The vertical structure of precipitation at two stations in East Antarctica derived from micro rain radars

<p>Precipitation over Antarctica is the main term in the surface mass balance of the Antarctic ice sheet, which is crucial for the future evolution of the sea level worldwide. Precipitation, however, remains poorly documented and understood mainly because of a lack of observations in this extr...

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Main Authors: C. Durán-Alarcón, B. Boudevillain, C. Genthon, J. Grazioli, N. Souverijns, N. P. M. van Lipzig, I. V. Gorodetskaya, A. Berne
Format: Article
Language:English
Published: Copernicus Publications 2019-01-01
Series:The Cryosphere
Online Access:https://www.the-cryosphere.net/13/247/2019/tc-13-247-2019.pdf
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author C. Durán-Alarcón
B. Boudevillain
C. Genthon
J. Grazioli
J. Grazioli
N. Souverijns
N. P. M. van Lipzig
I. V. Gorodetskaya
A. Berne
author_facet C. Durán-Alarcón
B. Boudevillain
C. Genthon
J. Grazioli
J. Grazioli
N. Souverijns
N. P. M. van Lipzig
I. V. Gorodetskaya
A. Berne
author_sort C. Durán-Alarcón
collection DOAJ
description <p>Precipitation over Antarctica is the main term in the surface mass balance of the Antarctic ice sheet, which is crucial for the future evolution of the sea level worldwide. Precipitation, however, remains poorly documented and understood mainly because of a lack of observations in this extreme environment. Two observatories dedicated to precipitation have been set up at the Belgian station Princess Elisabeth (PE) and at the French station Dumont d'Urville (DDU) in East Antarctica. Among other instruments, both sites have a vertically pointing micro rain radar (MRR) working at the K band. Measurements have been continuously collected at DDU since the austral summer of 2015–2016, while they have been collected mostly during summer seasons at PE since 2010, with a full year of observation during 2012. In this study, the statistics of the vertical profiles of reflectivity, vertical velocity, and spectral width are analyzed for all seasons. Vertical profiles were separated into surface precipitation and virga to evaluate the impact of virga on the structure of the vertical profiles. The climatology of the study area plays an important role in the structure of the precipitation: warmer and moister atmospheric conditions at DDU favor the occurrence of more intense precipitation compared with PE, with a difference of 8&thinsp;dBZ between both stations. The strong katabatic winds blowing at DDU induce a decrease in reflectivity close to the ground due to the sublimation of the snowfall particles. The vertical profiles of precipitation velocity show significant differences between the two stations. In general, at DDU the vertical velocity increases as the height decreases, while at PE the vertical velocity decreases as the height decreases. These features of the vertical profiles of reflectivity and vertical velocity could be explained by the more frequent occurrence of aggregation and riming at DDU compared to PE because of the lower temperature and relative humidity at the latter, located further in the interior. Robust and reliable statistics about the vertical profile of precipitation in Antarctica, as derived from MRRs for instance, are necessary and valuable for the evaluation of precipitation estimates derived from satellite measurements and from numerical atmospheric models.</p>
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spelling doaj.art-3346acf6f1be4063a34e8c6a2fc30df62022-12-21T19:48:27ZengCopernicus PublicationsThe Cryosphere1994-04161994-04242019-01-011324726410.5194/tc-13-247-2019The vertical structure of precipitation at two stations in East Antarctica derived from micro rain radarsC. Durán-Alarcón0B. Boudevillain1C. Genthon2J. Grazioli3J. Grazioli4N. Souverijns5N. P. M. van Lipzig6I. V. Gorodetskaya7A. Berne8CNRS, IRD, Grenoble INP Institute of Engineering, Université Grenoble Alpes, IGE, 38000 Grenoble, FranceCNRS, IRD, Grenoble INP Institute of Engineering, Université Grenoble Alpes, IGE, 38000 Grenoble, FranceCNRS, IRD, Grenoble INP Institute of Engineering, Université Grenoble Alpes, IGE, 38000 Grenoble, FranceEnvironmental Remote Sensing Laboratory, École polytechnique fédérale de Lausanne, 1015 Lausanne, SwitzerlandFederal Office of Meteorology and Climatology, MeteoSwiss, Locarno-Monti, SwitzerlandDepartment of Earth and Environmental Sciences, Katholieke Universiteit Leuven, Leuven, BelgiumDepartment of Earth and Environmental Sciences, Katholieke Universiteit Leuven, Leuven, BelgiumCentre for Environmental and Marine Studies, Department of Physics, University of Aveiro, Aveiro, PortugalEnvironmental Remote Sensing Laboratory, École polytechnique fédérale de Lausanne, 1015 Lausanne, Switzerland<p>Precipitation over Antarctica is the main term in the surface mass balance of the Antarctic ice sheet, which is crucial for the future evolution of the sea level worldwide. Precipitation, however, remains poorly documented and understood mainly because of a lack of observations in this extreme environment. Two observatories dedicated to precipitation have been set up at the Belgian station Princess Elisabeth (PE) and at the French station Dumont d'Urville (DDU) in East Antarctica. Among other instruments, both sites have a vertically pointing micro rain radar (MRR) working at the K band. Measurements have been continuously collected at DDU since the austral summer of 2015–2016, while they have been collected mostly during summer seasons at PE since 2010, with a full year of observation during 2012. In this study, the statistics of the vertical profiles of reflectivity, vertical velocity, and spectral width are analyzed for all seasons. Vertical profiles were separated into surface precipitation and virga to evaluate the impact of virga on the structure of the vertical profiles. The climatology of the study area plays an important role in the structure of the precipitation: warmer and moister atmospheric conditions at DDU favor the occurrence of more intense precipitation compared with PE, with a difference of 8&thinsp;dBZ between both stations. The strong katabatic winds blowing at DDU induce a decrease in reflectivity close to the ground due to the sublimation of the snowfall particles. The vertical profiles of precipitation velocity show significant differences between the two stations. In general, at DDU the vertical velocity increases as the height decreases, while at PE the vertical velocity decreases as the height decreases. These features of the vertical profiles of reflectivity and vertical velocity could be explained by the more frequent occurrence of aggregation and riming at DDU compared to PE because of the lower temperature and relative humidity at the latter, located further in the interior. Robust and reliable statistics about the vertical profile of precipitation in Antarctica, as derived from MRRs for instance, are necessary and valuable for the evaluation of precipitation estimates derived from satellite measurements and from numerical atmospheric models.</p>https://www.the-cryosphere.net/13/247/2019/tc-13-247-2019.pdf
spellingShingle C. Durán-Alarcón
B. Boudevillain
C. Genthon
J. Grazioli
J. Grazioli
N. Souverijns
N. P. M. van Lipzig
I. V. Gorodetskaya
A. Berne
The vertical structure of precipitation at two stations in East Antarctica derived from micro rain radars
The Cryosphere
title The vertical structure of precipitation at two stations in East Antarctica derived from micro rain radars
title_full The vertical structure of precipitation at two stations in East Antarctica derived from micro rain radars
title_fullStr The vertical structure of precipitation at two stations in East Antarctica derived from micro rain radars
title_full_unstemmed The vertical structure of precipitation at two stations in East Antarctica derived from micro rain radars
title_short The vertical structure of precipitation at two stations in East Antarctica derived from micro rain radars
title_sort vertical structure of precipitation at two stations in east antarctica derived from micro rain radars
url https://www.the-cryosphere.net/13/247/2019/tc-13-247-2019.pdf
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