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Dual-polarized C- and Ku-band ocean backscatter response to hurricane-force winds

机译:双极化C波段和Ku波段海洋背向散射对飓风强风的响应

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摘要

Airborne ocean backscatter measurements at C- and Ku-band wavelengths and H and V polarizations at multiple incidence angles obtained in moderate to very high wind speed conditions (25–65 m s−1) during missions through several tropical cyclones are presented. These measurements clearly show that the normalized radar cross sections (NRCS) response stops increasing at hurricane-force winds for both frequency bands and polarizations except for high incidence angles at C-band and H polarization. The results also show the mean NRCS departing from a power law behavior for all the presented frequency bands, polarizations, and incidence angles, suggesting a reduction in the drag coefficient. The overall flattening of the azimuthal response of the NRCS is also very apparent in all cases. A new set of geophysical model functions (GMFs) at C- and Ku-band are developed from these direct ocean backscatter observations for ocean surface winds ranging from 25 to 65 m s−1. The developed GMFs provide a much more accurate characterization of the NRCS versus wind speed and direction, and their implementation in operational retrieval algorithms from satellite-based scatterometer observations would result in better wind fields. The differences between these measurements and other currently available GMFs, such as QuikSCAT, NSCAT2, CMOD4, and CMOD5, are reported. The implementation of these GMFs in retrieval algorithms will result in better wind fields from satellite-based scatterometers measurements.
机译:提出了在中风到极高风速条件下(25–65 m s-1)通过多个热带气旋执行的任务期间,在多个入射角在C和Ku波段波长下进行的空中海洋反向散射测量。这些测量结果清楚地表明,除了C波段和H偏振的入射角较高之外,在两个频段和偏振的飓风风中,归一化雷达横截面(NRCS)的响应都不再增加。结果还表明,对于所有显示的频带,极化和入射角,平均NRCS均偏离幂律行为,这表明阻力系数降低了。在所有情况下,NRCS方位角响应的整体变平也非常明显。根据这些直接的海洋反向散射观测结果,针对25至65 m s-1的海洋表面风,开发了C波段和Ku波段的一组新的地球物理模型函数(GMF)。已开发的GMF提供了NRCS与风速和风向的更准确的表征,并且在基于卫星的散射仪观测结果的操作检索算法中实施它们会产生更好的风场。报告了这些测量值与其他当前可用的GMF(例如QuikSCAT,NSCAT2,CMOD4和CMOD5)之间的差异。这些GMF在检索算法中的实施将通过基于卫星的散射仪测量获得更好的风场。

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