两台望远镜与 CHARA 阵列实验室之间的室外光纤连接,波长 810 nm。光路伺服控制演示

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Experimental Astronomy Pub Date : 2024-03-14 DOI:10.1007/s10686-024-09935-x
Magri Julie, Grossard Ludovic, Reynaud François, Fabert Marc, Delage Laurent, Krawczyk Rodolphe, Le Duigou Jean-Michel
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引用次数: 0

摘要

ALOHA(天文光学混合分析)项目致力于利用光纤和非线性光学技术在 L 波段进行高分辨率成像,在该项目框架内,我们在两台望远镜和 CHARA 望远镜阵列的重组光束设施之间建立了一个伺服控制的公倍数室外光纤链路。两级伺服系统使用光纤调制器、光纤延迟线和波长为 1064 nm 的计量激光器,可在 3000 秒的记录中将光路差稳定在 3 nm RMS 范围内。利用波长为 810 nm 的内部光源,当伺服控制开启时,条纹调制峰值的信噪比提高了 2 倍以上。这项研究也可被视为超长基线光纤链路望远镜阵列的开创性工作,并可扩展室外光纤链路的扰动环境。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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Outdoor fibre link between two telescopes and the lab of the CHARA array at 810 nm. Demonstration of the optical path servo control

In the framework of the ALOHA (Astronomical Light Optical Hybrid Analysis) project, dedicated to high resolution imaging in the L-band using optical fibre and nonlinear optics, we have implemented a servo controlled hectometric outdoor fibre link between two telescopes and the recombination beam facility of the CHARA telescope array. A two-stage servo system using optical fibre modulator, fibre delay line, and a metrology laser at 1064 nm allows to stabilise the optical path difference within 3 nm RMS over a 3000 s record. Using an internal source at 810 nm, the signal-to-noise ratio of the fringe modulation peak is enhanced by a factor better than two when the servo control is switched on. This study can be also considered as a seminal work towards very long base fibre linked telescope arrays and allows to scale the perturbative environment of an outdoor fibre link.

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来源期刊
Experimental Astronomy
Experimental Astronomy 地学天文-天文与天体物理
CiteScore
5.30
自引率
3.30%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Many new instruments for observing astronomical objects at a variety of wavelengths have been and are continually being developed. Furthermore, a vast amount of effort is being put into the development of new techniques for data analysis in order to cope with great streams of data collected by these instruments. Experimental Astronomy acts as a medium for the publication of papers of contemporary scientific interest on astrophysical instrumentation and methods necessary for the conduct of astronomy at all wavelength fields. Experimental Astronomy publishes full-length articles, research letters and reviews on developments in detection techniques, instruments, and data analysis and image processing techniques. Occasional special issues are published, giving an in-depth presentation of the instrumentation and/or analysis connected with specific projects, such as satellite experiments or ground-based telescopes, or of specialized techniques.
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