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Sea State Impacts on Wind Speed Retrievals From C-Band Radars.
- Source :
- IEEE Journal of Selected Topics in Applied Earth Observations & Remote Sensing; May2017 Part 2, Vol. 10 Issue 5, p2147-2155, 9p
- Publication Year :
- 2017
-
Abstract
- Scatterometers, a proven technology, provide ocean wind speeds and directions that are essential in operational forecasts, monitoring of the climate, and scientific applications. While the missions and geophysical model functions are performing well, challenges remain. We analyze data from advanced scatterometer (ASCAT) aboard MetOp-A and the advanced synthetic aperture radar (ASAR) aboard Envisat, both of which operate in the C-band, against the in situ buoy wind speeds. We observe large variability in the wind speed residuals. Through analysis of these residuals, we find that they are related to sea state effects and atmospheric stability. The sea state dependence created by low-frequency swells is more pronounced for the lower incidence angles in ASCAT. In ASAR with a fixed angle of 23°, the sea state dominates the wind speed errors and these trends increase with the significant wave height. We observe that wind speeds from ASAR and ASCAT have a close resemblance, which helps us to extrapolate our findings. The synergy between the two technologies can be further exploited to improve wind speed retrievals. Future scatterometer missions, such as the next MetOp, will operate with the wider range of incidence angles (including lower angles) to increase their coverage together, have higher spatial resolution, and obtain measurements closer to the coasts. In these cases, high-resolution SAR data can aide in the understanding of the radar response. [ABSTRACT FROM PUBLISHER]
Details
- Language :
- English
- ISSN :
- 19391404
- Volume :
- 10
- Issue :
- 5
- Database :
- Complementary Index
- Journal :
- IEEE Journal of Selected Topics in Applied Earth Observations & Remote Sensing
- Publication Type :
- Academic Journal
- Accession number :
- 127949997
- Full Text :
- https://doi.org/10.1109/JSTARS.2016.2609101