首页> 外文会议>19th International technical meeting of the Satellite Division of the Institute of Navigation (ION GNSS 2006) >Satellite-to-Satellite Interference Effects Observed in High-Rate C/A-Code Power Measurements
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Satellite-to-Satellite Interference Effects Observed in High-Rate C/A-Code Power Measurements

机译:高速C / A码功率测量中观察到的卫星到卫星干扰效应

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Ionospheric scintillation studies required the development of Global Positioning System (GPS) receivers that could record high-rate correlator power measurements for the Coarse-Acquisition (C/A) code signal on the L1 carrier frequency. Spectrograms of 50-Hz power data soon revealed unusual time-varying patterns of weak power fluctuations that nonetheless were significant with respect to the background noise level. These spectrogram patterns, with approximately linear and parabolic forms, do not appear to be well known in the literature, although related phenomena have been observed and reported. We present examples of the patterns and evidence for their origin in satellite-to-satellite C/A-code interference. Among other factors, we demonstrate that the maximum value of the inter-satellite correlation term is not the -21.6 dB to be expected from the direct C/A-code cross-correlation result but rather is of the order of -9 dB. This inter-satellite correlation term permits the development ofrnradio wave interference between pairs of satellites that meet appropriate Doppler shift and amplitude criteria, ultimately leading to the observed spectrogram patterns. It is important to ionospheric scintillation studies, and other civil radio wave interference studies, to be able to separate these inter-satellite effects from daily and transient multipath effects. Therefore, we suggest some techniques to discriminate between these phenomena. The goal of this paper is to raise general awareness of these inter-satellite interference effects for GPS, although applications to other tasks such as satellite orbital parameter estimation may be possible in the long term.
机译:电离层闪烁研究要求开发全球定位系统(GPS)接收器,该接收器可以在L1载波频率上记录粗采集(C / A)码信号的高速率相关器功率测量。 50 Hz功率数据的频谱图很快显示出微弱的功率波动的异常时变模式,但相对于背景噪声电平而言却很重要。尽管已经观察到并报道了相关现象,但是这些具有近似线性和抛物线形式的频谱图模式在文献中似乎并不为人们所熟知。我们提供了模式示例及其在卫星到卫星C / A码干扰中的起源证据。除其他因素外,我们证明了卫星间相关项的最大值不是直接C / A码互相关结果所预期的-21.6 dB,而是约为-9 dB。这个卫星间相关项允许在满足适当多普勒频移和振幅标准的成对卫星之间发展无线电波干扰,最终导致观察到的频谱图模式。对于电离层闪烁研究和其他民用无线电波干扰研究而言,重要的是要能够将这些卫星间效应与日常和瞬态多径效应区分开。因此,我们建议一些技术来区分这些现象。本文的目的是提高人们对GPS的这些卫星间干扰影响的一般认识,尽管从长远来看,可能将其应用于其他任务,例如卫星轨道参数估计。

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