Error analysis based on a tunable wave plate polarization interferometric imaging spectrometer

Interference imaging spectroscopy combines modern imaging technology with spectral technology, holding significant importance for object imaging and spectral detection. This article introduces the principle of an adjustable wave plate polarization interferometric imaging spectrometer. The example design specifications are set for an observation wavelength range of 450–780 nm and a maximum resolution of 2 nm at 450 nm, with a 0.5 in detector as the base for calculating the specific dimensions of the Soleil–Babinet compensator. An investigation was conducted on the issues of nonuniform sampling, as well as three types of mechanical errors: flatness, wedge angle tolerance, and optical axis orientation accuracy. Emphasis was placed on discussing the impact of these errors on the instrument’s optical path difference and spectral reconstruction accuracy. This research provides theoretical guidance for the design and engineering of this miniaturized imaging spectrometer.

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Publication Details

Journal
Applied Optics
Published
2024-10-03
DOI
https://doi.org/10.1364/ao.538907
Primary Topic
Optical Polarization and Ellipsometry
Type
article
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article

Error analysis based on a tunable wave plate polarization interferometric imaging spectrometer

Feng Tang, Yanqiang Wang, Ke Ke, Zhen Ma et al.
Applied Optics
Optical Polarization and Ellipsometry
article

Error analysis based on a tunable wave plate polarization interferometric imaging spectrometer

Feng Tang, Yanqiang Wang, Ke Ke, Zhen Ma, Chunmin Zhang
article en

Abstract

Interference imaging spectroscopy combines modern imaging technology with spectral technology, holding significant importance for object imaging and spectral detection. This article introduces the principle of an adjustable wave plate polarization interferometric imaging spectrometer. The example design specifications are set for an observation wavelength range of 450–780 nm and a maximum resolution of 2 nm at 450 nm, with a 0.5 in detector as the base for calculating the specific dimensions of the Soleil–Babinet compensator. An investigation was conducted on the issues of nonuniform sampling, as well as three types of mechanical errors: flatness, wedge angle tolerance, and optical axis orientation accuracy. Emphasis was placed on discussing the impact of these errors on the instrument’s optical path difference and spectral reconstruction accuracy. This research provides theoretical guidance for the design and engineering of this miniaturized imaging spectrometer.

Applied OpticsVol. 63(30)
Chinese Academy of Sciences (CN), Daiseung Medics (South Korea) (KR), Xi'an Jiaotong University (CN)
Affordable and clean energy
Openalex Percentile: Top 84%
Optical Polarization and Ellipsometry
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