| Literature DB >> 30213127 |
Yingzhong Zhang1, Liangbo Zhang2, Jing Wang3, Xuxiao Tang4, Hong Wu5, Minghuai Wang6, Wu Zeng7, Qihui Mo8, Yongquan Li9, Jianwei Li10, Yijuan Huang11, Baohua Xu12, Mengyu Zhang13.
Abstract
A fast and effective determination method of different species of vegetable seeds oil is vital in the plant oil industry. The near-infrared reflectance spectroscopy (NIRS) method was developed in this study to analyze the oil and moisture contents of Camelliagauchowensis Chang and C.semiserrata Chi seeds kernels. Calibration and validation models were established using principal component analysis (PCA) and partial least squares (PLS) regression methods. In the prediction models of NIRS, the levels of accuracy obtained were sufficient for C.gauchowensis Chang and C.semiserrata Chi, the correlation coefficients of which for oil were 0.98 and 0.95, respectively, and those for moisture were 0.92 and 0.89, respectively. The near infrared spectrum of crush seeds kernels was more precise compared to intact kernels. Based on the calibration models of the two Camellia species, the NIRS predictive oil contents of C.gauchowensis Chang and C.semiserrata Chi seeds kernels were 48.71 ± 8.94% and 58.37 ± 7.39%, and the NIRS predictive moisture contents were 4.39 ± 1.08% and 3.49 ± 0.71%, respectively. The NIRS technique could determine successfully the oil and moisture contents of C.gauchowensis Chang and C.semiserrata Chi seeds kernels.Entities:
Keywords: Camellia seeds kernel; moisture content; near infrared reflectance spectroscopy; oil content
Mesh:
Substances:
Year: 2018 PMID: 30213127 PMCID: PMC6225329 DOI: 10.3390/molecules23092332
Source DB: PubMed Journal: Molecules ISSN: 1420-3049 Impact factor: 4.411
Figure 1Near infrared spectrogram comparison of Camellia gauchowensis Chang seeds kernels between: (A) non-destruction; and (B) comminution. 110 C. gauchowensis Chang samples represeneted 110 color lines, the same as C. semiserrata Chi seeds kernels (Figure not shown).
Calibration and validation statics in NIRS models for the estimation of oil and moisture contents of C. gauchowensis Chang and C. semiserrata Chi kernels used in sets (n = 110).
| Indicators | Seeds Kernels | Number | Statistics | Max 1/% | Min 2/% | Mean ± SD 3/% | CV 4 |
|---|---|---|---|---|---|---|---|
| Oil | 106 | Calibration set | 68.43 | 23.85 | 48.71 ± 8.94 | 0.18 | |
| Validation set | 56.82 | 22.16 | 45.32 ± 7.57 | 0.17 | |||
| 104 | Calibration set | 71.08 | 31.71 | 58.37 ± 7.39 | 0.13 | ||
| Validation set | 70.00 | 51.71 | 62.73 ± 4.38 | 0.07 | |||
| Moisture | 106 | Calibration set | 9.02 | 2.40 | 4.39 ± 1.08 | 0.25 | |
| Validation set | 9.00 | 2.74 | 4.62 ± 0.84 | 0.18 | |||
| 104 | Calibration set | 6.37 | 2.32 | 3.49 ± 0.71 | 0.20 | ||
| Validation set | 5.14 | 0.71 | 3.19 ± 0.84 | 0.26 |
Note: 1 Max, Maximum; 2 Min, Minimum; 3 SD, standard deviation; 4 CV, coefficient of variation.
Calibration and validation model parameters of oil and moisture contents by NIRS.
| Indicators | Seeds Kernels | Rc 1 | SEC 2 | SEP 3 | Offset | Bias | Slop | RPD 4 |
|---|---|---|---|---|---|---|---|---|
| Oil | 0.98 | 1.57 | 1.73 | 1.59 | 1.99 × 10−6 | 0.97 | 5.94 | |
| 0.95 | 1.72 | 1.92 | 5.26 | 1.26 × 10−6 | 0.91 | 4.92 | ||
| Moisture | 0.92 | 0.26 | 0.29 | 0.61 | 2.21 × 10−7 | 0.86 | 4.22 | |
| 0.89 | 0.27 | 0.30 | 0.70 | 4.87 × 10−8 | 0.80 | 2.77 |
Note: 1 Rc, Correlation coefficients of calibration; 2 SEC, Standard error of calibration; 3 SEP, Standard error of prediction; 4 RPD, Ratio of performance to deviation (Standard deviation/SEP).
Figure 2NIRS kernels oil content analysis of: Camellia gauchowensis Chang (A,B); and C. semiserrata Chi (C,D).
Figure 3Scatter plots of measured versus predicted oil content of kernels for the PLS models by NIRS: (A) Camellia gauchowensis Chang; and (B) C. semiserrata Chi.
Figure 4NIRS analysis kernel moisture content of: Camellia gauchowensis Chang (A,B); and C. semiserrata Chi (C,D).
Figure 5Scatter plots of measured versus predicted moisture content of: (A) Camellia gauchowensis Chang; and (B) C. semiserrata Chi kernels for the PLS models by NIRS.