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

机译:反射天线孔径场恢复使用具有三个固定参考波的相移全息术

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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.
机译:提出一种方法,用于通过记录具有参考波的固定相移的三个全息图来重建反射器天线的孔径场。进行了大率-600无线电望远镜的自动调压模式中的数学分析和模拟,并提出了初始实验结果。在无线电望远镜上使用该方法不需要特殊接收设备,并且标准无线电天文接收器可用于具有相干远程接地或空间信号源的全息测量。表面层大气湍流对三个全息图的连续记录过程的影响将限制大地面无线电望远镜方法的可用性。然而,由于其简单性,该方法可以成功地应用于较小的精密接地反射器天线(最多50米)或任何具有有源表面的精密空间无线电望远镜的全息测量。

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