Reflector Antenna Aperture Field Recovery using Phase Shift Holography with Three Fixed Reference Waves

A. Ripak, V. Khaikin, M. Lebedev, G. Junkin
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引用次数: 3

Abstract

A method is proposed for reconstructing the aperture field of a reflector antenna by recording three holograms having fixed phase shifts of the reference wave. Mathematical analysis and simulation of the method in the autocollimation mode of the RATAN-600 radio telescope were performed and initial experimental results are presented. Using this proposed method on a radio telescope does not require special receiving equipment and a standard radio astronomy receiver can be used for holography measurements with a coherent remote ground or space signal source. The influence of the surface layer atmospheric turbulence on the process of consecutive recording of three holograms will limit the usability of the method for large ground radio telescopes. However, due to its simplicity, the method can be successfully applied to holographic measurement of smaller precision ground reflector antennas (up to 50 m) or any precision space radio telescope with an active surface.
三固定参考波相移全息法反演反射面天线孔径场
提出了一种通过记录参考波相移固定的三个全息图来重建反射面天线孔径场的方法。对该方法在RATAN-600射电望远镜自准直模式下进行了数学分析和仿真,并给出了初步实验结果。在射电望远镜上使用这种方法不需要特殊的接收设备,并且标准的射电天文接收器可以用于具有相干远程地面或空间信号源的全息测量。地表大气湍流对连续记录三个全息图过程的影响将限制该方法在大型地面射电望远镜上的可用性。然而,由于其简单性,该方法可以成功地应用于较小精度地面反射天线(高达50米)或任何具有活动表面的精密空间射电望远镜的全息测量。
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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