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Transcript of Identification of western Canadian wheat classes at different moisture levels using near-infrared...
Identification of western Canadian wheat classes at
different moisture levels using near-infrared (NIR) hyperspectral imaging
S. Mahesh, D.S. Jayas, J. Paliwal, and N.D.G. WhiteCSBE Annual Meeting 2008
Outline Introduction Objectives Materials and Methods Results and Discussion Conclusions and Future work Acknowledgements
Introduction Wheat production = 26.7 Mt and
export = 14.0 Mt in Canada in 2005 (FAO statistics)
Eight major wheat classes in western Canada:Canada western red spring (CWRS)Canada western hard white spring (CWHWS)Canada western amber durum (CWAD)Canada western soft white spring (CWSWS)Canada western red winter (CWRW)Canada western extra strong (CWES)Canada prairie spring white (CPSW)Canada prairie spring red (CPSR)
Introduction Wheat harvesting – 13 to 15% m.c. (normally
15% m.c.) – drying – storage
Wheat @ 12 to 13% m.c.- safe moisture for effective storage- prevention of spoilage by fungi- sprouting before processing can be prevented
Wheat class identification – Major task in grain handling facilities
Visual method (common method)- to identify different wheat classes - but not to identify their moisture levels
Machine vision, PAGE, and HPLC methods
Introduction Near infrared (NIR) hyperspectral imaging
- Machine vision + NIR spectroscopy
- to develop a rapid and consistent method- Non destructive, non subjective method- Food science, Chemistry, Pharmaceuticals, Animal
science- Grain storage: wheat class identification, moisture
identification, protein and oil content determination in wheat
Objectives To identify western Canadian wheat classes at
different moisture levels by developing statistical classification models
Materials and Methods Hyperspectral imaging system
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1. Bulk wheat sample, 2. Liquid crystal tunable filter (LCTF), 3. Lens, 4. NIR camera, 5. Copy stand, 6. Illumination, and 7. Data processing system.
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Methods and Materials Wheat classes: CWRS, CWSWS, CWHWS, CWRW,
and CWES
Moisture levels: 12, 14, 16, 18, and 20%
100 images/class/m.c. – 960 to 1700 nm – 10 nm interval
Methods and Materials Relative reflectance intensity, R = ([S-D]/[W-D]
where: R = relative reflectance intensity of each slice of the NIR
hyperspectral image of wheat; S = reflectance intensity of each slice of the NIR
hyperspectral image; D = reflectance intensity of the dark current; W = reflectance intensity of a 99% reflectance standard white panel
Linear and quadratic discriminant analyses: statistical classification models
Results Linear discriminant analysis
9598
9396
100
94
83
89
969495
93
8892
100
75
81
87
99
94
58
65
98100
91
0
20
40
60
80
100
CWES CWHWS CWRS CWRW CWSWS
Cla
ssif
icat
ion
acc
ura
cy (
%)
12% 14% 16% 18% 20%
Results Quadratic discriminant analysis
70
57
74
8082
75 74 73
59
89
72
6165
83 84
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78
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89
0
20
40
60
80
100
CWES CWHWS CWRS CWRW CWSWS
Cla
ssif
icat
ion
acc
ura
cy (
%)
12% 14% 16% 18% 20%
Results Top 10 wavelengths in wheat class identification
No. Wavelength (nm) Partial R2 ASCC
1 1310 0.66 0.032 1450 0.80 0.063 1060 0.76 0.094 1700 0.72 0.125 1330 0.55 0.136 1200 0.33 0.147 1160 0.33 0.158 1090 0.29 0.169 1490 0.28 0.1610 1070 0.26 0.18
ASCC = Average squared canonical correlation
Discussion Identification of waxy wheat – 1 to 10 principal
component scores as input – 42 to 71% (LDA) and 46 to 71% (QDA) (Delwiche and Graybosch 2002)
Classification of barley based on ergosterol levels - 86.6% (LDA and QDA) (Balasubramanian et al. 2006)
Mohan et al. 2005: Mean classification accuracies = 89.1% (LDA, Top 2 Ref. features), 99.1% (LDA, Top 5 Ref. features) – Cereal grains classification
Discussion 81 – 100% (LDA) and 60 – 89% (QDA) – relative
reflectance intensities – Identification of wheat classes at different moisture levels
Conclusions and future work NIR hyperspectral imaging was found useful to
identify different moisture level wheat classes with the extracted relative reflectance intensities as input for classification
This technique could be used to develop an automatic grain assessment tool
Wheat samples from different crop years and locations could be included in the sample space to improve the robustness and classification efficiency of the models
Acknowledgements Dr. Digvir S. Jayas Dr. Jitendra Paliwal Dr. Noel D.G. White