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- W3157305293 abstract "In astronomical spectroscopy, optical fibers are abundantly used for multiplexing and decoupling the spectrograph from the telescope to provide stability in a controlled environment. However, fibers are less than perfect optical components and introduce complex effects that diminish the overall throughput, efficiency, and stability of the instrument. We present a novel numerical field propagation model that emulates the effects of modal noise, scrambling, and focal ratio degradation with a rigorous treatment of wave optics. We demonstrate that the simulation of the near- and far-field output of a fiber, injected into a ray-tracing model of the spectrograph, allows us to assess performance at the detector level." @default.
- W3157305293 created "2021-05-10" @default.
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- W3157305293 date "2021-05-24" @default.
- W3157305293 modified "2023-10-03" @default.
- W3157305293 title "Mode expansion theory and application in step-index multimode fibers for astronomical spectroscopy" @default.
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- W3157305293 doi "https://doi.org/10.1364/josab.423866" @default.
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