Discrimination of Wheat Grain Varieties Using X-Ray Images

Author(s):  
Małgorzata Charytanowicz ◽  
Jerzy Niewczas ◽  
Piotr Kulczycki ◽  
Piotr A. Kowalski ◽  
Szymon Łukasik
Keyword(s):  
2020 ◽  
Author(s):  
Hu Zhou ◽  
William R. Whalley ◽  
Malcolm J. Hawkesford ◽  
Andrew B. Riche ◽  
Brian Atkinson ◽  
...  

Abstract BackgroundWheat spike architecture is a key determinant of multiple grain yield components and detailed examination of spike morphometric traits is beneficial to explain wheat grain yield and the effects of differing agronomy and genetics. However, quantification of spike morphometric traits has been very limited because it relies on time-consuming manual measurements. ResultsIn this study, using X-ray Computed Tomography imaging, we proposed a method to automatically and efficiently detect the 3D architecture of wheat spikes and component spikelets by clustering grains based on their Euclidean distance and relative positions. Morphometric characteristics of wheat spikelets and grains, e.g. number, size and spatial distribution along the spike can be automatically determined. Two commercial wheat cultivars, one old, Maris Widgeon, and one modern, Siskin, were studied as examples. The average grain volume of Maris Widgeon and Siskin did not differ, but Siskin had more grains per spike and therefore greater total grain volume per spike. The spike length and spikelet number were not statistically different between the two cultivars. However, Siskin had a higher spikelet density (number of spikelets per unit spike length), with more grains and greater grain volume per spikelet than Maris Widgeon. Spatial distribution analysis revealed the number of grains, the average grain volume and the total grain volume of individual spikelets varied along the spike. Siskin had more grains and greater grain volumes per spikelet from spikelet 6, but not spikelet 1-5, compared with Maris Widgeon. The distribution of average grain volume along the spike was similar for the two wheat cultivars. ConclusionThe proposed method can automatically and efficiently extract spike, spikelet and grain morphometric traits of different wheat cultivars, which can contribute to a more detailed understanding of the sink of wheat grain yield.


Plant Methods ◽  
2019 ◽  
Vol 15 (1) ◽  
Author(s):  
Thang Duong Quoc Le ◽  
Camille Alvarado ◽  
Christine Girousse ◽  
David Legland ◽  
Anne-Laure Chateigner-Boutin

Plant Methods ◽  
2021 ◽  
Vol 17 (1) ◽  
Author(s):  
Hu Zhou ◽  
Andrew B. Riche ◽  
Malcolm J. Hawkesford ◽  
William R. Whalley ◽  
Brian S. Atkinson ◽  
...  

Abstract Background Wheat spike architecture is a key determinant of multiple grain yield components and detailed examination of spike morphometric traits is beneficial to explain wheat grain yield and the effects of differing agronomy and genetics. However, quantification of spike morphometric traits has been very limited because it relies on time-consuming manual measurements. Results In this study, using X-ray Computed Tomography imaging, we proposed a method to efficiently detect the 3D architecture of wheat spikes and component spikelets by clustering grains based on their Euclidean distance and relative positions. Morphometric characteristics of wheat spikelets and grains, e.g., number, size and spatial distribution along the spike can be determined. Two commercial wheat cultivars, one old, Maris Widgeon, and one modern, Siskin, were studied as examples. The average grain volume of Maris Widgeon and Siskin did not differ, but Siskin had more grains per spike and therefore greater total grain volume per spike. The spike length and spikelet number were not statistically different between the two cultivars. However, Siskin had a higher spikelet density (number of spikelets per unit spike length), with more grains and greater grain volume per spikelet than Maris Widgeon. Spatial distribution analysis revealed the number of grains, the average grain volume and the total grain volume of individual spikelets varied along the spike. Siskin had more grains and greater grain volumes per spikelet from spikelet 6, but not spikelet 1–5, compared with Maris Widgeon. The distribution of average grain volume along the spike was similar for the two wheat cultivars. Conclusion The proposed method can efficiently extract spike, spikelet and grain morphometric traits of different wheat cultivars, which can contribute to a more detailed understanding of the sink of wheat grain yield.


2021 ◽  
Author(s):  
Hu Zhou ◽  
Andrew B. Riche ◽  
Malcolm J. Hawkesford ◽  
William R. Whalley ◽  
Brian S. Atkinson ◽  
...  

