| Literature DB >> 26901202 |
Chu Zhang1, Hui Ye2, Fei Liu3, Yong He4, Wenwen Kong5, Kuichuan Sheng6.
Abstract
Biomass energy represents a huge supplement for meeting current energy demands. A hyperspectral imaging system covering the spectral range of 874-1734 nm was used to determine the pH value of anaerobic digestion liquid produced by water hyacinth and rice straw mixtures used for methane production. Wavelet transform (WT) was used to reduce noises of the spectral data. Successive projections algorithm (SPA), random frog (RF) and variable importance in projection (VIP) were used to select 8, 15 and 20 optimal wavelengths for the pH value prediction, respectively. Partial least squares (PLS) and a back propagation neural network (BPNN) were used to build the calibration models on the full spectra and the optimal wavelengths. As a result, BPNN models performed better than the corresponding PLS models, and SPA-BPNN model gave the best performance with a correlation coefficient of prediction (rp) of 0.911 and root mean square error of prediction (RMSEP) of 0.0516. The results indicated the feasibility of using hyperspectral imaging to determine pH values during anaerobic digestion. Furthermore, a distribution map of the pH values was achieved by applying the SPA-BPNN model. The results in this study would help to develop an on-line monitoring system for biomass energy producing process by hyperspectral imaging.Entities:
Keywords: anaerobic digestion; distribution map; hyperspectral imaging; pH value; variable selection
Mesh:
Year: 2016 PMID: 26901202 PMCID: PMC4801620 DOI: 10.3390/s16020244
Source DB: PubMed Journal: Sensors (Basel) ISSN: 1424-8220 Impact factor: 3.576
Figure 1The unpreprocessed of spectra of (a) five randomly selected pixels; (b) the spectra of the five pixels preprocessed by WT; and (c) the average spectra of each sample.
The statistic description of sample sets split.
| Sample Set | Number | Range | Mean | STD a |
|---|---|---|---|---|
| Calibration set | 62 | 7.13–7.48 | 7.34 | 0.10 |
| Prediction set | 31 | 7.13–7.46 | 7.31 | 0.10 |
STD = standard deviation.
The results of PLS model and BPNN model on full spectra.
| Models | LVs a/Nodes | Calibration | Prediction | ||
|---|---|---|---|---|---|
| RMSEC | RMSEP | ||||
| PLS | 10/ | 0.904 | 0.0443 | 0.880 | 0.0695 |
| BP | /14 | 0.910 | 0.0446 | 0.894 | 0.0684 |
LVs were the number of latent variables in PLS model; nodes were the number of nodes in the hidden layer of BPNN mode.
The optimal wavelengths selected by SPA, RF and VIP.
| Methods | Number | Optimal Wavelengths (nm) |
|---|---|---|
| SPA | 8 | 1210.29, 1395.67, 1129.54, 1287.75, 1058.95, 1574.74, 1520.64, 1372.05 |
| RF | 15 | 1378.8, 1274.27, 1183.36, 1237.22, 1240.59, 1270.91, 1301.23, 1375.42, 1277.64, 1129.54, 1176.63, 1109.36, 1159.8108, 1095.92, 1388.92 |
| VIP | 20 | 1042.16, 1045.52, 1156.4399, 1159.8108, 1163.9, 1166.54, 1203.55, 1206.92, 1210.29, 1213.65, 1217.02, 1355.1801, 1358.55, 1361.9301, 1365.3, 1395.67, 1399.04, 1402.42, 1405.79, 1409.17 |
The results of PLS models and BPNN models on optimal wavelengths selected by SPA, RF and VIP.
| Methods | PLS | BP | ||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| LVs | Calibration | Prediction | Nodes | Calibration | Prediction | |||||
| RMSEC | RMSEP | RMSEC | RMSEP | |||||||
| SPA | 7 | 0.891 | 0.0471 | 0.853 | 0.0697 | 6 | 0.941 | 0.0351 | 0.911 | 0.0516 |
| RF | 11 | 0.852 | 0.0545 | 0.829 | 0.0698 | 10 | 0.903 | 0.0463 | 0.877 | 0.0589 |
| VIP | 12 | 0.866 | 0.0519 | 0.822 | 0.0745 | 5 | 0.921 | 0.0417 | 0.820 | 0.0636 |
Figure 2The results of SPA-BPNN model (a) calibration set; (b) prediction set.
Figure 3The pseudo color image of (a) a hyperspectral image and (b) the corresponding distribution map of pH obtained by SPA-BPNN.