Paper
13 September 2012 Potential applications of ring resonators for astronomical instrumentation
S. C. Ellis, A. Crouzier, J. Bland-Hawthorn, J. S. Lawrence, J. Kepple
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Abstract
Ring resonators are a looped waveguide coupled to an input and an output waveguide. They can be used to filter, and drop, a series of wavelengths at the resonant frequencies of the ring. Both these properties are useful for astronomical applications. The dropped signal provides a frequency comb that can be used to provide accurate wavelength calibration. The free spectral range of such a device is larger than that from a laser comb, removing the requirement to perform subsequent filtering. The filtered signal could be used to suppress specific wavelengths, e.g. corresponding to atmospheric emission lines. We present the expected performance of devices designed for both applications and discuss their advantages and limitations.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
S. C. Ellis, A. Crouzier, J. Bland-Hawthorn, J. S. Lawrence, and J. Kepple "Potential applications of ring resonators for astronomical instrumentation", Proc. SPIE 8450, Modern Technologies in Space- and Ground-based Telescopes and Instrumentation II, 84501J (13 September 2012); https://doi.org/10.1117/12.925804
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CITATIONS
Cited by 5 scholarly publications.
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KEYWORDS
Resonators

Frequency combs

Waveguides

Spectrographs

Astronomy

Calibration

Linear filtering

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