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Spectral Calibration Method for All-Reflected Fourier TransformImaging Spectrometer

机译:用于全反射傅里叶变压镜谱仪的光谱校准方法

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All-Reflected Fourier Transform Imaging Spectrometer (ARFTIS) is a novel type of instrument based on Fouriertransform spectroscopy. ARFTIS will offer high luminous flux and high spectral resolution, well suited to remote sensingwith low energy. But there is nearly not any method of convenient spectrum calibration for this kind of instrument. Inthis paper, we analyze the spectrum calibration principle of ARFTIS and the cause of the calibration error. We reachedthe result that the calibration error is getting bigger with the increase of spectrum peak wavelength of the calibration light.By these we develop three convenient spectrum calibration methods used in Visible/Near-Infrared waveband, which arethe Monochromatic Method, the Average Method and the Weighted Average Method respectively. We apply thesemethods to ARFTIS calibrate experiment. According to the experiment results, The Monochromatic Method cancalibrate by using only one group of data, but with a little lower calibration precision. However the Weighted AverageMethod can provide a higher calibration precision than the other two methods. So, the Monochromatic method and theWeighted Average Method both have good application value for ARFTIS calibration.
机译:全反映的傅立叶变换成像光谱仪(ARFTIS)是一种基于FourierTransform光谱的新型仪器。 ARFTIS将提供高光通量和高光谱分辨率,非常适合于遥感的低能量。但是几乎没有任何用于这种仪器的方便谱校准方法。纸张,我们分析了ARFTIS的频谱校准原理和校准误差的原因。我们达到了校准误差随着校准光的频谱峰值波长的增加而越来越大。通过这些,我们开发了三种方便的光谱校准方法,用于可见/近红外波段,这是单色方法,平均方法和加权平均法。我们将其作为Arftis Calibrate实验应用。根据实验结果,单色方法仅使用一组数据凝固,但校准精度稍低。然而,加权AverageMethod可以提供比其他两种方法更高的校准精度。因此,单色方法和重量的平均方法都具有良好的ARFTIS校准应用值。

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