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3-D Inverse Synthetic Aperture Ladar Imaging and Scaling of Space Debris Based on the Fractional Fourier Transform

机译:基于分数傅里叶变换的3D逆合成孔径雷达成像和空间碎片缩放

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摘要

The inverse synthetic aperture ladar (ISAL) is an important method for observation and imaging of space targets. Here, a 3-D ISAL imaging algorithm is proposed for spinning targets such as space debris. Since laser wavelength is 4-5 orders of magnitude smaller than that of microwave, the Doppler frequency caused by target motion is more pronounced in ISAL. Doppler frequency modulation rates can he estimated by the fractional Fourier transform with respect to azimuth slow time even when the rotation angle is small such that scattering centers do not migrate through a range cell. Then, slant range, Doppler frequency, and Doppler frequency modulation rates form a 3-D space. The angular velocity and the incident angle can he estimated by the position relationship between the scattering centers in two observations. After image scaling, the 3-D shape and size of the target can be obtained. The 3-D structure of the target in the simulation experiment is accurately reconstructed. Monte Carlo experiments are conducted to discuss the effect of the signal-to-noise ratio and observation time on the algorithm. Finally, the effectiveness and robustness of the algorithm are verified.
机译:合成孔径逆激光雷达(ISAL)是观察和成像空间目标的重要方法。在此,提出了一种用于旋转目标(例如空间碎片)的3-D ISAL成像算法。由于激光波长比微波波长小4-5个数量级,因此目标运动引起的多普勒频率在ISAL中更为明显。即使当旋转角很小使得散射中心不会通过测距单元迁移时,也可以通过分数傅里叶变换相对于方位角慢时间来估计多普勒频率调制率。然后,倾斜范围,多普勒频率和多普勒频率调制率形成一个3-D空间。可以通过两次观察中散射中心之间的位置关系来估算角速度和入射角。图像缩放后,可以获得目标的3D形状和大小。仿真实验中目标的3-D结构被精确地重建。进行了蒙特卡罗实验,以讨论信噪比和观察时间对算法的影响。最后,验证了算法的有效性和鲁棒性。

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