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通过种子分析利用近红外光谱技术早期筛选木薯蜡质品种

Near-infrared spectroscopy for early selection of waxy cassava clones via seed analysis.

作者信息

Sousa Massaine Bandeira E, Filho Juraci Souza Sampaio, de Andrade Luciano Rogerio Braatz, de Oliveira Eder Jorge

机构信息

Embrapa Mandioca e Fruticultura, Cruz das Almas, Bahia, Brazil.

Universidade Federal do Recôncavo da Bahia, Cruz das Almas, Bahia, Brazil.

出版信息

Front Plant Sci. 2023 Jan 23;14:1089759. doi: 10.3389/fpls.2023.1089759. eCollection 2023.

DOI:10.3389/fpls.2023.1089759
PMID:36755702
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC9900181/
Abstract

Cassava ( Crantz) starch consists of amylopectin and amylose, with its properties determined by the proportion of these two polymers. Waxy starches contain at least 95% amylopectin. In the food industry, waxy starches are advantageous, with pastes that are more stable towards retrogradation, while high-amylose starches are used as resistant starches. This study aimed to associate near-infrared spectrophotometry (NIRS) spectra with the waxy phenotype in cassava seeds and develop an accurate classification model for indirect selection of plants. A total of 1127 F seeds were obtained from controlled crosses performed between 77 F genotypes (wild-type, _). Seeds were individually identified, and spectral data were obtained NIRS using a benchtop NIRFlex N-500 and a portable SCiO device spectrometer. Four classification models were assessed for waxy cassava genotype identification: k-nearest neighbor algorithm (KNN), C5.0 decision tree (CDT), parallel random forest (parRF), and eXtreme Gradient Boosting (XGB). Spectral data were divided between a training set (80%) and a testing set (20%). The accuracy, based on NIRFlex N-500 spectral data, ranged from 0.86 (parRF) to 0.92 (XGB). The Kappa index displayed a similar trend as the accuracy, considering the lowest value for the parRF method (0.39) and the highest value for XGB (0.71). For the SCiO device, the accuracy (0.88-0.89) was similar among the four models evaluated. However, the Kappa index was lower than that of the NIRFlex N-500, and this index ranged from 0 (parRF) to 0.16 (KNN and CDT). Therefore, despite the high accuracy these last models are incapable of correctly classifying waxy and non-waxy clones based on the SCiO device spectra. A confusion matrix was performed to demonstrate the classification model results in the testing set. For both NIRS, the models were efficient in classifying non-waxy clones, with values ranging from 96-100%. However, the NIRS differed in the potential to predict waxy genotype class. For the NIRFlex N-500, the percentage ranged from 30% (parRF) to 70% (XGB). In general, the models tended to classify waxy genotypes as non-waxy, mainly SCiO. Therefore, the use of NIRS can perform early selection of cassava seeds with a waxy phenotype.

摘要

木薯(Crantz)淀粉由支链淀粉和直链淀粉组成,其性质由这两种聚合物的比例决定。糯性淀粉至少含有95%的支链淀粉。在食品工业中,糯性淀粉具有优势,其糊化产物对回生更稳定,而高直链淀粉则用作抗性淀粉。本研究旨在将近红外分光光度法(NIRS)光谱与木薯种子的糯性表型相关联,并开发一种用于间接选择植株的准确分类模型。通过77个F基因型(野生型,_)之间进行的控制杂交获得了总共1127粒F种子。对种子进行单独识别,并使用台式NIRFlex N - 500和便携式SCiO设备光谱仪通过NIRS获取光谱数据。评估了四种用于识别木薯糯性基因型的分类模型:k近邻算法(KNN)、C5.0决策树(CDT)、并行随机森林(parRF)和极端梯度提升(XGB)。光谱数据被分为训练集(80%)和测试集(20%)。基于NIRFlex N - 500光谱数据的准确率在0.86(parRF)至0.92(XGB)之间。考虑到parRF方法的最低值(0.39)和XGB的最高值(0.71),卡帕指数呈现出与准确率相似的趋势。对于SCiO设备,在所评估的四个模型中准确率(0.88 - 0.89)相似。然而,卡帕指数低于NIRFlex N - 500,该指数范围从0(parRF)至0.16(KNN和CDT)。因此,尽管这些模型准确率较高,但基于SCiO设备光谱无法正确区分糯性和非糯性克隆。通过混淆矩阵展示了测试集中分类模型的结果。对于两种NIRS,模型在分类非糯性克隆方面效率较高,值范围为96 - 100%。然而,NIRS在预测糯性基因型类别方面的潜力有所不同。对于NIRFlex N - 500,百分比范围从30%(parRF)至70%(XGB)。总体而言,模型倾向于将糯性基因型分类为非糯性,主要是SCiO设备。因此,使用NIRS可以对具有糯性表型的木薯种子进行早期选择。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8724/9900181/26dd760b7489/fpls-14-1089759-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8724/9900181/6fc92267942a/fpls-14-1089759-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8724/9900181/f83c6e067f30/fpls-14-1089759-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8724/9900181/3199aa02aa95/fpls-14-1089759-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8724/9900181/c374e2ab3a5a/fpls-14-1089759-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8724/9900181/6594f788e82b/fpls-14-1089759-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8724/9900181/26dd760b7489/fpls-14-1089759-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8724/9900181/6fc92267942a/fpls-14-1089759-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8724/9900181/f83c6e067f30/fpls-14-1089759-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8724/9900181/3199aa02aa95/fpls-14-1089759-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8724/9900181/c374e2ab3a5a/fpls-14-1089759-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8724/9900181/6594f788e82b/fpls-14-1089759-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8724/9900181/26dd760b7489/fpls-14-1089759-g006.jpg

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