Broadband astigmatism-free Czerny-Turner imaging spectrometer using spherical mirrors.

We describe the elimination of the astigmatism of a Czerny-Turner imaging spectrometer, built using spherical optics and a plane grating, over a broad spectral region. Starting with the principle of divergent illumination of the grating, which removes astigmatism at one chosen wavelength, we obtain...

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Main Authors: Austin, DR, Witting, T, Walmsley, I
Format: Journal article
Language:English
Published: 2009
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author Austin, DR
Witting, T
Walmsley, I
author_facet Austin, DR
Witting, T
Walmsley, I
author_sort Austin, DR
collection OXFORD
description We describe the elimination of the astigmatism of a Czerny-Turner imaging spectrometer, built using spherical optics and a plane grating, over a broad spectral region. Starting with the principle of divergent illumination of the grating, which removes astigmatism at one chosen wavelength, we obtain design equations for the distance from the grating to the focusing mirror and the detector angle that remove the astigmatism to first order in wavelength. Experimentally, we demonstrate near diffraction-limited performance from 740 to 860 nm and over a 5 mm transverse spatial extent, while ray-tracing calculations show that barring finite-aperture and detector size limitations, this range extends from 640 to 900 nm and over 10 mm transversely. Our technique requires no additional optics and uses standard off-the-shelf components.
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spelling oxford-uuid:86d8262c-053b-4270-8bf8-21920241a8612022-03-26T22:06:53ZBroadband astigmatism-free Czerny-Turner imaging spectrometer using spherical mirrors.Journal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:86d8262c-053b-4270-8bf8-21920241a861EnglishSymplectic Elements at Oxford2009Austin, DRWitting, TWalmsley, IWe describe the elimination of the astigmatism of a Czerny-Turner imaging spectrometer, built using spherical optics and a plane grating, over a broad spectral region. Starting with the principle of divergent illumination of the grating, which removes astigmatism at one chosen wavelength, we obtain design equations for the distance from the grating to the focusing mirror and the detector angle that remove the astigmatism to first order in wavelength. Experimentally, we demonstrate near diffraction-limited performance from 740 to 860 nm and over a 5 mm transverse spatial extent, while ray-tracing calculations show that barring finite-aperture and detector size limitations, this range extends from 640 to 900 nm and over 10 mm transversely. Our technique requires no additional optics and uses standard off-the-shelf components.
spellingShingle Austin, DR
Witting, T
Walmsley, I
Broadband astigmatism-free Czerny-Turner imaging spectrometer using spherical mirrors.
title Broadband astigmatism-free Czerny-Turner imaging spectrometer using spherical mirrors.
title_full Broadband astigmatism-free Czerny-Turner imaging spectrometer using spherical mirrors.
title_fullStr Broadband astigmatism-free Czerny-Turner imaging spectrometer using spherical mirrors.
title_full_unstemmed Broadband astigmatism-free Czerny-Turner imaging spectrometer using spherical mirrors.
title_short Broadband astigmatism-free Czerny-Turner imaging spectrometer using spherical mirrors.
title_sort broadband astigmatism free czerny turner imaging spectrometer using spherical mirrors
work_keys_str_mv AT austindr broadbandastigmatismfreeczernyturnerimagingspectrometerusingsphericalmirrors
AT wittingt broadbandastigmatismfreeczernyturnerimagingspectrometerusingsphericalmirrors
AT walmsleyi broadbandastigmatismfreeczernyturnerimagingspectrometerusingsphericalmirrors