| Literature DB >> 29881393 |
Changwei Tan1, Ying Du1, Jian Zhou1, Dunliang Wang1, Ming Luo1, Yongjian Zhang1, Wenshan Guo1.
Abstract
Hyperspectral remote sensing is a rapid non-destructive method for diagnosing nitrogen status in wheat crops. In this study, a quantitative correlation was associated with following parameters: leaf nitrogen accumulation (LNA), raw hyperspectral reflectance, first-order differential hyperspectra, and hyperspectral characteristics of wheat. In this study, integrated linear regression of LNA was obtained with raw hyperspectral reflectance (measurement wavelength = 790.4 nm). Furthermore, an exponential regression of LNA was obtained with first-order differential hyperspectra (measurement wavelength = 831.7 nm). Coefficients (R2) were 0.813 and 0.847; root mean squared errors (RMSE) were 2.02 g·m-2 and 1.72 g·m-2; and relative errors (RE) were 25.97% and 20.85%, respectively. Both the techniques were considered as optimal in the diagnoses of wheat LNA. Nevertheless, the better one was the new normalized variable (SDr - SDb)/(SDr + SDb), which was based on vegetation indices of R2 = 0.935, RMSE = 0.98, and RE = 11.25%. In addition, (SDr - SDb)/(SDr + SDb) was reliable in the application of a different cultivar or even wheat grown elsewhere. This indicated a superior fit and better performance for (SDr - SDb)/(SDr + SDb). For diagnosing LNA in wheat, the newly normalized variable (SDr - SDb)/(SDr + SDb) was more effective than the previously reported data of raw hyperspectral reflectance, first-order differential hyperspectra, and red-edge parameters.Entities:
Keywords: diagnostic model; hyperspectral remote sensing; leaf nitrogen accumulation; vegetation index; wheat
Year: 2018 PMID: 29881393 PMCID: PMC5976834 DOI: 10.3389/fpls.2018.00674
Source DB: PubMed Journal: Front Plant Sci ISSN: 1664-462X Impact factor: 5.753
Definitions of hyperspectral remote sensing parameters used in the study.
| Hyperspectral characteristic variables based on red-edge position | First-order maximal derivative inside red edge | Red edge covers 680-780 nm; | Gong et al., | |
| λr | Red edge position | λr is the wavelength with respect to | ||
| First-order maximal derivative inside blue edge | Blue edge covers 490–530 nm; | |||
| λb | Corresponding band length with | λb is the wavelength with respect to | ||
| First-order maximal derivative inside yellow edge | Yellow edge covers 550–582 nm; | |||
| λy | Corresponding band length with | λy is the wavelength with respect to | ||
| Hyperspectral reflectance at the peak of green band | ||||
| λg | Corresponding band length with | λg is the wavelength with respect to | ||
| Hyperspectral reflectance at valley of red band | ||||
| Hyperspectral characteristic variables based on red-edge area | Summation of first-order derivatives inside red edge | The sum of the values of first-order differential spectra in the red edge wavelength range | ||
| Summation of first-order derivatives inside blue edge | The sum of the values of first-order differential spectra in the blue edge wavelength range | |||
| Summation of first-order derivatives inside yellow edge | The sum of the values of first-order differential spectra in the yellow edge wavelength range | |||
| Hyperspectral characteristic variables based on vegetation indices | – | |||
| – | ||||
| – | ||||
| – | ||||
| – | ||||
| – |
Distribution of LNA in training and test datasets.
| Training set | 2016 | 144 | 17.556 | 1.52 | 7.858 | 3.742 | 0.306 |
| Test set | 2015 | 150 | 18.835 | 0.312 | 8.024 | 4.617 | 0.378 |
Figure 1Correlation coefficient between raw hyperspectral reflectance and wheat LNA (The correlation coefficient outside the two P0.05 lines was significant at 0.05 level, while the correlation coefficient outside the two P0.01 lines was significant at 0.01 level).
Figure 2Correlation coefficient between first-order hyperspectral reflectance and wheat LNA (The correlation coefficient outside the two P0.05 lines was significant at 0.05 level, while the correlation coefficient outside the two P0.01 lines was significant at 0.01 level).
Correlation coefficients between hyperspectral characteristic variables and wheat LNA (n = 144).
| −0.014 | |
| λb | 0.031 |
| −0.893 | |
| λr | 0.820 |
| 0.843 | |
| λy | −0.009 |
| −0.186 | |
| λg | −0.194 |
| −0.143 | |
| 0.911 | |
| −0.821 | |
| −0.146 | |
| −0.214 | |
| 0.201 | |
| 0.151 | |
| 0.941 | |
| 0.856 | |
| −0.137 |
P < 0.05, | r | > 0.174;
P < 0.01, | r | > 0.228. The same below.
