First steps for a Giant FOG: Searching for the limits

E. de Toldi, H. Lefèvre, F. Guattari, A. Bigueur, Adrien Steib, D. Ponceau, C. Moluçon, E. Ducloux, J. Wassermann, U. Schreiber
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引用次数: 9

Abstract

Based on recent experiences developing very low noise fiber-optic gyroscopes (FOG), as presented at ISS-2016, first performance results on very large optical fiber coils of up to 1 m diameter are presented. The goal for constructing large FOGs is to evaluate experimentally the physical limits of this kind of technology and to reach the lowest possible noise. While these experiments are probing the fundamental limits of FOG technology, they also serves as a first step for a cost effective very low noise laboratory rotational seismometer and will contribute in a second step to performance improvements on the portable rotational seismometer ‘blueSeis-3A&B’. This goal has several difficulties: the first one is the winding of the coil, the second concerns the mechanical substrate, and the third is, as usual, related to the measurement. To our knowledge, a winding machine, large enough to wind a 1 meter-diameter coil, does not exist, but thanks to iXblue expertise in the manufacturing of winding machines and calibration tables, a hydride system has been designed, merging these two technologies to fulfill the requirement of winding a large coil on an adequate rotational platform. The characterization of the wobble of the system is presented, since this is a critical parameter for the winding and ultimately the performance. To decrease the sensor sensitivity to environmental noises, unrelated to real ground rotation, is a critical process to achieve the highest attainable measurement sensitivity in seismology. The mechanical substrate of the coil is critical, as it must handle thermal, acoustic, magnetic, and electromagnetic isolation. To demonstrate a very low self-noise, the ideal way is to find an experiment place near a much more precise instrument in a calm enough location. The seismic station collocated to ROMY tetrahedral ring-laser gyroscope [0] is the ideal place to do that. Results of different prototypes during the development process are presented to underline the applicability of each technological response to the Large-FOG requirements. Finally we conclude with presentation of the achieved results with a 1 meter-diameter FOG having a fiber length of 5000 meters.
巨大雾的第一步:寻找极限
根据最近在ISS-2016上展示的开发超低噪声光纤陀螺仪(FOG)的经验,介绍了直径达1米的超大光纤线圈的首次性能结果。构建大型雾化器的目标是通过实验来评估这种技术的物理极限,并达到尽可能低的噪声。虽然这些实验正在探索光纤陀螺技术的基本限制,但它们也可以作为具有成本效益的极低噪声实验室旋转地震仪的第一步,并将在第二步为便携式旋转地震仪“blueSeis-3A&B”的性能改进做出贡献。这个目标有几个困难:第一个是线圈的缠绕,第二个涉及机械基板,第三个是,像往常一样,与测量有关。据我们所知,目前还没有大到足以缠绕直径为1米的线圈的绕线机,但由于iXblue在绕线机和校准表制造方面的专业知识,我们设计了一个氢化物系统,将这两种技术融合在一起,以满足在适当的旋转平台上缠绕大线圈的要求。提出了系统摆动的特性,因为这是绕组和最终性能的关键参数。在地震学中,降低传感器对与实际地面旋转无关的环境噪声的灵敏度是实现最高测量灵敏度的关键过程。线圈的机械基板是至关重要的,因为它必须处理热、声、磁和电磁隔离。为了演示非常低的自噪声,理想的方法是在足够安静的地方找到一个靠近更精确的仪器的实验场所。配备ROMY四面体环形激光陀螺仪[0]的地震台站是实现这一目标的理想场所。在开发过程中,提出了不同原型的结果,以强调每种技术响应对Large-FOG要求的适用性。最后给出了光纤长度为5000米,光纤直径为1米的光纤光纤的实验结果。
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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