Abstract Background: Wheat spike architecture is a key determinant of multiple grain yield components and detailed examination of spike morphometric traits is beneficial to explain wheat grain yield and the effects of differing agronomy and genetics. However, quantification of spike morphometric traits has been very limited because it relies on time-consuming manual measurements. Results: In this study, using X-ray Computed Tomography imaging, we proposed a method to efficiently detect the 3D architecture of wheat spikes and component spikelets by clustering grains based on their Euclidean distance and relative positions. Morphometric characteristics of wheat spikelets and grains, e.g., number, size and spatial distribution along the spike can be determined. Two commercial wheat cultivars, one old, Maris Widgeon, and one modern, Siskin, were studied as examples. The average grain volume of Maris Widgeon and Siskin did not differ, but Siskin had more grains per spike and therefore greater total grain volume per spike. The spike length and spikelet number were not statistically different between the two cultivars. However, Siskin had a higher spikelet density (number of spikelets per unit spike length), with more grains and greater grain volume per spikelet than Maris Widgeon. Spatial distribution analysis revealed the number of grains, the average grain volume and the total grain volume of individual spikelets varied along the spike. Siskin had more grains and greater grain volumes per spikelet from spikelet 6, but not spikelet 1-5, compared with Maris Widgeon. The distribution of average grain volume along the spike was similar for the two wheat cultivars. Conclusion: The proposed method can efficiently extract spike, spikelet and grain morphometric traits of different wheat cultivars, which can contribute to a more detailed understanding of the sink of wheat grain yield.


1990 ◽  
Vol 51 (1) ◽  
pp. 27-33 ◽  
Author(s):  
Martyn W Griffiths ◽  
Andrew D E Martin ◽  
Trevor J Hocking ◽  
Steve B Reynolds

Plant Methods ◽  
2017 ◽  
Vol 13 (1) ◽  
Author(s):  
Nathan Hughes ◽  
Karen Askew ◽  
Callum P. Scotson ◽  
Kevin Williams ◽  
Colin Sauze ◽  
...  

2018 ◽  
Vol 144 ◽  
pp. 260-268 ◽  
Author(s):  
Małgorzata Charytanowicz ◽  
Piotr Kulczycki ◽  
Piotr A. Kowalski ◽  
Szymon Łukasik ◽  
Róża Czabak-Garbacz

2007 ◽  
Vol 43 (2) ◽  
pp. 142-148 ◽  
Author(s):  
Józef Fornal ◽  
Tomasz Jeliński ◽  
Jadwiga Sadowska ◽  
Stanisław Grundas ◽  
Jan Nawrot ◽  
...  

1994 ◽  
Vol 144 ◽  
pp. 275-277
Author(s):  
M. Karlický ◽  
J. C. Hénoux

AbstractUsing a new ID hybrid model of the electron bombardment in flare loops, we study not only the evolution of densities, plasma velocities and temperatures in the loop, but also the temporal and spatial evolution of hard X-ray emission. In the present paper a continuous bombardment by electrons isotropically accelerated at the top of flare loop with a power-law injection distribution function is considered. The computations include the effects of the return-current that reduces significantly the depth of the chromospheric layer which is evaporated. The present modelling is made with superthermal electron parameters corresponding to the classical resistivity regime for an input energy flux of superthermal electrons of 109erg cm−2s−1. It was found that due to the electron bombardment the two chromospheric evaporation waves are generated at both feet of the loop and they propagate up to the top, where they collide and cause temporary density and hard X-ray enhancements.


1994 ◽  
Vol 144 ◽  
pp. 1-9
Author(s):  
A. H. Gabriel

The development of the physics of the solar atmosphere during the last 50 years has been greatly influenced by the increasing capability of observations made from space. Access to images and spectra of the hotter plasma in the UV, XUV and X-ray regions provided a major advance over the few coronal forbidden lines seen in the visible and enabled the cooler chromospheric and photospheric plasma to be seen in its proper perspective, as part of a total system. In this way space observations have stimulated new and important advances, not only in space but also in ground-based observations and theoretical modelling, so that today we find a well-balanced harmony between the three techniques.


Sign in / Sign up

Export Citation Format

Share Document