首页> 外文期刊>Optik: Zeitschrift fur Licht- und Elektronenoptik: = Journal for Light-and Electronoptic >Polarization effects in KAT-7 telescope optical fibre network: Towards the distribution of frequency and timing references in the MeerKAT telescope
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Polarization effects in KAT-7 telescope optical fibre network: Towards the distribution of frequency and timing references in the MeerKAT telescope

机译:KAT-7望远镜光纤网络中的极化效果:迈进Meerkat望远镜的频率和定时引用分布

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摘要

Polarization mode dispersion (PMD) is one of the key effects in optical fibre communication that distorts the transmitted signal. The effect of birefringence on the polarization states of an optical signal leads to broadening of the pulses in an optical fibre. The difference in propagation time of the orthogonal modes in a fibre results in differential group delay (DGD). For proper functioning of a telescope, accurate and stable clock signals will be distributed via an optical fibre network to each of the dishes. This paper presents field PMD measurement that is essential in estimating the expected phase change of the clock signal. The average DGD of a 10.2 km fibre link established to be about 62.1 fs. This study serves to address the applicability of optical fibre network transmission in the distribution of frequency and timing reference signals in the MeerKAT and later phases of the square kilometre array (SKA) telescope. (C) 2017 Elsevier GmbH. All rights reserved.
机译:偏振模式色散(PMD)是扭曲发送信号的光纤通信中的关键效果之一。 双折射对光信号的偏振状态的影响导致光纤中的脉冲的展宽。 光纤中的正交模式的传播时间的差异导致差分组延迟(DGD)。 为了望远镜的正常运行,精确稳定的时钟信号将通过光纤网络分布到每个菜肴。 本文介绍了现场PMD测量,这在估计时钟信号的预期相位变化方面是必不可少的。 建立10.2公里的光纤链路的平均DGD为约62.1fs。 本研究有助于解决光纤网络传输在Meerkat(SKA)望远镜的Meerkat中的频率和定时参考信号的分布中的应用。 (c)2017年Elsevier GmbH。 版权所有。

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