Antarctic Snowmelt Detected by Diurnal Variations of AMSR-E Brightness Temperature

Antarctic surface snowmelt is sensitive to the polar climate. The ascending and descending passes of the Advanced Microwave Scanning Radiometer for Earth Observing System Sensor (AMSR-E) observed the Antarctic ice sheet in the afternoon (the warmest period) and at midnight (a cold period), enabling...

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Published in:Remote Sensing
Main Authors: Lei Zheng, Chunxia Zhou, Ruixi Liu, Qizhen Sun
Format: Text
Language:English
Published: Multidisciplinary Digital Publishing Institute 2018
Subjects:
Online Access:https://doi.org/10.3390/rs10091391
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spelling ftmdpi:oai:mdpi.com:/2072-4292/10/9/1391/ 2023-08-20T04:02:14+02:00 Antarctic Snowmelt Detected by Diurnal Variations of AMSR-E Brightness Temperature Lei Zheng Chunxia Zhou Ruixi Liu Qizhen Sun agris 2018-08-31 application/pdf https://doi.org/10.3390/rs10091391 EN eng Multidisciplinary Digital Publishing Institute Remote Sensing in Geology, Geomorphology and Hydrology https://dx.doi.org/10.3390/rs10091391 https://creativecommons.org/licenses/by/4.0/ Remote Sensing; Volume 10; Issue 9; Pages: 1391 Antarctica snowmelt AMSR-E MEMLS Text 2018 ftmdpi https://doi.org/10.3390/rs10091391 2023-07-31T21:42:19Z Antarctic surface snowmelt is sensitive to the polar climate. The ascending and descending passes of the Advanced Microwave Scanning Radiometer for Earth Observing System Sensor (AMSR-E) observed the Antarctic ice sheet in the afternoon (the warmest period) and at midnight (a cold period), enabling us to make full use of the diurnal amplitude variations (DAV) in brightness temperature (Tb) to detect snowmelt. The DAV in vertically polarized 36.5 GHz Tb (DAV36V) is extremely sensitive to liquid water and can reduce the effects of the structural changes in snowpacks during melt seasons. A set of controlled experiments based on the microwave emission model of layered snow (MEMLS) were conducted to study the changes of the vertically polarized 36.5 GHz Tb (Δ36V) during the transitions from dry to wet snow regimes. Results of the experiments suggest that 9 K can be used as a DAV36V threshold to recognize snowmelt. The analyses of snowmelt suggest that the Antarctic ice sheet began to melt in November and became almost completely frozen in late March of the following year. The total cumulative melt area from 2002 to 2011 was 2.44 × 106 km2, i.e., 17.58% of the Antarctic ice sheet. The annual cumulative melt area showed considerable fluctuations, with a significant (above 90% confidence level) drop of 5.24 × 104 km2/year in the short term. Persistent snowmelt (i.e., melt that continues for at least three days) detected by AMSR-E and hourly air temperatures (Tair) were very consistent. Though melt seasons became longer in the western Antarctic Peninsula and the Shackleton Ice Shelf, Antarctica was subjected to considerable decreases in duration and melting days in stable melt areas, i.e., −0.64 and −0.81 days/year, respectively. Surface snowmelt in Antarctica decreased temporally and spatially from 2002 to 2011. Text Antarc* Antarctic Antarctic Peninsula Antarctica Ice Sheet Ice Shelf Shackleton Ice Shelf MDPI Open Access Publishing Antarctic The Antarctic Antarctic Peninsula Shackleton Shackleton Ice Shelf ENVELOPE(100.504,100.504,-65.996,-65.996) Remote Sensing 10 9 1391
institution Open Polar
collection MDPI Open Access Publishing
op_collection_id ftmdpi
language English
topic Antarctica
snowmelt
AMSR-E
MEMLS
spellingShingle Antarctica
snowmelt
AMSR-E
MEMLS
Lei Zheng
Chunxia Zhou
Ruixi Liu
