| Literature DB >> 27441244 |
Chu Zhang1, Wenwen Kong1, Fei Liu1, Yong He1.
Abstract
Oilseed rape is used as both food and a renewable energy resource. Physiological parameters, such as the amino acid aspartic acid, can indicate the growth status of oilseed rape. Traditional detection methods are laborious, time consuming, costly, and not usable in the field. Here, we investigate near infrared spectroscopy (NIRS) as a fast and non-destructive detection method of aspartic acid in oilseed rape leaves under herbicide stress. Different spectral pre-processing methods were compared for optimal prediction performance. The variable selection methods were applied for relevant variable selection, including successive projections algorithm (SPA), Monte Carlo-uninformative variable elimination (MC-UVE) and random frog (RF). The selected effective wavelengths (EWs) were used as input by multiple linear regression (MLR), partial least squares (PLS) and least-square support vector machine (LS-SVM). The best predictive performance was achieved by SPA-LS-SVM (Raw) model using 22 EWs, and the prediction results were Rp = 0.9962 and RMSEP = 0.0339 for the prediction set. The result indicated that NIR combined with LS-SVM is a powerful new method to detect aspartic acid in oilseed rape leaves under herbicide stress.Entities:
Keywords: Agricultural engineering; Agricultural techniques; Data mining; Mass spectroscopy applications
Year: 2016 PMID: 27441244 PMCID: PMC4945898 DOI: 10.1016/j.heliyon.2015.e00064
Source DB: PubMed Journal: Heliyon ISSN: 2405-8440
Fig. 1The raw and preprocessed spectra of oilseed rape leaves: (a) Raw; (b) SG; (c) SNV; (d) MSC; (e) 1st-Der; (f) 2nd-Der; (g) De-trending; (h) DOSC.
Statistics of aspartic acid content of oilseed rape leaves.
| Set | Number | Range (mg/100 g DW) | Mean (mg/100 g DW) | Standard deviation(mg/100 g DW) |
|---|---|---|---|---|
| Calibration | 124 | 0.926-2.746 | 1.773 | 0.3810 |
| Validation | 62 | 0.937-2.579 | 1.775 | 0.3803 |
| Prediction | 62 | 0.932-2.662 | 1.773 | 0.3849 |
DW: dry matter.
Prediction results of aspartic acid by the PLS model with different preprocessing methods.
| Model | Treatment | LV/EW/(γ, σ2) | Calibration | Prediction | ||
|---|---|---|---|---|---|---|
| RMSEC | RMSEP | |||||
| PLS | Raw | 8/700/- | 0.9715 | 0.0899 | 0.9766 | 0.0824 |
| SG | 7/700/- | 0.9675 | 0.0956 | 0.9681 | 0.0958 | |
| SNV | 5/700/- | 0.9619 | 0.1037 | 0.9631 | 0.1029 | |
| MSC | 5/700/- | 0.9625 | 0.1030 | 0.9637 | 0.1021 | |
| 1st-Der | 6/700/- | 0.9768 | 0.0813 | 0.9789 | 0.0782 | |
| 2st-Der | 4/700/- | 0.9882 | 0.0582 | 0.9599 | 0.1111 | |
| De-trending | 6/700/- | 0.9687 | 0.0941 | 0.9731 | 0.0881 | |
| DOSC | 6/700/- | 0.9669 | 0.0968 | 0.9680 | 0.0958 | |
LV: latent variable in PLS model; EW: effective wavelengths used in the models; (γ, σ2): parameters of LS-SVM.
R: correlation coefficient of calibration; R: correlation coefficient of prediction; RMSEC: root mean square error of calibration; RMSEP: root mean square error of prediction.
Fig. 2Reference vs. predicted values of aspartic acid by PLS (1st-Der) in prediction set (The solid line is regression line and the dash line is the target 45 degree line).
