NASA NTRS · 19930066891
Passive microwave remote sensing of thin sea ice using principal component analysis
Abstract
The 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.
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Wensnahan, Mark, Maykut, Gary A., Grenfell, Thomas C., Winebrenner, Dale P.. 1993-07-15. Passive microwave remote sensing of thin sea ice using principal component analysis. https://ntrs.nasa.gov/citations/19930066891
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