Highly-chirped Bragg gratings for integrated silica spectrometers
Highly-chirped Bragg gratings for integrated silica spectrometers
A blazed chirped Bragg grating in a planar silica waveguide device was used to create an integrated diffractive element for a spectrometer. The grating diffracts light from a waveguide and creates a wavelength dependent focus in a manner similar to a bulk diffraction grating spectrometer. An external imaging system is used to analyse the light, later device iterations plan to integrate detectors to make a fully integrated spectrometer. Devices were fabricated with grating period chirp rates in excess of 100nm/mm, achieving a focal length of 5.5 mm. Correction of coma aberrations resulted in a device with a footprint of 20 mm x 10mm, a peak FWHM resolution of 1.8 nm, a typical FWHM resolution of 2.6 nm and operating with a 160 nm bandwidth centered at 1550 nm.
21247-21259
Field, James
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Berry, Sam A
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Bannerman, Rex
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Smith, Devin H.
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Gawith, Corin
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Smith, Peter G.R.
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Gates, James
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6 July 2020
Field, James
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Berry, Sam A
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Bannerman, Rex
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Smith, Devin H.
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Gawith, Corin
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Smith, Peter G.R.
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Gates, James
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Field, James, Berry, Sam A, Bannerman, Rex, Smith, Devin H., Gawith, Corin, Smith, Peter G.R. and Gates, James
(2020)
Highly-chirped Bragg gratings for integrated silica spectrometers.
Optics Express, 28 (14), .
(doi:10.1364/OE.389211).
Abstract
A blazed chirped Bragg grating in a planar silica waveguide device was used to create an integrated diffractive element for a spectrometer. The grating diffracts light from a waveguide and creates a wavelength dependent focus in a manner similar to a bulk diffraction grating spectrometer. An external imaging system is used to analyse the light, later device iterations plan to integrate detectors to make a fully integrated spectrometer. Devices were fabricated with grating period chirp rates in excess of 100nm/mm, achieving a focal length of 5.5 mm. Correction of coma aberrations resulted in a device with a footprint of 20 mm x 10mm, a peak FWHM resolution of 1.8 nm, a typical FWHM resolution of 2.6 nm and operating with a 160 nm bandwidth centered at 1550 nm.
Text
J FIELD Highly Chirped Bragg Gratings for Integrated Silica Spectrometers
- Accepted Manuscript
More information
Accepted/In Press date: 13 May 2020
e-pub ahead of print date: 2 July 2020
Published date: 6 July 2020
Additional Information:
Funding Information:
Engineering and Physical Sciences Research Council (EP/M024539/1, EP/N509747/1). All data supporting this study are openly available from the University of Southampton repository at https://DOI.org/10.5258/SOTON/D1356
Publisher Copyright:
© 2020 OSA - The Optical Society. All rights reserved.
Copyright:
Copyright 2020 Elsevier B.V., All rights reserved.
Identifiers
Local EPrints ID: 440970
URI: http://eprints.soton.ac.uk/id/eprint/440970
ISSN: 1094-4087
PURE UUID: d1f8abd6-2a89-4d72-ba57-f27c4b496681
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Date deposited: 26 May 2020 16:31
Last modified: 17 Mar 2024 02:52
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Contributors
Author:
James Field
Author:
Sam A Berry
Author:
Rex Bannerman
Author:
Devin H. Smith
Author:
Corin Gawith
Author:
Peter G.R. Smith
Author:
James Gates
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