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: Article in Journal/Newspaper
Language:English
Published: MDPI AG 2018
Subjects:
Q
Online Access:https://doi.org/10.3390/rs10091391
https://doaj.org/article/8c0ae060162749e59f856da56500872f
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spelling ftdoajarticles:oai:doaj.org/article:8c0ae060162749e59f856da56500872f 2023-05-15T14:01:44+02:00 Antarctic Snowmelt Detected by Diurnal Variations of AMSR-E Brightness Temperature Lei Zheng Chunxia Zhou Ruixi Liu Qizhen Sun 2018-08-01T00:00:00Z https://doi.org/10.3390/rs10091391 https://doaj.org/article/8c0ae060162749e59f856da56500872f EN eng MDPI AG http://www.mdpi.com/2072-4292/10/9/1391 https://doaj.org/toc/2072-4292 2072-4292 doi:10.3390/rs10091391 https://doaj.org/article/8c0ae060162749e59f856da56500872f Remote Sensing, Vol 10, Iss 9, p 1391 (2018) Antarctica snowmelt AMSR-E MEMLS Science Q article 2018 ftdoajarticles https://doi.org/10.3390/rs10091391 2022-12-31T16:19:37Z 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. Article in Journal/Newspaper Antarc* Antarctic Antarctic Peninsula Antarctica Ice Sheet Ice Shelf Shackleton Ice Shelf Directory of Open Access Journals: DOAJ Articles 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 Directory of Open Access Journals: DOAJ Articles
op_collection_id ftdoajarticles
language English
topic Antarctica
snowmelt
AMSR-E
MEMLS
Science
Q
spellingShingle Antarctica
snowmelt
AMSR-E
MEMLS
Science
Q
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
Science
Q
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 Article in Journal/Newspaper
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 MDPI AG
publishDate 2018
url https://doi.org/10.3390/rs10091391
https://doaj.org/article/8c0ae060162749e59f856da56500872f
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, Vol 10, Iss 9, p 1391 (2018)
op_relation http://www.mdpi.com/2072-4292/10/9/1391
https://doaj.org/toc/2072-4292
2072-4292
doi:10.3390/rs10091391
https://doaj.org/article/8c0ae060162749e59f856da56500872f
op_doi https://doi.org/10.3390/rs10091391
container_title Remote Sensing
container_volume 10
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