MICROWAVE SIGNATURE OF POLAR FIRN AND SEA ICE IN THE ANTARCTIC FROM AIRBORNE OBSERVATION

P(論文) Airborne observations of 19.35 GHz microwave radiation were taken over the sea ice and firn cover of Antarctic ice sheet. Microwave brightness temperature was analyzed to explain satellite observations.As for the polar firn over the ice sheet, brightness temperature varied greatly from the coa...

Full description

Bibliographic Details
Main Authors: ヤマノウチ, タカシ, ワダ, マコト, YAMANOUCHI, Takashi, WADA, Makoto
Language:English
Published: National Institute of Polar Research 1992
Subjects:
Online Access:https://nipr.repo.nii.ac.jp/record/3735/files/KJ00000767889.pdf
https://doi.org/10.15094/00003735
https://nipr.repo.nii.ac.jp/records/3735
_version_ 1829306961791811584
author ヤマノウチ, タカシ
ワダ, マコト
YAMANOUCHI, Takashi
WADA, Makoto
author_facet ヤマノウチ, タカシ
ワダ, マコト
YAMANOUCHI, Takashi
WADA, Makoto
author_sort ヤマノウチ, タカシ
collection National Institute of Polar Research Repository, Japan
description P(論文) Airborne observations of 19.35 GHz microwave radiation were taken over the sea ice and firn cover of Antarctic ice sheet. Microwave brightness temperature was analyzed to explain satellite observations.As for the polar firn over the ice sheet, brightness temperature varied greatly from the coast to the interior, which noticeably corresponded to the mean annual accumulation obtained at the surface. Also found was the variation of brightness temperature on a small scale of about 1-10 km, which became extreme in the sastrugi/glazed surface zone (Z route), where the accumulation is variable. Calculated emissivity using the semi-empirical relation to the accumulation rate and physical temperature proposed in the past could not always explain the observed emissivity because of the limit of the theoretical relation, or shortage of measurements. Satellite passive microwave observations were of very low resolution, making it difficult to show these small scale great variations corresponding to the surface accumulation. In the sea ice area, the brightness temperatures observed were similar to the results from the satellite. Brightness temperature was low for multi-year ice and high for first year fast ice; the brightness temperature for new ice increases from a lower value and converges to the value of first year ice. From the flight across Riiser-Larsen Peninsula, smooth variation up to 225K was seen over the central part of the peninsula. This high value could be explained by the extremely high accumulation, which occurred asymmetrically against the height of the peninsula. Also along the flight, it was easy to distinguish the ice shelf and sea ice, even when covered with snow, by microwave brightness temperature measurement. departmental bulletin paper
genre Antarc*
Antarctic
Ice Sheet
Ice Shelf
Polar meteorology and glaciology
Proceedings of the NIPR Symposium on Polar Meteorology and Glaciology
Sea ice
genre_facet Antarc*
Antarctic
Ice Sheet
Ice Shelf
Polar meteorology and glaciology
Proceedings of the NIPR Symposium on Polar Meteorology and Glaciology
Sea ice
geographic Antarctic
Riiser-Larsen
Riiser-Larsen Peninsula
Sastrugi
The Antarctic
geographic_facet Antarctic
Riiser-Larsen
Riiser-Larsen Peninsula
Sastrugi
The Antarctic
id ftnipr:oai:nipr.repo.nii.ac.jp:00003735
institution Open Polar
language English
long_lat ENVELOPE(50.667,50.667,-66.783,-66.783)
ENVELOPE(34.000,34.000,-68.917,-68.917)
ENVELOPE(163.683,163.683,-74.617,-74.617)
op_collection_id ftnipr
op_doi https://doi.org/10.15094/00003735
op_relation Proceedings of the NIPR Symposium on Polar Meteorology and Glaciology
6
16
35
AA10756213
https://nipr.repo.nii.ac.jp/record/3735/files/KJ00000767889.pdf
https://doi.org/10.15094/00003735
https://nipr.repo.nii.ac.jp/records/3735
publishDate 1992
publisher National Institute of Polar Research
