Heat flow in Antarctica: How can it influence ice dynamics?
High-quality maps of Geothermal heat flow (GHF) are crucial when modeling ice dynamics, shape, and mass loss of the Antarctic Ice Sheet, which is one of the largest potential contributors to sea level rise. The determination of GHF remains challenging, as in situ data are sparse and geophysical mode...
Published in: | Geochemistry, Geophysics, Geosystems |
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Language: | English |
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ftgfzpotsdam:oai:gfzpublic.gfz-potsdam.de:item_5011234 2023-05-15T14:02:24+02:00 Heat flow in Antarctica: How can it influence ice dynamics? Haeger, C. Petrunin, A. Kaban, M. 2022 application/pdf https://gfzpublic.gfz-potsdam.de/pubman/item/item_5011234 https://gfzpublic.gfz-potsdam.de/pubman/item/item_5011234_1/component/file_5013655/5011234.pdf eng eng info:eu-repo/semantics/altIdentifier/doi/10.1029/2022GC010501 https://gfzpublic.gfz-potsdam.de/pubman/item/item_5011234 https://gfzpublic.gfz-potsdam.de/pubman/item/item_5011234_1/component/file_5013655/5011234.pdf info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/4.0/ CC-BY Geochemistry Geophysics Geosystems (G3) info:eu-repo/semantics/article 2022 ftgfzpotsdam https://doi.org/10.1029/2022GC010501 2022-11-07T00:31:34Z High-quality maps of Geothermal heat flow (GHF) are crucial when modeling ice dynamics, shape, and mass loss of the Antarctic Ice Sheet, which is one of the largest potential contributors to sea level rise. The determination of GHF remains challenging, as in situ data are sparse and geophysical models exhibit large discrepancies in amplitude and resolution, especially on regional scales. Using a novel approach implementing a joint inversion of gravity and seismic tomography data with various geophysical and mineral physics information, we estimate the 3D thermal lithospheric structure and present a new GHF map. The resulting surface heat flow correlates with the location of subglacial volcanism and can represent a boundary condition for accurate ice dynamics models that can explain observed acceleration in the ongoing ice mass loss. Absolute values are within the range of other seismology-based methods and are much lower than those obtained using for example, magnetic data. High uncertainties remain in the parametrization of the upper crustal structure and thermal parameters. Article in Journal/Newspaper Antarc* Antarctic Antarctica Ice Sheet GFZpublic (German Research Centre for Geosciences, Helmholtz-Zentrum Potsdam) Antarctic The Antarctic Geochemistry, Geophysics, Geosystems 23 10 |
institution |
Open Polar |
collection |
GFZpublic (German Research Centre for Geosciences, Helmholtz-Zentrum Potsdam) |
op_collection_id |
ftgfzpotsdam |
language |
English |
description |
High-quality maps of Geothermal heat flow (GHF) are crucial when modeling ice dynamics, shape, and mass loss of the Antarctic Ice Sheet, which is one of the largest potential contributors to sea level rise. The determination of GHF remains challenging, as in situ data are sparse and geophysical models exhibit large discrepancies in amplitude and resolution, especially on regional scales. Using a novel approach implementing a joint inversion of gravity and seismic tomography data with various geophysical and mineral physics information, we estimate the 3D thermal lithospheric structure and present a new GHF map. The resulting surface heat flow correlates with the location of subglacial volcanism and can represent a boundary condition for accurate ice dynamics models that can explain observed acceleration in the ongoing ice mass loss. Absolute values are within the range of other seismology-based methods and are much lower than those obtained using for example, magnetic data. High uncertainties remain in the parametrization of the upper crustal structure and thermal parameters. |
format |
Article in Journal/Newspaper |
author |
Haeger, C. Petrunin, A. Kaban, M. |
spellingShingle |
Haeger, C. Petrunin, A. Kaban, M. Heat flow in Antarctica: How can it influence ice dynamics? |
author_facet |
Haeger, C. Petrunin, A. Kaban, M. |
author_sort |
Haeger, C. |
title |
Heat flow in Antarctica: How can it influence ice dynamics? |
title_short |
Heat flow in Antarctica: How can it influence ice dynamics? |
title_full |
Heat flow in Antarctica: How can it influence ice dynamics? |
title_fullStr |
Heat flow in Antarctica: How can it influence ice dynamics? |
title_full_unstemmed |
Heat flow in Antarctica: How can it influence ice dynamics? |
title_sort |
heat flow in antarctica: how can it influence ice dynamics? |
publishDate |
2022 |
url |
https://gfzpublic.gfz-potsdam.de/pubman/item/item_5011234 https://gfzpublic.gfz-potsdam.de/pubman/item/item_5011234_1/component/file_5013655/5011234.pdf |
geographic |
Antarctic The Antarctic |
geographic_facet |
Antarctic The Antarctic |
genre |
Antarc* Antarctic Antarctica Ice Sheet |
genre_facet |
Antarc* Antarctic Antarctica Ice Sheet |
op_source |
Geochemistry Geophysics Geosystems (G3) |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.1029/2022GC010501 https://gfzpublic.gfz-potsdam.de/pubman/item/item_5011234 https://gfzpublic.gfz-potsdam.de/pubman/item/item_5011234_1/component/file_5013655/5011234.pdf |
op_rights |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/4.0/ |
op_rightsnorm |
CC-BY |
op_doi |
https://doi.org/10.1029/2022GC010501 |
container_title |
Geochemistry, Geophysics, Geosystems |
container_volume |
23 |
container_issue |
10 |
_version_ |
1766272664086773760 |