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    請使用永久網址來引用或連結此文件: https://ir.lib.ncu.edu.tw/handle/987654321/98126


    題名: 光譜量測之校正程序;Spectral Measurement Calibration Procedure
    作者: 趙柏幀;Chao, Po-Chen
    貢獻者: 照明與顯示科技研究所
    關鍵詞: 單光儀;光譜儀;反捲積;校正;Monochromator;Spectrometer;Deconvolution;Calibration
    日期: 2025-08-27
    上傳時間: 2025-10-17 12:23:10 (UTC+8)
    出版者: 國立中央大學
    摘要: 本研究提出一種方法,用以從光譜儀量測結果中重建原始光譜,該量測結果常因儀器響應與光學捲積效應而失真。在實驗中,利用連續光譜的寬頻白光通過單色儀,產生窄頻可見光,接著使用光譜儀進行量測與分析。
    單色儀透過旋轉其光柵調整中心波長,以掃描特定波長。然而,由於光學系統解析度有限,每個像素接收到的訊號實際上是來自鄰近波長的整合結果,使得所量測的光譜實際上為原始光譜與儀器響應之捲積結果。
    為了還原原始光譜,本研究將量測資料轉換至頻率域,並分析系統響應,特別關注由矩形窗函數傅立葉轉換所產生的 Sinc 函數特性。由於 Sinc 函數在某些頻率點會等於零,若在頻域中直接除以該響應,容易放大雜訊。因此,本研究引入Tikhonov 正則化方法,來抑制反捲積過程中產生的雜訊。

    ;This study proposes a method to reconstruct the original spectrum from spectrometer measurements, which are often distorted due to instrument response and optical convolution effects. In the experiment, broadband white light with a continuous spectrum is passed through a monochromator to produce narrowband visible light, which is then measured and analyzed using a spectrometer.
    The monochromator scans specific wavelengths by rotating its diffraction grating to adjust the central wavelength. However, due to the limited resolution of the optical system, each pixel receives an integrated signal from neighboring wavelengths, resulting in a measured spectrum that is the convolution of the original spectrum and the instrument response.
    To recover the original spectrum, the measured data is transformed into the frequency domain using the Fourier transform, and the system response is analyzed, with particular attention to the characteristics of the Sinc function resulting from the Fourier transform of a rectangular window. Since the Sinc function becomes zero at certain frequencies, direct division in the frequency domain tends to amplify noise. Therefore, this study introduces the Tikhonov Regularization method to suppress noise generated during the deconvolution process.
    顯示於類別:[照明與顯示科技研究所 ] 博碩士論文

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