligtenberg, Stefan R. M. 2019-07-08 application/pdf https://doi.org/10.5194/tc-13-1801-2019 https://tc.copernicus.org/articles/13/1801/2019/ eng eng doi:10.5194/tc-13-1801-2019 https://tc.copernicus.org/articles/13/1801/2019/ eISSN: 1994-0424 Text 2019 ftcopernicus https://doi.org/10.5194/tc-13-1801-2019 2020-07-20T16:22:46Z We calculate rates of ice thickness change and bottom melt for ice shelves in West Antarctica and the Antarctic Peninsula from a combination of elevation measurements from NASA–CECS Antarctic ice mapping campaigns and NASA Operation IceBridge corrected for oceanic processes from measurements and models, surface velocity measurements from synthetic aperture radar, and high-resolution outputs from regional climate models. The ice thickness change rates are calculated in a Lagrangian reference frame to reduce the effects from advection of sharp vertical features, such as cracks and crevasses, that can saturate Eulerian-derived estimates. We use our method over different ice shelves in Antarctica, which vary in terms of size, repeat coverage from airborne altimetry, and dominant processes governing their recent changes. We find that the Larsen-C Ice Shelf is close to steady state over our observation period with spatial variations in ice thickness largely due to the flux divergence of the shelf. Firn and surface processes are responsible for some short-term variability in ice thickness of the Larsen-C Ice Shelf over the time period. The Wilkins Ice Shelf is sensitive to short-timescale coastal and upper-ocean processes, and basal melt is the dominant contributor to the ice thickness change over the period. At the Pine Island Ice Shelf in the critical region near the grounding zone, we find that ice shelf thickness change rates exceed 40 m yr −1 , with the change dominated by strong submarine melting. Regions near the grounding zones of the Dotson and Crosson ice shelves are decreasing in thickness at rates greater than 40 m yr −1 , also due to intense basal melt. NASA–CECS Antarctic ice mapping and NASA Operation IceBridge campaigns provide validation datasets for floating ice shelves at moderately high resolution when coregistered using Lagrangian methods. Text Antarc* Antarctic Antarctic Peninsula Antarctica Ice Shelf Ice Shelves Pine Island West Antarctica Wilkins Ice Shelf Copernicus Publications: E-Journals Antarctic Antarctic Peninsula The Antarctic West Antarctica Wilkins ENVELOPE(59.326,59.326,-67.248,-67.248) Wilkins Ice Shelf ENVELOPE(-72.500,-72.500,-70.416,-70.416) The Cryosphere 13 7 1801 1817
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description We calculate rates of ice thickness change and bottom melt for ice shelves in West Antarctica and the Antarctic Peninsula from a combination of elevation measurements from NASA–CECS Antarctic ice mapping campaigns and NASA Operation IceBridge corrected for oceanic processes from measurements and models, surface velocity measurements from synthetic aperture radar, and high-resolution outputs from regional climate models. The ice thickness change rates are calculated in a Lagrangian reference frame to reduce the effects from advection of sharp vertical features, such as cracks and crevasses, that can saturate Eulerian-derived estimates. We use our method over different ice shelves in Antarctica, which vary in terms of size, repeat coverage from airborne altimetry, and dominant processes governing their recent changes. We find that the Larsen-C Ice Shelf is close to steady state over our observation period with spatial variations in ice thickness largely due to the flux divergence of the shelf. Firn and surface processes are responsible for some short-term variability in ice thickness of the Larsen-C Ice Shelf over the time period. The Wilkins Ice Shelf is sensitive to short-timescale coastal and upper-ocean processes, and basal melt is the dominant contributor to the ice thickness change over the period. At the Pine Island Ice Shelf in the critical region near the grounding zone, we find that ice shelf thickness change rates exceed 40 m yr −1 , with the change dominated by strong submarine melting. Regions near the grounding zones of the Dotson and Crosson ice shelves are decreasing in thickness at rates greater than 40 m yr −1 , also due to intense basal melt. NASA–CECS Antarctic ice mapping and NASA Operation IceBridge campaigns provide validation datasets for floating ice shelves at moderately high resolution when coregistered using Lagrangian methods.
format Text
author Sutterley, Tyler C.
Markus, Thorsten
Neumann, Thomas A.
Broeke, Michiel
Wessem, J. Melchior
Ligtenberg, Stefan R. M.
spellingShingle Sutterley, Tyler C.
Markus, Thorsten
Neumann, Thomas A.
Broeke, Michiel
Wessem, J. Melchior
Ligtenberg, Stefan R. M.
Antarctic ice shelf thickness change from multimission lidar mapping
author_facet Sutterley, Tyler C.
Markus, Thorsten
Neumann, Thomas A.
Broeke, Michiel
Wessem, J. Melchior
Ligtenberg, Stefan R. M.
author_sort Sutterley, Tyler C.
title Antarctic ice shelf thickness change from multimission lidar mapping
title_short Antarctic ice shelf thickness change from multimission lidar mapping
title_full Antarctic ice shelf thickness change from multimission lidar mapping
title_fullStr Antarctic ice shelf thickness change from multimission lidar mapping
title_full_unstemmed Antarctic ice shelf thickness change from multimission lidar mapping
title_sort antarctic ice shelf thickness change from multimission lidar mapping
publishDate 2019
url https://doi.org/10.5194/tc-13-1801-2019
https://tc.copernicus.org/articles/13/1801/2019/
long_lat ENVELOPE(59.326,59.326,-67.248,-67.248)
ENVELOPE(-72.500,-72.500,-70.416,-70.416)
geographic Antarctic
Antarctic Peninsula
The Antarctic
West Antarctica
Wilkins
Wilkins Ice Shelf
geographic_facet Antarctic
Antarctic Peninsula
The Antarctic
West Antarctica
Wilkins
Wilkins Ice Shelf
genre Antarc*
Antarctic
Antarctic Peninsula
Antarctica
Ice Shelf
Ice Shelves
Pine Island
West Antarctica
Wilkins Ice Shelf
genre_facet Antarc*
Antarctic
Antarctic Peninsula
Antarctica
Ice Shelf
Ice Shelves
Pine Island
West Antarctica
Wilkins Ice Shelf
op_source eISSN: 1994-0424
op_relation doi:10.5194/tc-13-1801-2019
https://tc.copernicus.org/articles/13/1801/2019/
op_doi https://doi.org/10.5194/tc-13-1801-2019
container_title The Cryosphere
container_volume 13
container_issue 7
container_start_page 1801
op_container_end_page 1817
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