Observations, theory, and modeling of the differential accumulation of Antarctic megadunes

Antarctic megadunes are characterized by significant spatial differences in accumulation rate, with higher accumulation on the windward side and near-zero accumulation on the lee side. This leads to spatial differences in physical properties of snow and surface roughness, as well as to the upwind mi...

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Published in:Journal of Geophysical Research: Earth Surface
Main Authors: Dadic, Ruzica, Mott, Rebecca, Horgan, Huw J., Lehning, Michael
Format: Text
Language:unknown
Published: Washington, Amer Geophysical Union 2014
Subjects:
Online Access:https://doi.org/10.1002/2013Jf002844
http://infoscience.epfl.ch/record/196795
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spelling ftinfoscience:oai:infoscience.tind.io:196795 2023-05-15T13:51:37+02:00 Observations, theory, and modeling of the differential accumulation of Antarctic megadunes Dadic, Ruzica Mott, Rebecca Horgan, Huw J. Lehning, Michael 2014-02-17T18:14:14Z https://doi.org/10.1002/2013Jf002844 http://infoscience.epfl.ch/record/196795 unknown Washington, Amer Geophysical Union doi:10.1002/2013Jf002844 ISI:000329873500021 http://infoscience.epfl.ch/record/196795 http://infoscience.epfl.ch/record/196795 Text 2014 ftinfoscience https://doi.org/10.1002/2013Jf002844 2023-02-13T22:19:15Z Antarctic megadunes are characterized by significant spatial differences in accumulation rate, with higher accumulation on the windward side and near-zero accumulation on the lee side. This leads to spatial differences in physical properties of snow and surface roughness, as well as to the upwind migration of the megadunes. While previous studies agree that megadunes are a result of complex interactions between wind, topography, and snow, it is not clear how they form or why they accumulate on the windward side. Here we use ICESat observations, dimensional analysis, and atmospheric flow modeling to investigate what conditions are responsible for the accumulation patterns and upwind migration of the megadunes. First, we use ICESat data to quantify the pattern of differential surface elevation change across the megadunes. We then use dimensional analysis based on supercritical-flow theory and atmospheric flow modeling to show that the megadunes topography and a stable atmosphere will always lead to upwind dune migration. We show that a combination of persistent katabatic winds, strong stability, and spatial variability in surface roughness is responsible for the accumulation on the upwind slope and hence the upwind migration of the megadunes. We further show that spatial differences in surface roughness are the primary control on accumulation magnitudes and hence dune migration velocity. The dune migration velocity in turn influences the degree of snow-metamorphism and the physical properties of snow that are relevant for paleoclimate records. Our findings pertain to the ongoing evolution of the megadunes, but their genesis remains an open question. Text Antarc* Antarctic EPFL Infoscience (Ecole Polytechnique Fédérale Lausanne) Antarctic Journal of Geophysical Research: Earth Surface 118 4 2343 2353
institution Open Polar
collection EPFL Infoscience (Ecole Polytechnique Fédérale Lausanne)
op_collection_id ftinfoscience
language unknown
description Antarctic megadunes are characterized by significant spatial differences in accumulation rate, with higher accumulation on the windward side and near-zero accumulation on the lee side. This leads to spatial differences in physical properties of snow and surface roughness, as well as to the upwind migration of the megadunes. While previous studies agree that megadunes are a result of complex interactions between wind, topography, and snow, it is not clear how they form or why they accumulate on the windward side. Here we use ICESat observations, dimensional analysis, and atmospheric flow modeling to investigate what conditions are responsible for the accumulation patterns and upwind migration of the megadunes. First, we use ICESat data to quantify the pattern of differential surface elevation change across the megadunes. We then use dimensional analysis based on supercritical-flow theory and atmospheric flow modeling to show that the megadunes topography and a stable atmosphere will always lead to upwind dune migration. We show that a combination of persistent katabatic winds, strong stability, and spatial variability in surface roughness is responsible for the accumulation on the upwind slope and hence the upwind migration of the megadunes. We further show that spatial differences in surface roughness are the primary control on accumulation magnitudes and hence dune migration velocity. The dune migration velocity in turn influences the degree of snow-metamorphism and the physical properties of snow that are relevant for paleoclimate records. Our findings pertain to the ongoing evolution of the megadunes, but their genesis remains an open question.
format Text
author Dadic, Ruzica
Mott, Rebecca
Horgan, Huw J.
Lehning, Michael
spellingShingle Dadic, Ruzica
Mott, Rebecca
Horgan, Huw J.
Lehning, Michael
Observations, theory, and modeling of the differential accumulation of Antarctic megadunes
author_facet Dadic, Ruzica
Mott, Rebecca
Horgan, Huw J.
Lehning, Michael
author_sort Dadic, Ruzica
title Observations, theory, and modeling of the differential accumulation of Antarctic megadunes
title_short Observations, theory, and modeling of the differential accumulation of Antarctic megadunes
title_full Observations, theory, and modeling of the differential accumulation of Antarctic megadunes
title_fullStr Observations, theory, and modeling of the differential accumulation of Antarctic megadunes
title_full_unstemmed Observations, theory, and modeling of the differential accumulation of Antarctic megadunes
title_sort observations, theory, and modeling of the differential accumulation of antarctic megadunes
publisher Washington, Amer Geophysical Union
publishDate 2014
url https://doi.org/10.1002/2013Jf002844
http://infoscience.epfl.ch/record/196795
geographic Antarctic
geographic_facet Antarctic
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_source http://infoscience.epfl.ch/record/196795
op_relation doi:10.1002/2013Jf002844
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http://infoscience.epfl.ch/record/196795
op_doi https://doi.org/10.1002/2013Jf002844
container_title Journal of Geophysical Research: Earth Surface
container_volume 118
container_issue 4
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