Abstract
High-accurate evaluation of coal quality is crucial for efficient energy use. Laser-induced breakdown spectroscopy (LIBS), a fast and efficient detection method, has become a key focus in the field of coal quality detection. However, the complexity of the coal matrix significantly limits the classification accuracy of LIBS, hardly meeting the current needs. To overcome this challenge, a novel plasma image-spectrum fusion method was proposed in this study. It provided supplementary information to the spectra through the plasma images, thus significantly improving the accuracy of coal classification models. To verify the classification accuracy of this method, a systematic experimental study was carried out. The spectra, coaxial plasma images, and paraxial plasma images of coal samples were obtained simultaneously, and three different data fusion schemes were compared with the traditional spectral scheme. Meanwhile, three machine learning models, k-nearest neighbor (KNN), decision tree (Tree), and support vector machine (SVM), were used to verify the broad applicability of this method. The results demonstrated that the performance of the classification models based on fusion schemes significantly improved compared with those based solely on spectra. Among them, the classification models based on spectra coupled with coaxial plasma images and paraxial plasma images achieved the best classification results. The accuracies of the prediction set of these three models (KNN, Tree, and SVM) were improved from 76.51%, 91.23%, and 93.69% to 89.05%, 97.90%, and 96.65%, respectively. Therefore, the relevant results fully verify the feasibility and wide applicability of this method.
© The Royal Society of Chemistry 2025
© The Royal Society of Chemistry 2025
| Original language | English |
|---|---|
| Pages (from-to) | 1796-1803 |
| Number of pages | 8 |
| Journal | Journal of Analytical Atomic Spectrometry |
| Volume | 40 |
| Issue number | 7 |
| Online published | 5 May 2025 |
| DOIs | |
| Publication status | Published - 1 Jul 2025 |
Funding
This research was financially supported by the National Key Research and Development Program of China (No. 2022YFE0118700), National Natural Science Foundation of China (No. 62405138), Open Project Program of Wuhan National Laboratory for Optoelectronics (No. 2023WNLOKF008), and the Science Research Project of the Hubei Provincial Department of Education, China (No. D20222703).
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