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Phased array of large reflectors for deep-space communication

机译:大型反射器的相控阵,用于深空通信

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In this paper the problem of uplink array calibration for deep-space communication is considered. A phased array of many modest-size reflectors antennas is used to drastically improve the uplink effective isotropic radiated power of a ground station. A radar calibration procedure for the array phase distribution is presented using a number of in-orbit targets. Design of optimal orbit and the number of calibration targets is investigated for providing frequent calibration opportunities needed for compensating array elements phase center movements as the array tracks a spacecraft. Array far-field focusing based on the near-filed in-orbit (low Earth orbit (LEO)) calibration targets is also presented and array gain degradation analysis based on the position error of the array elements and in-orbit targets has been carried out. It is shown that errors in the in-orbit targets positions significantly degrade the far-field array gain while the errors in array elements positions are not very important. Analysis of phase errors caused by thermal noise, system instability, and atmospheric effects show insignificant array gain degradation by these factors
机译:本文考虑了用于深空通信的上行链路阵列校准问题。许多适中尺寸的反射器天线的相控阵被用来极大地改善地面站的上行链路有效各向同性辐射功率。利用许多在轨目标,提出了一种用于阵列相位分布的雷达校准程序。研究了最佳轨道的设计和校准目标的数量,以提供频繁的校准机会,以补偿在阵列跟踪航天器时阵列元素的相位中心运动。还提出了基于近场在轨(低地球轨道(LEO))标定目标的阵列远场聚焦,并基于阵列元件和在轨目标的位置误差进行了阵列增益衰减分析。 。结果表明,在轨目标位置的误差大大降低了远场阵列增益,而阵列单元位置的误差不是很重要。由热噪声,系统不稳定和大气影响引起的相位误差分析表明,这些因素对阵列增益的影响不明显

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