天体光子学中集成多模到单模波导跃迁的超快激光刻录

R. Thomson, T. Birks, S. Leon-Saval, A. Kar, J. Bland-Hawthorn
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引用次数: 7

摘要

天体光子学是将光子原理应用于天文仪器,以降低成本、尺寸、重量和复杂性,同时提高性能。在天体光子学中,“光子灯”(PL)[1-4]是一种非凡的光子器件,它可以在多模(MM)光纤和一组简并单模(SMs)之间有效地耦合光,这些简并单模(SMs)由单个SM光纤[1-3]或多芯光纤[4]的核心引导。如果由PL产生的SMs被安排成线性阵列[5],则PL便于使用MM光纤从望远镜有效地收集光,并将该光的低损耗重新格式化为接近衍射限制的输入(在一个轴上),用于光谱仪[6]。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Ultrafast laser inscription of an integrated multimode-to-single-modes waveguide transition for astrophotonics
Astrophotonics is the application of photonic principles to astronomical instrumentation, in order to reduce cost, size, weight and complexity while increasing performance. In astrophotonics the “photonic lantern” (PL) [1–4] is a remarkable photonic device which efficiently couples light between a multimode (MM) optical fibre and a set of degenerate single modes (SMs) which are guided by the cores of either individual SM fibres [1–3] or a multicore optical fibre [4]. If the SMs produced by the PL are arranged into a linear array [5], the PL facilitates the efficient collection of light from a telescope using a MM fibre and the low-loss reformatting of this light into a near diffraction limited input (in one axis) for a spectrometer [6].
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