Paper
29 June 2006 Coupling light into optical fibres near the diffraction limit
Author Affiliations +
Abstract
The burgeoning field of astrophotonics explores the interface between astronomy and photonics. Important applications include photonic OH suppression at near-infrared wavelengths, and integrated photonic spectroscopy. These new photonic mechanisms are not well matched to conventional multi-mode fibre bundles, and are best fed with single or few-mode fibres. We envisage the largest gains in astrophotonics will come from instruments that operate with single or few mode fibres in the diffraction limited or near diffraction limited regime. While astronomical instruments have largely solved the problem of coupling light into multi-mode fibres, this is largely unexplored territory for few-mode and single-mode fibres. Here we describe a project to explore this topic in detail, and present initial results on coupling light into single and few-mode fibres at the diffraction limit. We find that fibres with as few as ~ 5 guided modes have qualitatively different behaviour to single-mode fibres and share a number of the beneficial characteristics of multi-mode fibres.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Anthony J. Horton and Joss Bland-Hawthorn "Coupling light into optical fibres near the diffraction limit", Proc. SPIE 6269, Ground-based and Airborne Instrumentation for Astronomy, 62691K (29 June 2006); https://doi.org/10.1117/12.670943
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KEYWORDS
Single mode fibers

Astronomy

Diffraction

Adaptive optics

Astrophotonics

Telescopes

Optical fibers

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