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通道式光谱偏振计光谱响应的推导与校准。

Derivation and calibration of spectral response for a channeled spectropolarimeter.

作者信息

Zhao Zhe, Li Yanqiu, Liu Ke, Zhou Guodong

出版信息

Opt Express. 2023 Jul 31;31(16):25763-25780. doi: 10.1364/OE.492952.

Abstract

The channeled spectropolarimeter (CSP) measures the spectrally-resolved Stokes vector from a snapshot by employing spectral modulation. The spectral modulation transfer function (SMTF) of the spectrometer preferentially suppresses the high-frequency channel amplitude in CSP, resulting in reduced measurement accuracy. This paper rigorously derives the SMTF theory and proposes an efficient calibration method for SMTF via channel shifting in a CSP. The SMTF value, obtained by channel shifting, is used to correct the high-frequency channel amplitude. Moreover, alignment and phase errors, as well as nonlinear dispersion, are compensated in situ. Other than rotating the retarder twice, no additional instruments or algorithms are required in the proposed method. In simulations and experiments, the proposed method shows high accuracy, with a maximum root-mean-square error (RMSE) of the reconstructed Stokes spectrum below 0.01, demonstrating its potential for enhancing the simplicity and practicability of Stokes CSP.

摘要

通道式光谱偏振计(CSP)通过采用光谱调制从快照中测量光谱分辨的斯托克斯矢量。光谱仪的光谱调制传递函数(SMTF)优先抑制CSP中的高频通道幅度,导致测量精度降低。本文严格推导了SMTF理论,并提出了一种通过CSP中的通道移位对SMTF进行有效校准的方法。通过通道移位获得的SMTF值用于校正高频通道幅度。此外,对准误差、相位误差以及非线性色散都在原位得到补偿。除了将延迟器旋转两次外,该方法不需要额外的仪器或算法。在模拟和实验中,该方法显示出高精度,重建的斯托克斯光谱的最大均方根误差(RMSE)低于0.01,证明了其在提高斯托克斯CSP的简单性和实用性方面的潜力。

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