Formation of glacier tables caused by differential ice melting: field observation and modelling

International audience Abstract. Glacier tables are structures frequently encountered on temperate glaciers. They consist of a rock supported by a narrow ice foot which forms through differential melting of the ice. In this article, we investigate their formation by following their dynamics on the M...

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Published in:The Cryosphere
Main Authors: Hénot, Marceau, Langlois, Vincent, J., Vessaire, Jérémy, Plihon, Nicolas, Taberlet, Nicolas
Other Authors: Laboratoire de Physique de l'ENS Lyon (Phys-ENS), École normale supérieure de Lyon (ENS de Lyon)-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement (LGL-TPE), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Université Jean Monnet - Saint-Étienne (UJM)-Centre National de la Recherche Scientifique (CNRS)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2022
Subjects:
Online Access:https://hal.science/hal-03708597
https://hal.science/hal-03708597/document
https://hal.science/hal-03708597/file/tc-16-2617-2022.pdf
https://doi.org/10.5194/tc-16-2617-2022
id ftunivstetienne:oai:HAL:hal-03708597v1
record_format openpolar
spelling ftunivstetienne:oai:HAL:hal-03708597v1 2024-05-12T08:11:55+00:00 Formation of glacier tables caused by differential ice melting: field observation and modelling Hénot, Marceau Langlois, Vincent, J. Vessaire, Jérémy Plihon, Nicolas Taberlet, Nicolas Laboratoire de Physique de l'ENS Lyon (Phys-ENS) École normale supérieure de Lyon (ENS de Lyon)-Université de Lyon-Centre National de la Recherche Scientifique (CNRS) Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement (LGL-TPE) École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL) Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Université Jean Monnet - Saint-Étienne (UJM)-Centre National de la Recherche Scientifique (CNRS) 2022 https://hal.science/hal-03708597 https://hal.science/hal-03708597/document https://hal.science/hal-03708597/file/tc-16-2617-2022.pdf https://doi.org/10.5194/tc-16-2617-2022 en eng HAL CCSD Copernicus info:eu-repo/semantics/altIdentifier/doi/10.5194/tc-16-2617-2022 hal-03708597 https://hal.science/hal-03708597 https://hal.science/hal-03708597/document https://hal.science/hal-03708597/file/tc-16-2617-2022.pdf doi:10.5194/tc-16-2617-2022 http://creativecommons.org/licenses/by/ info:eu-repo/semantics/OpenAccess ISSN: 1994-0424 EISSN: 1994-0416 The Cryosphere https://hal.science/hal-03708597 The Cryosphere, 2022, 16 (6), pp.2617-2628. ⟨10.5194/tc-16-2617-2022⟩ [PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph] [SDU.STU.GL]Sciences of the Universe [physics]/Earth Sciences/Glaciology [SDU.STU.GM]Sciences of the Universe [physics]/Earth Sciences/Geomorphology info:eu-repo/semantics/article Journal articles 2022 ftunivstetienne https://doi.org/10.5194/tc-16-2617-2022 2024-04-18T00:14:06Z International audience Abstract. Glacier tables are structures frequently encountered on temperate glaciers. They consist of a rock supported by a narrow ice foot which forms through differential melting of the ice. In this article, we investigate their formation by following their dynamics on the Mer de Glace (the Alps, France). We report field measurements of four specific glacier tables over the course of several days, as well as snapshot measurements of a field of 80 tables performed on a given day. We develop a simple model accounting for the various mechanisms of the heat transfer on the glacier using local meteorological data, which displays a quantitative agreement with the field measurements. We show that the formation of glacier tables is controlled by the global heat flux received by the rocks, which causes the ice underneath to melt at a rate proportional to the one of the surrounding ice. Under large rocks the ice ablation rate is reduced compared to bare ice, leading to the formation of glacier tables. This thermal insulation effect is due to the warmer surface temperature of rocks compared to the ice, which affects the net long-wave and turbulent fluxes. While the short-wave radiation, which is the main source of heat, is slightly more absorbed by the rocks than the ice, it plays an indirect role in the insulation by inducing a thermal gradient across the rocks which warms them. Under a critical size, however, rocks can enhance ice melting and consequently sink into the ice surface. This happens when the insulation effect is too weak to compensate for a geometrical amplification effect: the external heat fluxes are received on a larger surface than the contact area with the ice. We identified the main parameters controlling the ability of a rock to form a glacier table: the rock thickness, its aspect ratio, and the ratio between the averaged turbulent and short-wave heat fluxes. Article in Journal/Newspaper The Cryosphere Université Jean Monnet – Saint-Etienne: HAL The Cryosphere 16 6 2617 2628
institution Open Polar
collection Université Jean Monnet – Saint-Etienne: HAL
op_collection_id ftunivstetienne
language English
topic [PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph]
[SDU.STU.GL]Sciences of the Universe [physics]/Earth Sciences/Glaciology
[SDU.STU.GM]Sciences of the Universe [physics]/Earth Sciences/Geomorphology
spellingShingle [PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph]
[SDU.STU.GL]Sciences of the Universe [physics]/Earth Sciences/Glaciology
[SDU.STU.GM]Sciences of the Universe [physics]/Earth Sciences/Geomorphology
Hénot, Marceau
Langlois, Vincent, J.
