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A Wide-Swath Spaceborne TOPS SAR Image Formation Algorithm Based on Chirp Scaling and Chirp-Z Transform

机译:基于Chirp scaling和Chirp-Z变换的宽幅星载TOps saR图像形成算法

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摘要

Based on the terrain observation by progressive scans (TOPS) mode, an efficientudfull-aperture image formation algorithm for focusing wide-swath spaceborne TOPS data is proposed.udFirst, to overcome the Doppler frequency spectrum aliasing caused by azimuth antenna steering,udthe range-independent derotation operation is adopted, and the signal properties after derotationudare derived in detail. Then, the azimuth deramp operation is performed to resolve image foldingudin azimuth. The traditional dermap function will introduce a time shift, resulting in appearanceudof ghost targets and azimuth resolution reduction at the scene edge, especially in the wide-swathudcoverage case. To avoid this, a novel solution is provided using a modified range-dependent derampudfunction combined with the chirp-z transform. Moreover, range scaling and azimuth scaling areudperformed to provide the same azimuth and range sampling interval for all sub-swaths, instead of theudinterpolation operation for the sub-swath image mosaic. Simulation results are provided to validateudthe proposed algorithm.
机译:基于逐行扫描(TOPS)模式对地形的观测,提出了一种有效的 udper-perperture成像算法,用于聚焦广域星载TOPS数据。 ud首先,要克服由方位角天线操纵引起的多普勒频谱混叠,采用了与范围无关的解旋操作,详细推导了解旋后的信号特性。然后,执行方位角去采样操作以解决图像折叠 udin方位角。传统的dermap函数将引入时移,从而导致外观 udof幻影目标的出现和场景边缘的方位分辨率降低,尤其是在宽幅 udcoverage情况下。为了避免这种情况,提供了一种新颖的解决方案,它使用了与chirp-z变换相结合的,范围相关的deramp udfunction。此外,对距离缩放和方位角缩放进行了演算,以为所有子波段提供相同的方位角和范围采样间隔,而不是对子波段图像镶嵌图进行了内插操作。仿真结果验证了所提算法的有效性。

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