Phase Synchronization of Distorted Imaging Antenna Arrays

B. Steinberg
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引用次数: 0

Abstract

Diffraction-limited performance of an imaging system is often unattainable without some feedback-controlled compensation built into the image-forming process. Dielectric-constant perturbations due to atmospheric turbulence distort the phasefront of the optical radiation field. Muller and Buffington have discovered a class of integrals of the image intensity which, when maximized by adjustments of a compensating lens or mirror, reduce the error in the image to zero, except for an unknown shift in the optical axis [1]. This is a remarkable theorem. Its success depends upon the spatial incoherence of optical sources. Another approach, due to Gerchberg and Saxton [2], utilizes known properties of the class of expected signals, their autocorrelations or their Fourier transforms. It introduces considerable heuristics into the iterative Fourier transformation process. After each successive transformation, portions of the image or its Fourier transform are retained and portions deleted. Retention or deletion is based on a priori scene information and the physics of the process. Ref. [3] and [4] apply [2] to the optical problem.
畸变成像天线阵列的相位同步
成像系统的衍射限制性能通常是无法实现的,如果没有一些反馈控制的补偿内置于图像形成过程。大气湍流引起的介电常数扰动使光辐射场的相前变形。Muller和Buffington已经发现了一类图像强度的积分,当通过补偿透镜或反射镜的调整使其最大化时,除了光轴的未知位移外,图像中的误差将减少到零[1]。这是一个了不起的定理。它的成功取决于光源的空间非相干性。另一种方法是由Gerchberg和Saxton[2]提出的,它利用了期望信号的已知性质、它们的自相关性或它们的傅里叶变换。它在迭代傅里叶变换过程中引入了相当多的启发式方法。在每次连续变换之后,图像或其傅里叶变换的部分被保留,部分被删除。保留或删除是基于先验的场景信息和物理过程。参考文献[3]和[4]将[2]应用于光学问题。
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