Linear and non-linear regression analysis between hyperspectral characteristic variables and wheat LNA (n = 144).
| Linear | 23.346 | −11.372 | 0.797** | |||
| Exponential | 11.037 | −19.836 | 0.846** | |||
| Logarithm | 21.821 | −88.931 | 0.803** | |||
| Parabolic | 39.024 | −1021.93 | −1674.36 | 0.839** | ||
| Power | 6.946 | −12.877 | 0.816** | |||
| Cubic | 1121.84 | −3452.92 | 4481.62 | −109.74 | 0.819** | |
| λr | Linear | 4022.63 | 599.37 | 0.673** | ||
| Exponential | 36.933 | 301.77 | 0.686** | |||
| Logarithm | 3.936 | 9.758 | 0.611** | |||
| Parabolic | 33.811 | 2.976 | 6.938 | 0.681** | ||
| Power | 34.733 | 6.292 | 0.637** | |||
| Cubic | 41.767 | 856.091 | 46.711 | 0.649** | ||
| Linear | 22.734 | 881.463 | 0.711** | |||
| Exponential | 32.071 | 14.877 | 0.802** | |||
| Logarithm | 73.791 | 263.88 | 0.643** | |||
| Parabolic | 542.766 | 3671.65 | 3722.62 | 0.791** | ||
| Power | 7.821 | 46.943 | 0.677** | |||
| Cubic | 12.833 | 48.773 | 83.552 | −101.72 | 0.756** | |
| Linear | 553.472 | 738.822 | 0.886** | |||
| Exponential | 2116.82 | 4231.63 | 0.862** | |||
| Logarithm | 186.52 | 1863.81 | 0.872** | |||
| Parabolic | 92.573 | 7.736 | −37.282 | 0.891** | ||
| Power | 291.778 | 101.627 | 0.862** | |||
| Cubic | 57.116 | 1928.93 | −311.261 | 97.246 | 0.898** | |
| Linear | 43.623 | 13.383 | 0.733** | |||
| Exponential | 61.782 | 21.822 | 0.636** | |||
| Logarithm | 9.793 | 23.161 | 0.672** | |||
| Parabolic | 4.683 | 21.981 | −8.572 | 0.696** | ||
| Power | 28.861 | 31.173 | 0.708** | |||
| Cubic | 13.711 | 33.908 | −18.167 | 9.678 | 0.684** | |
| Linear | 11.127 | 42.657 | 0.829** | |||
| Exponential | 12.658 | 17.267 | 0.841** | |||
| Logarithm | 9.486 | 15.167 | 0.792** | |||
| Parabolic | 12.386 | 34.232 | −12.186 | 0.841** | ||
| Power | 16.563 | 15.677 | 0.687** | |||
| Cubic | 6.637 | 16.574 | −11.232 | 3.761 | 0.846** | |
| Linear | 13.346 | −11.783 | 0.674** | |||
| Exponential | 8.774 | −23.063 | 0.472** | |||
| Logarithm | 14.833 | −6.843 | 0.562** | |||
| Parabolic | 5.927 | −12.126 | −2.103 | 0.683** | ||
| Power | 3.218 | −9.253 | 0.617** | |||
| Cubic | 9.145 | −6.264 | −7.691 | 3.588 | 0.737** | |
Linear function: y = a + bx; Exponential function: y = a × exp (bx); Logarithm function: y = a + b × lnx; Parabolic function: y = a + bx + cx.
Figure 3Evaluating the diagnostic models for wheat LNA based on ρ790.4, ρ′831.7 and (SD − SD)/(SD + SD) (model based on ρ790.4: y = 1.065x + 0.09, R2 = 0.813, RMSE (g·m−2) = 2.02, RE (%) = 25.97, n = 150; model based on ρ′831.7: y = 1.069x – 0.501, R2 = 0.847, RMSE (g·m−2) = 1.72, RE (%) = 20.85, n = 150; model based on (SD − SD)/(SD + SD): y = 0.978x + 0.307, R2 = 0.935, RMSE (g·m−2) = 0.98, RE (%) = 11.25, n = 150).
Figure 4Evaluating the diagnostic model based on (SDr−SDb)/(SDr+SDb) using a different cultivar or even wheat grown elsewhere: y = 1.179x - 0.974, R2 = 0.902, RMSE (mg.g−1) = 1.46, RE(%) = 13.74, n = 120).