An efficient wavefront curvature correction algorithm for turntable spotlight ISAR systems using stepped frequency waveforms

S.D. Fisher, M. Richards, J. McClellan
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Abstract

Wavefront curvature phenomena have a noticeably negative impact on the final formed image, removing the distortion and defocusing effects become an important step in a turntable ISAR imaging system. This paper outlines an efficient wavefront curvature correction algorithm that corrects the distortion effects by implementing a set of 1-D operations in spatial frequency before the final image is formed. By implementing the algorithm in spatial frequency space, several advantages over post-image formation wavefront curvature correction techniques can be realized. The first advantage is that this algorithm can be broken down into a set of 1-D operations that can be applied across each row or column of the 2-D spatial frequency data grid, while post-image formation techniques can require a 2-D spatially varying filter, or a pixel-by-pixel remapping, to "unwarp" and focus the image. The second advantage of this algorithm stems from the fact that the number of data samples in the spatial frequency domain is often much smaller than the number of samples in the final image, because relatively large discrete Fourier transforms (DFTs) are used in image formation to create finely-detailed imagery. Performing the correction in the frequency domain thus requires operation on fewer samples than does correcting the warping in the more densely-sampled image domain.
基于阶跃频率波形的转台聚光灯ISAR系统波前曲率校正算法
波前曲率现象对最终形成的图像有明显的负面影响,消除畸变和散焦效应成为转台ISAR成像系统的重要步骤。本文概述了一种有效的波前曲率校正算法,该算法通过在最终图像形成之前在空间频率上实施一组一维操作来校正畸变效应。通过在空间频率空间中实现该算法,可以实现相对于成像后波前曲率校正技术的几个优点。第一个优点是,该算法可以分解成一组1-D操作,可以应用于2-D空间频率数据网格的每一行或每一列,而图像后形成技术可能需要一个2-D空间变化滤波器,或逐像素重新映射,以“解扭曲”和聚焦图像。该算法的第二个优点是,由于在图像形成中使用了相对较大的离散傅里叶变换(dft)来创建精细的图像,因此空间频域的数据样本数量通常比最终图像中的样本数量要小得多。因此,在频域中执行校正所需的操作比在更密集采样的图像域中校正翘曲所需的操作更少。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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