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Pretreatment and Wavelength Selection Method for Near-Infrared Spectra Signal Based on Improved CEEMDAN Energy Entropy and Permutation Entropy

机译:基于改进的CeeMDAN能量熵和排列熵的预处理和波长选择方法近红外光谱信号

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摘要

The noise of near-infrared spectra and spectral information redundancy can affect the accuracy of calibration and prediction models in near-infrared analytical technology. To address this problem, the improved Complete Ensemble Empirical Mode Decomposition with Adaptive Noise (CEEMDAN) and permutation entropy (PE) were used to propose a new method for pretreatment and wavelength selection of near-infrared spectra signal. The near-infrared spectra of glucose solution was used as the research object, the improved CEEMDAN energy entropy was then used to reconstruct spectral data for removing noise, and the useful wavelengths are selected based on PE after spectra segmentation. Firstly, the intrinsic mode functions of original spectra are obtained by improved CEEMDAN algorithm. The useful signal modes and noisy signal modes were then identified by the energy entropy, and the reconstructed spectral signal is the sum of useful signal modes. Finally, the reconstructed spectra were segmented and the wavelengths with abundant glucose information were selected based on PE. To evaluate the performance of the proposed method, support vector regression and partial least square regression were used to build the calibration model using the wavelengths selected by the new method, mutual information, successive projection algorithm, principal component analysis, and full spectra data. The results of the model were evaluated by the correlation coefficient and root mean square error of prediction. The experimental results showed that the improved CEEMDAN energy entropy can effectively reconstruct near-infrared spectra signal and that the PE can effectively solve the wavelength selection. Therefore, the proposed method can improve the precision of spectral analysis and the stability of the model for near-infrared spectra analysis.
机译:近红外光谱和光谱信息冗余的噪声可以影响近红外分析技术中的校准和预测模型的准确性。为了解决这个问题,使用具有自适应噪声(CeeMDAN)和排列熵(PE)的改进的完整集合经验模式分解来提出一种用于近红外光谱信号的预处理和波长选择的新方法。然后使用葡萄糖溶液的近红外光谱作为研究对象,然后使用改进的CeeMDAN能量熵来重建用于去除噪声的光谱数据,并且基于光谱分割后基于PE选择有用的波长。首先,通过改进的CeeMDAN算法获得原始光谱的内在模式功能。然后通过能量熵识别有用的信号模式和噪声信号模式,并且重建的光谱信号是有用信号模式的总和。最后,将重建的光谱进行分段,基于PE选择具有丰富血糖信息的波长。为了评估所提出的方法的性能,使用支持向量回归和部分最小二乘回归来使用新方法,相互信息,连续投影算法,主成分分析和全谱数据选择的波长来构建校准模型。通过预测的相关系数和根均方误差来评估模型的结果。实验结果表明,改进的CeeMDAN能量熵可以有效地重建近红外光谱信号,并且PE可以有效地解决波长选择。因此,该方法可以提高光谱分析的精度和近红外光谱分析模型的稳定性。

著录项

  • 作者

    Xiaoli Li; Chengwei Li;

  • 作者单位
  • 年度 2017
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  • 原文格式 PDF
  • 正文语种 eng
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