旋转天线本振子的光分布

M. Bibey, S. Formont, F. Deborgies, C. Moronvalle, G. Auvray, A. Brillman
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引用次数: 2

摘要

研究了旋转天线的光LO分布。建立了一个具有4条微波链路和1条光学数字链路的光学演示器。不同波长的信号沿着同一根光纤向两个方向传播。加性相位噪声的测量表明,在S和c波段可以达到所需的规格:-135 dBc/Hz在10 kHz偏移。研究了通道间的电隔离和光反馈引起的相位噪声退化,并提出了改善这些参数的解决方案。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Optical distribution of local oscillators for a rotating antenna
Optical LO distribution to a rotating antenna has been studied. An optical demonstrator has been built with four microwave links and one optical digital link. Signals at different wavelengths are travelling in both directions along the same optical fibre. Measurements of additive phase noise show that the required specifications in S- and C-band can be reached: -135 dBc/Hz at 10 kHz offset. Electric isolation between channels and optical feedback inducing degradation of phase noise have also been studied and solutions have been proposed to improve these parameters.
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