Fiber-based Microwave Interferometer monitoring the Delay of Fiber-Optic Antenna Downlinks in Radioastronomic Scenarios

J. Nanni, Enrico Lenzi, F. Perini, J. Monari, G. Tartarini
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Abstract

In large radioastronomic facilities, such as the Square Kilometre Array (SKA), where arrays of a great many antennas are connected to the processing station through optical fiber connections, the monitoring of the phase shift (or, equivalently, of the delay) induced to the transmitted signal by each optical link is crucial for the array calibration process. Indeed, these connections typically lie (partially or totally) in environments where climate/environmental agents can change the electromagnetic properties of the cable in a significant measure and in a different fashion between one fiber and the other, and this can therefore have a different impact on the value of phase shift (or delay) of each travelling signal. This paper proposes a simple and low-cost technique based on a microwave interferometer realized on optical fiber to monitor the delay introduced by the optical connections and its variations due to external climate agents.
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基于光纤的微波干涉仪监测射电天文场景下光纤天线下行链路的时延
在大型射电天文设施中,如平方公里阵列(SKA),其中大量天线阵列通过光纤连接到处理站,监测每个光链路引起的传输信号的相移(或等效的延迟)对于阵列校准过程至关重要。事实上,这些连接通常(部分或全部)位于气候/环境因素可以显著改变电缆电磁特性的环境中,并且在一根光纤和另一根光纤之间以不同的方式改变,因此这可能对每个传播信号的相移(或延迟)值产生不同的影响。本文提出了一种简单、低成本的基于光纤微波干涉仪的技术,用于监测光纤连接所带来的延迟以及外界气候因素对延迟的影响。
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