record_format openpolar
spelling ftnipr:oai:nipr.repo.nii.ac.jp:00003735 2025-04-13T14:07:29+00:00 MICROWAVE SIGNATURE OF POLAR FIRN AND SEA ICE IN THE ANTARCTIC FROM AIRBORNE OBSERVATION ヤマノウチ, タカシ ワダ, マコト YAMANOUCHI, Takashi WADA, Makoto 1992-12 application/pdf https://nipr.repo.nii.ac.jp/record/3735/files/KJ00000767889.pdf https://doi.org/10.15094/00003735 https://nipr.repo.nii.ac.jp/records/3735 eng eng National Institute of Polar Research Proceedings of the NIPR Symposium on Polar Meteorology and Glaciology 6 16 35 AA10756213 https://nipr.repo.nii.ac.jp/record/3735/files/KJ00000767889.pdf https://doi.org/10.15094/00003735 https://nipr.repo.nii.ac.jp/records/3735 1992 ftnipr https://doi.org/10.15094/00003735 2025-03-19T10:19:57Z P(論文) Airborne observations of 19.35 GHz microwave radiation were taken over the sea ice and firn cover of Antarctic ice sheet. Microwave brightness temperature was analyzed to explain satellite observations.As for the polar firn over the ice sheet, brightness temperature varied greatly from the coast to the interior, which noticeably corresponded to the mean annual accumulation obtained at the surface. Also found was the variation of brightness temperature on a small scale of about 1-10 km, which became extreme in the sastrugi/glazed surface zone (Z route), where the accumulation is variable. Calculated emissivity using the semi-empirical relation to the accumulation rate and physical temperature proposed in the past could not always explain the observed emissivity because of the limit of the theoretical relation, or shortage of measurements. Satellite passive microwave observations were of very low resolution, making it difficult to show these small scale great variations corresponding to the surface accumulation. In the sea ice area, the brightness temperatures observed were similar to the results from the satellite. Brightness temperature was low for multi-year ice and high for first year fast ice; the brightness temperature for new ice increases from a lower value and converges to the value of first year ice. From the flight across Riiser-Larsen Peninsula, smooth variation up to 225K was seen over the central part of the peninsula. This high value could be explained by the extremely high accumulation, which occurred asymmetrically against the height of the peninsula. Also along the flight, it was easy to distinguish the ice shelf and sea ice, even when covered with snow, by microwave brightness temperature measurement. departmental bulletin paper Other/Unknown Material Antarc* Antarctic Ice Sheet Ice Shelf Polar meteorology and glaciology Proceedings of the NIPR Symposium on Polar Meteorology and Glaciology Sea ice National Institute of Polar Research Repository, Japan Antarctic Riiser-Larsen ENVELOPE(50.667,50.667,-66.783,-66.783) Riiser-Larsen Peninsula ENVELOPE(34.000,34.000,-68.917,-68.917) Sastrugi ENVELOPE(163.683,163.683,-74.617,-74.617) The Antarctic
spellingShingle ヤマノウチ, タカシ
ワダ, マコト
YAMANOUCHI, Takashi
WADA, Makoto
MICROWAVE SIGNATURE OF POLAR FIRN AND SEA ICE IN THE ANTARCTIC FROM AIRBORNE OBSERVATION
title MICROWAVE SIGNATURE OF POLAR FIRN AND SEA ICE IN THE ANTARCTIC FROM AIRBORNE OBSERVATION
title_full MICROWAVE SIGNATURE OF POLAR FIRN AND SEA ICE IN THE ANTARCTIC FROM AIRBORNE OBSERVATION
title_fullStr MICROWAVE SIGNATURE OF POLAR FIRN AND SEA ICE IN THE ANTARCTIC FROM AIRBORNE OBSERVATION
title_full_unstemmed MICROWAVE SIGNATURE OF POLAR FIRN AND SEA ICE IN THE ANTARCTIC FROM AIRBORNE OBSERVATION
title_short MICROWAVE SIGNATURE OF POLAR FIRN AND SEA ICE IN THE ANTARCTIC FROM AIRBORNE OBSERVATION
title_sort microwave signature of polar firn and sea ice in the antarctic from airborne observation
url https://nipr.repo.nii.ac.jp/record/3735/files/KJ00000767889.pdf
https://doi.org/10.15094/00003735
https://nipr.repo.nii.ac.jp/records/3735