Calving of Ross Ice Shelf from wave erosion and hydrostatic stresses

Ice shelf calving constitutes roughly half of the total mass loss from the Antarctic ice sheet. Although much attention is paid to calving of giant tabular icebergs, these events are relatively rare. More frequent, smaller-scale calving events likely play an important role in the ice shelf frontal d...

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Main Authors: Sartore, Nicolas B., Wagner, Till J. W., Siegfried, Matthew R., Pujara, Nimish, Zoet, Lucas K.
Format: Text
Language:English
Published: 2024
Subjects:
Online Access:https://doi.org/10.5194/egusphere-2024-571
https://egusphere.copernicus.org/preprints/2024/egusphere-2024-571/
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spelling ftcopernicus:oai:publications.copernicus.org:egusphere118409 2024-09-09T19:02:29+00:00 Calving of Ross Ice Shelf from wave erosion and hydrostatic stresses Sartore, Nicolas B. Wagner, Till J. W. Siegfried, Matthew R. Pujara, Nimish Zoet, Lucas K. 2024-03-26 application/pdf https://doi.org/10.5194/egusphere-2024-571 https://egusphere.copernicus.org/preprints/2024/egusphere-2024-571/ eng eng doi:10.5194/egusphere-2024-571 https://egusphere.copernicus.org/preprints/2024/egusphere-2024-571/ eISSN: Text 2024 ftcopernicus https://doi.org/10.5194/egusphere-2024-571 2024-08-28T05:24:15Z Ice shelf calving constitutes roughly half of the total mass loss from the Antarctic ice sheet. Although much attention is paid to calving of giant tabular icebergs, these events are relatively rare. More frequent, smaller-scale calving events likely play an important role in the ice shelf frontal dynamics. Here, we investigate the role of bending stresses at the ice shelf front in driving calving on the scale 100 m – 1 km, perpendicular to the ice edge. We focus in particular on how buoyant underwater "feet" that protrude beyond the above-water ice cliff may cause tensile stresses at the base of the ice and ultimately lead to fracture. Indirect and anecdotal observations of such feet at the Ross Ice Shelf front suggest that this process may be widespread. We consider satellite observations, together with an elastic beam model and a parameterization of frontal wave erosion to estimate the size and frequency of such calving events. Our results suggest that foot-induced mass loss at Ross Ice Shelf may cause up to 25 % of the total frontal ablation. However, stresses induced through this process are likely not sufficient to initiate crevassing but rather act to propagate existing crevasses. In addition, the relatively strong ice thickness dependence of the frontal uplift suggests an important role for internal bending moments due to temperature gradients in the ice. The highly variable environment, irregularity of pre-existing crevasse spacing, and complex rheology of the ice continue to pose challenges in better constraining the drivers behind the observed deformations and resulting calving rates. Text Antarc* Antarctic Ice Sheet Ice Shelf Iceberg* Ross Ice Shelf Copernicus Publications: E-Journals Antarctic Ross Ice Shelf The Antarctic
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description Ice shelf calving constitutes roughly half of the total mass loss from the Antarctic ice sheet. Although much attention is paid to calving of giant tabular icebergs, these events are relatively rare. More frequent, smaller-scale calving events likely play an important role in the ice shelf frontal dynamics. Here, we investigate the role of bending stresses at the ice shelf front in driving calving on the scale 100 m – 1 km, perpendicular to the ice edge. We focus in particular on how buoyant underwater "feet" that protrude beyond the above-water ice cliff may cause tensile stresses at the base of the ice and ultimately lead to fracture. Indirect and anecdotal observations of such feet at the Ross Ice Shelf front suggest that this process may be widespread. We consider satellite observations, together with an elastic beam model and a parameterization of frontal wave erosion to estimate the size and frequency of such calving events. Our results suggest that foot-induced mass loss at Ross Ice Shelf may cause up to 25 % of the total frontal ablation. However, stresses induced through this process are likely not sufficient to initiate crevassing but rather act to propagate existing crevasses. In addition, the relatively strong ice thickness dependence of the frontal uplift suggests an important role for internal bending moments due to temperature gradients in the ice. The highly variable environment, irregularity of pre-existing crevasse spacing, and complex rheology of the ice continue to pose challenges in better constraining the drivers behind the observed deformations and resulting calving rates.
format Text
author Sartore, Nicolas B.
Wagner, Till J. W.
Siegfried, Matthew R.
Pujara, Nimish
Zoet, Lucas K.
spellingShingle Sartore, Nicolas B.
Wagner, Till J. W.
Siegfried, Matthew R.
Pujara, Nimish
Zoet, Lucas K.
Calving of Ross Ice Shelf from wave erosion and hydrostatic stresses
author_facet Sartore, Nicolas B.
Wagner, Till J. W.
Siegfried, Matthew R.
Pujara, Nimish
Zoet, Lucas K.
author_sort Sartore, Nicolas B.
title Calving of Ross Ice Shelf from wave erosion and hydrostatic stresses
title_short Calving of Ross Ice Shelf from wave erosion and hydrostatic stresses
title_full Calving of Ross Ice Shelf from wave erosion and hydrostatic stresses
title_fullStr Calving of Ross Ice Shelf from wave erosion and hydrostatic stresses
title_full_unstemmed Calving of Ross Ice Shelf from wave erosion and hydrostatic stresses
title_sort calving of ross ice shelf from wave erosion and hydrostatic stresses
publishDate 2024
url https://doi.org/10.5194/egusphere-2024-571
https://egusphere.copernicus.org/preprints/2024/egusphere-2024-571/
geographic Antarctic
Ross Ice Shelf
The Antarctic
geographic_facet Antarctic
Ross Ice Shelf
The Antarctic
genre Antarc*
Antarctic
Ice Sheet
Ice Shelf
Iceberg*
Ross Ice Shelf
genre_facet Antarc*
Antarctic
Ice Sheet
Ice Shelf
Iceberg*
Ross Ice Shelf
op_source eISSN:
op_relation doi:10.5194/egusphere-2024-571
https://egusphere.copernicus.org/preprints/2024/egusphere-2024-571/
op_doi https://doi.org/10.5194/egusphere-2024-571
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