Selected EWs by SPA, MC-UVE and RF.
| Treatment | No. | Selected EWs (nm) | ||
|---|---|---|---|---|
| SPA | Raw | 22 | 2304, 2272, 1410, 2372, 1190, 1730, 2098, 1528, 1438, 2058, 1692, 1104, 1878, 2022, 2234, 2178, 2290, 1344, 2352, 1818, 1994, 1942 | |
| 1st-Der | 17 | 1684, 1950, 2180, 2232, 1298, 1720, 2308, 1534, 1528, 2326, 2096, 2492, 1110, 2442, 1310, 2336, 2276 | ||
| MC-UVE | Raw | 22 | 1444, 1446, 2038, 1442, 2036, 2108, 1448, 2032, 1512, 2110, 1760, 1828, 1440, 2106, 1510, 1504, 1506, 2298, 2034, 1932, 1830, 1436 | |
| 1st-Der | 22 | 1248, 1146, 1430, 1330, 1144, 1328, 1246, 1428, 1660, 1148, 1250, 1714, 1658, 1712, 2284, 1432, 2384, 2382, 1662, 1224, 1716, 2286 | ||
| RF | Raw | 22 | 1334, 1340, 1828, 1252, 1328, 1140, 1244, 1254, 1326, 1816, 1336, 1804, 1142, 1246, 1830, 2198, 1342, 2200, 1332, 2362, 2202, 2082 | |
| 1st-Der | 26 | 1146, 1714, 1834, 1836, 1256, 1300, 2342, 1154, 1328, 1166, 1330, 1658, 2384, 1470, 1390, 1468, 1660, 2284, 1338, 1824, 1144, 1236, 1388, 1686, 1744, 2344 |
No.: number of selected effective wavelengths.
Prediction results by the MLR, PLS and LS-SVM models using EWs.
| Model | Treatment | LV/EW/(γ, σ2) | Calibration | Prediction | ||
|---|---|---|---|---|---|---|
| RMSEC | RMSEP | |||||
| SPA-MLR | Raw | -/22/- | 0.9811 | 0.0734 | 0.9833 | 0.0709 |
| 1st-Der | -/17/- | 0.9692 | 0.0934 | 0.9720 | 0.0898 | |
| SPA-PLS | Raw | 7/22/- | 0.9754 | 0.0837 | 0.9747 | 0.0854 |
| 1st-Der | 5/17/- | 0.9703 | 0.0918 | 0.9749 | 0.0860 | |
| SPA-LS-SVM | Raw | -/22/(7.1×104, 171.6) | 0.9936 | 0.0428 | 0.9962 | 0.0339 |
| 1st-Der | -/17/(749.0, 427.7) | 0.9907 | 0.0516 | 0.9871 | 0.0613 | |
| MC-UVE-MLR | Raw | -/22/- | 0.9706 | 0.0914 | 0.9647 | 0.1009 |
| 1st-Der | -/22/- | 0.9682 | 0.0949 | 0.9551 | 0.1145 | |
| MC-UVE-PLS | Raw | 5/22/- | 0.9509 | 0.1174 | 0.9554 | 0.1130 |
| 1st-Der | 5/22/- | 0.9545 | 0.1131 | 0.9516 | 0.1175 | |
| MC-UVE-LS-SVM | Raw | -/22/(143.8, 4.2) | 0.9968 | 0.0306 | 0.9840 | 0.0715 |
| 1st-Der | -/22/(56.8, 19.0) | 0.9962 | 0.0336 | 0.9832 | 0.0736 | |
| RF-MLR | Raw | -/22/- | 0.9771 | 0.0807 | 0.9632 | 0.1046 |
| 1st-Der | -/26/- | 0.9872 | 0.0604 | 0.9634 | 0.1038 | |
| RF-PLS | Raw | 5/22/- | 0.9582 | 0.1085 | 0.9569 | 0.1109 |
| 1st-Der | 6/26- | 0.9759 | 0.0828 | 0.9679 | 0.0960 | |
| RF-LS-SVM | Raw | -/26/(9.9×104,110.3) | 0.9903 | 0.0528 | 0.9889 | 0.0569 |
| 1st-Der | -/26/(4.9×104, 7.5×103) | 0.9895 | 0.0549 | 0.9730 | 0.0891 | |
Fig. 3Reference vs. predicted values of aspartic acid by SPA-LS-SVM (Raw) in prediction set (The solid line is regression line and the dash line is the target 45 degree line).