存在星历误差时卫星传输的空间获取

M. Plonski
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引用次数: 0

摘要

自动远程跟踪站(ARTS)计划的一个组成部分是自动获取卫星传输的能力。在星历表不精确的异常情况下,在进行单脉冲跟踪以完成采集之前,有必要确保天线位于主波束上。ARTS项目使用基于辅助孔径振幅比较(AAAC)的自动主波束采集程序进行初始主波束检测,然后进行主波束汇聚的质心定位。提出了一种确定用于AAAC的鲁棒决策边界的方法。与其他方法相比,该边界允许更大的误差容忍度和更低的输入动态范围成本。此外,还提出了几种改进的替代方案,以用于主束收敛。这些技术并不局限于卫星,可以用来获取来自任何发射机的传输信息。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Spatial acquisition of satellite transmissions in the presence of ephemeris errors
One component of the Automated Remote Tracking Station (ARTS) Program is the ability to acquire a satellite transmission automatically. Under abnormal conditions, where the ephemeris is not precisely known, it is necessary to ensure that the antenna is positioned on the main beam prior to engaging monopulse tracking to complete the acquisition. The ARTS program uses an automated main beam acquisition procedure that is based on auxiliary-aperture amplitude comparison (AAAC) for initial main beam detection, followed by centroiding for main beam convergence. A method for determining a robust decision boundary for use in AAAC is presented. Compared to other methods, this boundary allows for greater tolerance of errors at a lower cost to the input dynamic range. Several improved alternatives to centroiding for main beam convergence are also presented. These techniques are not restricted to satellites and can be used to acquire the transmission from any transmitter.<>
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