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首页> 外文期刊>Cosmic research >Fundamental Constraints on the Coherence of Probing Signals in the Problem of Maximizing the Resolution and Range in the Stroboscopic Range of Asteroids
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Fundamental Constraints on the Coherence of Probing Signals in the Problem of Maximizing the Resolution and Range in the Stroboscopic Range of Asteroids

机译:在小行星频闪观测范围内的分辨率和射程最大化问题中探测信号相干性的基本约束

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摘要

The problem of coherence violation in stroboscopic ranging with a high resolution in the range due to mutual phase instability of probing and reference radio signals has been considered. It has been shown that the violation of coherence in stroboscopic ranging systems is equivalent to the action of modulating interface and leads to a decrease in the system sensitivity. Requirements have been formulated for the coherence of reference generators in the stroboscopic processing system. The results of statistical modeling have been presented. It was shown that, in the current state of technology with stability of the frequencies of the reference generators, the achieved coherence is sufficient to probe asteroids with super-resolving signals in the range of up to 70 million kilometers. In this case, the dispersion of the signal in cosmic plasma limits the value of the linear resolution of the asteroid details at this range by the value of similar to 2.7 m. Comparison with the current radar resolution of asteroids has been considered, which, at the end of 2015, were similar to 7.5 m in the range of similar to 7 million kilometers.
机译:已经考虑了由于探测和参考无线电信号的相互相位不稳定性而在频域内以高分辨率在频闪范围内发生相干冲突的问题。已经表明,频闪测距系统中相干性的破坏等同于调制界面的作用,并导致系统灵敏度的降低。已为频闪处理系统中参考发生器的相干性提出了要求。统计建模的结果已经提出。结果表明,在目前技术水平以及参考发生器频率稳定的情况下,所获得的相干性足以探测超小信号的小行星,探测信号的范围高达7000万公里。在这种情况下,信号在宇宙等离子体中的分散将在此范围内小行星细节的线性分辨率值限制为类似于2.7 m的值。已考虑将其与当前小行星的雷达分辨率进行比较,到2015年底,该分辨率与7.5 m相似,范围约为700万公里。

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