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Passive microwave remote sensing of thin sea ice using principal component analysisThe possibility of developing a satellite-based sea-ice-concentration algorithm which solves for the presence of thinner ice is explored on the basis of time sequences of surface-based measurements of passive MW emission from growing saline ice reported by Wensnahan et al. (1993). It is shown that two classes of thinner ice can be distinguished from mixtures of open water, first-year ice, and multiyear ice. Newly formed ice appears to be optically thick at 37 and 90 GHz and has a relatively dry surface. The thin ice spectrum occurs when the ice is greater than 4 cm thick and appears to result from the accumulation of brine at the ice surface. Thin ice has a relatively stable spectrum characterized by high brightness temperatures, a near-zero spectral gradient at vertical polarization, and a large difference between vertical and horizontal polarizations. It is concluded that thin ice can be detected using satellite data.
Document ID
19930066891
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Wensnahan, Mark
(NASA Headquarters Washington, DC United States)
Maykut, Gary A.
(NASA Headquarters Washington, DC United States)
Grenfell, Thomas C.
(NASA Headquarters Washington, DC United States)
Winebrenner, Dale P.
(Washington Univ. Seattle, United States)
Date Acquired
August 16, 2013
Publication Date
July 15, 1993
Publication Information
Publication: Journal of Geophysical Research
Volume: 98
Issue: C7
ISSN: 0148-0227
Subject Category
Oceanography
Accession Number
93A50888
Funding Number(s)
CONTRACT_GRANT: NGT-50723
CONTRACT_GRANT: NAGW-2574
CONTRACT_GRANT: N00014-89-J-1140
Distribution Limits
Public
Copyright
Other

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