用于射电天文学的光纤连接LIFT

C. Clivati, R. Ambrosini, C. Bortolotti, G. Costanzo, M. Frittelli, F. Levi, A. Mura, F. Perini, M. Roma, M. Zucco, D. Calonico
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引用次数: 3

摘要

光纤链路不仅有利于频率计量,也有利于其他物理研究领域,如射电天文学和大地测量学。我们实现了从国家计量研究所到用于甚长基线干涉测量和大地测量的射电望远镜的第一条光纤连接,距离超过544公里。我们对意大利中部梅迪纳射电望远镜中用作频率参考的氢脉泽进行了远程校准,以反对意大利Cs喷泉初级频率标准。这种比较受到氢脉泽统计不确定性的限制。该实验表明,光链路可以为射电天文设施提供非常精确和稳定的频率参考,在角度上优于目前使用的氢脉泽。这为VLBI的极限和更精确的空间大地测量开辟了新的视角。
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The optical fiber link LIFT for radioastronomy
Optical fiber links are beneficial not only for frequency metrology, but also for other fields of physical research, such as radioastronomy and geodesy. We realized the first optical fiber link from a National Institute of Metrology to a Radiotelescope used for Very Long Baseline Interferometry and for geodetic measurements, over a distance of 544 km. We performed a remote calibration of the hydrogen-maser used as a frequency reference at Medicina Radiotelescopes, in central Italy, against the Italian Cs fountain primary frequency standard. The comparison was limited by the statistical uncertainty of the hydrogen-masers. This experiment demonstrates that optical links can provide radioastronomical facilities with very accurate and stable frequency references, in perspective better than the currently used hydrogen-masers. This opens new perspectives in the ultimate limits of VLBI and a more precise space geodesy.
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