Vessaire, Jérémy
Plihon, Nicolas
Taberlet, Nicolas
Formation of glacier tables caused by differential ice melting: field observation and modelling
topic_facet [PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph]
[SDU.STU.GL]Sciences of the Universe [physics]/Earth Sciences/Glaciology
[SDU.STU.GM]Sciences of the Universe [physics]/Earth Sciences/Geomorphology
description International audience Abstract. Glacier tables are structures frequently encountered on temperate glaciers. They consist of a rock supported by a narrow ice foot which forms through differential melting of the ice. In this article, we investigate their formation by following their dynamics on the Mer de Glace (the Alps, France). We report field measurements of four specific glacier tables over the course of several days, as well as snapshot measurements of a field of 80 tables performed on a given day. We develop a simple model accounting for the various mechanisms of the heat transfer on the glacier using local meteorological data, which displays a quantitative agreement with the field measurements. We show that the formation of glacier tables is controlled by the global heat flux received by the rocks, which causes the ice underneath to melt at a rate proportional to the one of the surrounding ice. Under large rocks the ice ablation rate is reduced compared to bare ice, leading to the formation of glacier tables. This thermal insulation effect is due to the warmer surface temperature of rocks compared to the ice, which affects the net long-wave and turbulent fluxes. While the short-wave radiation, which is the main source of heat, is slightly more absorbed by the rocks than the ice, it plays an indirect role in the insulation by inducing a thermal gradient across the rocks which warms them. Under a critical size, however, rocks can enhance ice melting and consequently sink into the ice surface. This happens when the insulation effect is too weak to compensate for a geometrical amplification effect: the external heat fluxes are received on a larger surface than the contact area with the ice. We identified the main parameters controlling the ability of a rock to form a glacier table: the rock thickness, its aspect ratio, and the ratio between the averaged turbulent and short-wave heat fluxes.
author2 Laboratoire de Physique de l'ENS Lyon (Phys-ENS)
École normale supérieure de Lyon (ENS de Lyon)-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)
Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement (LGL-TPE)
École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL)
Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Université Jean Monnet - Saint-Étienne (UJM)-Centre National de la Recherche Scientifique (CNRS)
format Article in Journal/Newspaper
author Hénot, Marceau
Langlois, Vincent, J.
Vessaire, Jérémy
Plihon, Nicolas
Taberlet, Nicolas
author_facet Hénot, Marceau
Langlois, Vincent, J.
Vessaire, Jérémy
Plihon, Nicolas
Taberlet, Nicolas
author_sort Hénot, Marceau
title Formation of glacier tables caused by differential ice melting: field observation and modelling
title_short Formation of glacier tables caused by differential ice melting: field observation and modelling
title_full Formation of glacier tables caused by differential ice melting: field observation and modelling
title_fullStr Formation of glacier tables caused by differential ice melting: field observation and modelling
title_full_unstemmed Formation of glacier tables caused by differential ice melting: field observation and modelling
title_sort formation of glacier tables caused by differential ice melting: field observation and modelling
publisher HAL CCSD
publishDate 2022
url https://hal.science/hal-03708597
https://hal.science/hal-03708597/document
https://hal.science/hal-03708597/file/tc-16-2617-2022.pdf
https://doi.org/10.5194/tc-16-2617-2022
genre The Cryosphere
genre_facet The Cryosphere
op_source ISSN: 1994-0424
EISSN: 1994-0416
The Cryosphere
https://hal.science/hal-03708597
The Cryosphere, 2022, 16 (6), pp.2617-2628. ⟨10.5194/tc-16-2617-2022⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.5194/tc-16-2617-2022
hal-03708597
https://hal.science/hal-03708597
https://hal.science/hal-03708597/document
https://hal.science/hal-03708597/file/tc-16-2617-2022.pdf
doi:10.5194/tc-16-2617-2022
op_rights http://creativecommons.org/licenses/by/
info:eu-repo/semantics/OpenAccess
op_doi https://doi.org/10.5194/tc-16-2617-2022
container_title The Cryosphere
container_volume 16
container_issue 6
container_start_page 2617
op_container_end_page 2628
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