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In-Situ Pattern Measurement of the Johns Hopkins University Applied Physics Laboratory 60-foot Parabolic Reflector Antenna

机译:约翰·霍普金斯大学应用物理实验室的60英尺抛物面反射天线的原位方向图测量

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In-situ pattern measurement of JHU/APL's 60-foot parabolic reflector antenna (S-band), using a low-earth orbit satellite as the source is described. The signal strength and X and Y tracking error voltages are measured as the antenna dish sweeps a matrix of points around the position of the moving satellite. The swept region is approximately ±0.30° from the antenna's boresight. This technique was evaluated during April 1998.rnThis measurement was used to baseline the current performance of the ground station before the feed underwent significant modifications. Before the new feed assembly was installed, the position of the current feed was translated to the new feed assembly. Once installed the performance of the reflector was verified. Misalignment of the feed broadens the main beam and increases the sidelobes. More importantly, the inclusion of new components inside the feed also has the potential to introduce phase errors onto the tracking signals. These phase errors will be translated by the auto-track electronics into pointing errors causing the antenna system to inaccurately follow a target. This paper describes the measurement of the reflector antenna pattern and tracking pattern before the new assembly was installed. Results of pattern measurements with the new assembly will be presented at the conference.
机译:描述了使用低地球轨道卫星作为源头对JHU / APL的60英尺抛物面反射器天线(S波段)进行的原位方向图测量。当天线天线在移动卫星的位置周围扫描点矩阵时,将测量信号强度以及X和Y跟踪误差电压。扫描区域与天线的视轴成大约±0.30°。该技术在1998年4月进行了评估。该测量用于在对馈源进行重大修改之前将地面站的当前性能作为基准。在安装新的提要组件之前,当前提要的位置已转换为新的提要组件。安装完成后,反射器的性能将得到验证。进给不对准会扩大主光束并增加旁瓣。更重要的是,在馈送中包含新的组件也有可能将相位误差引入到跟踪信号中。这些相位误差将由自动跟踪电子设备转换为指向误差,从而导致天线系统不准确地跟随目标。本文介绍了在安装新组件之前对反射器天线方向图和跟踪方向图的测量。新组件的图案测量结果将在会议上介绍。

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