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Resolution and synthetic aperture characterization of sparse radar arrays

机译:稀疏雷达阵列的分辨率和合成孔径表征

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摘要

The concept of radar satellite constellations, or clusters, for synthetic aperture radar (SAR), moving target indicator (MTI), and other radar modes has been proposed and is currently under research. These constellations form an array that is sparsely populated and irregularly spaced; therefore, traditional matched filtering is inadequate for dealing with the constellation's radiation pattern. To aid in the design, analysis, and signal processing of radar satellite constellations and sparse arrays in general, the characterization of the resolution and ambiguity functions of such systems is investigated. We project the radar's received phase history versus five sensor parameters: time, frequency, and three-dimensional position, into a phase history in terms of two eigensensors that can be interpreted as the dimensions of a two-dimensional synthetic aperture. Then, the synthetic aperture expression is used to derive resolution and the ambiguity function. Simulations are presented to verify the theory.
机译:已经提出了用于合成孔径雷达(SAR),运动目标指示器(MTI)和其他雷达模式的雷达卫星星座或群集的概念,目前正在研究中。这些星座形成了一个稀疏且间隔不规则的阵列。因此,传统的匹配滤波不足以处理星座的辐射方向图。通常,为了辅助雷达卫星星座图和稀疏阵列的设计,分析和信号处理,研究了此类系统的分辨率和歧义函数的特性。我们将雷达的接收相位历史与五个传感器参数(时间,频率和三维位置)相对应,投影到一个相位历史中,即两个本征传感器,这些特征传感器可以解释为二维合成孔径的尺寸。然后,使用合成孔径表达式得出分辨率和模糊函数。通过仿真验证了该理论。

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