Ultrafast laser inscription of an integrated multimode-to-single-modes waveguide transition for astrophotonics

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

Abstract

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].
天体光子学中集成多模到单模波导跃迁的超快激光刻录
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。
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