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AN AUTOMATIC PROCEDURE FOR IMPROVING SEA SURFACE WIND FIELD ESTIMATION FROM X-BAND COSMO-SKYMED SAR DATA

机译:改善X波段Cosmo-Skymed SAR数据的海面风场估计的自动过程

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The Synthetic Aperture Radar (SAR) has been increasingly used as the key sensor for extracting environmental information over the ocean surface and in particular for characterizing a wide range of ocean parameters such as waves, wind, surf and currents. In particular, ScanSAR acquisition mode has been widely employed for sea surface observation due to its peculiarities to provide data with huge swath and low revisit time. In SAR data the study of ocean parameters depend on the atmosphere-sea surface interaction that results in features and imprints appearance, e.g. wind direction retrieval is achievable from the orientation of Atmospheric Boundary Layer (ABL) rolls. Unfortunately, features extraction can be corrupted by the presence of processing artifacts, i.e. scalloping, and atmospheric artifacts that hamper image interpretation. In this paper, an automatic procedure able to perform scalloping suppression and atmospheric fronts analysis over Multi-Look Ground Detected (MGD) ScanSAR HugeRegion X-band Cosmo-SkyMed(CSK) is presented. Experimental results confirm the physical soundness of the proposed model from an operational view point.
机译:合成孔径雷达(SAR)已经越来越多地用作用于在海洋表面上提取环境信息的关键传感器,特别是用于表征诸如波浪,风,冲浪和电流的广泛海洋参数。特别地,由于其特点,ScanSAR采集模式已被广泛用于海面观察,以提供具有巨大条件和低重差时间的数据。在SAR数据中,海洋参数的研究取决于大气 - 海表面相互作用,从而产生特征和印记外观,例如,从大气边界层(ABL)辊的方向可以实现风向检索。遗憾的是,通过处理伪影的存在,即妨碍图像解释的扇形和大气伪影,可以损坏特征。本文介绍了一种能够在检测到的多外观接地(MGD)Scansar Hualeregion X频带Cosmo-Skymed(CSK)上进行扇形抑制和大气前部分析的自动过程。实验结果证实了从操作视点中提出的模型的物理声音。

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