Qizhen Sun
Antarctic Snowmelt Detected by Diurnal Variations of AMSR-E Brightness Temperature
topic_facet Antarctica
snowmelt
AMSR-E
MEMLS
description Antarctic surface snowmelt is sensitive to the polar climate. The ascending and descending passes of the Advanced Microwave Scanning Radiometer for Earth Observing System Sensor (AMSR-E) observed the Antarctic ice sheet in the afternoon (the warmest period) and at midnight (a cold period), enabling us to make full use of the diurnal amplitude variations (DAV) in brightness temperature (Tb) to detect snowmelt. The DAV in vertically polarized 36.5 GHz Tb (DAV36V) is extremely sensitive to liquid water and can reduce the effects of the structural changes in snowpacks during melt seasons. A set of controlled experiments based on the microwave emission model of layered snow (MEMLS) were conducted to study the changes of the vertically polarized 36.5 GHz Tb (Δ36V) during the transitions from dry to wet snow regimes. Results of the experiments suggest that 9 K can be used as a DAV36V threshold to recognize snowmelt. The analyses of snowmelt suggest that the Antarctic ice sheet began to melt in November and became almost completely frozen in late March of the following year. The total cumulative melt area from 2002 to 2011 was 2.44 × 106 km2, i.e., 17.58% of the Antarctic ice sheet. The annual cumulative melt area showed considerable fluctuations, with a significant (above 90% confidence level) drop of 5.24 × 104 km2/year in the short term. Persistent snowmelt (i.e., melt that continues for at least three days) detected by AMSR-E and hourly air temperatures (Tair) were very consistent. Though melt seasons became longer in the western Antarctic Peninsula and the Shackleton Ice Shelf, Antarctica was subjected to considerable decreases in duration and melting days in stable melt areas, i.e., −0.64 and −0.81 days/year, respectively. Surface snowmelt in Antarctica decreased temporally and spatially from 2002 to 2011.
format Text
author Lei Zheng
Chunxia Zhou
Ruixi Liu
Qizhen Sun
author_facet Lei Zheng
Chunxia Zhou
Ruixi Liu
Qizhen Sun
author_sort Lei Zheng
title Antarctic Snowmelt Detected by Diurnal Variations of AMSR-E Brightness Temperature
title_short Antarctic Snowmelt Detected by Diurnal Variations of AMSR-E Brightness Temperature
title_full Antarctic Snowmelt Detected by Diurnal Variations of AMSR-E Brightness Temperature
title_fullStr Antarctic Snowmelt Detected by Diurnal Variations of AMSR-E Brightness Temperature
title_full_unstemmed Antarctic Snowmelt Detected by Diurnal Variations of AMSR-E Brightness Temperature
title_sort antarctic snowmelt detected by diurnal variations of amsr-e brightness temperature
publisher Multidisciplinary Digital Publishing Institute
publishDate 2018
url https://doi.org/10.3390/rs10091391
op_coverage agris
long_lat ENVELOPE(100.504,100.504,-65.996,-65.996)
geographic Antarctic
The Antarctic
Antarctic Peninsula
Shackleton
Shackleton Ice Shelf
geographic_facet Antarctic
The Antarctic
Antarctic Peninsula
Shackleton
Shackleton Ice Shelf
genre Antarc*
Antarctic
Antarctic Peninsula
Antarctica
Ice Sheet
Ice Shelf
Shackleton Ice Shelf
genre_facet Antarc*
Antarctic
Antarctic Peninsula
Antarctica
Ice Sheet
Ice Shelf
Shackleton Ice Shelf
op_source Remote Sensing; Volume 10; Issue 9; Pages: 1391
op_relation Remote Sensing in Geology, Geomorphology and Hydrology
https://dx.doi.org/10.3390/rs10091391
op_rights https://creativecommons.org/licenses/by/4.0/
op_doi https://doi.org/10.3390/rs10091391
container_title Remote Sensing
container_volume 10
container_issue 9
container_start_page 1391
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