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Evaluating the utility of mid-infrared spectral subspaces for predicting soil properties

机译:评估中红外光谱子空间用于预测土壤性质的效用

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摘要

We propose four methods for finding local subspaces in large spectral libraries. The proposed four methods include (a) cosine angle spectral matching; (b) hit quality index spectral matching; (c) self-organizing maps and (d) archetypal analysis methods. Then evaluate prediction accuracies for global and subspaces calibration models. These methods were tested on a mid-infrared spectral library containing 1907 soil samples collected from 19 different countries under the Africa Soil Information Service project. Calibration models for pH, Mehlich-3 Ca, Mehlich-3 Al, total carbon and clay soil properties were developed for the whole library and for the subspace. Root mean square error of prediction was used to evaluate predictive performance of subspace and global models. The root mean square error of prediction was computed using a one-third-holdout validation set. Effect of pretreating spectra with different methods was tested for 1st and 2nd derivative Savitzky-Golay algorithm, multiplicative scatter correction, standard normal variate and standard normal variate followed by detrending methods. In summary, the results show that global models outperformed the subspace models. We, therefore, conclude that global models are more accurate than the local models except in few cases. For instance, sand and clay root mean square error values from local models from archetypal analysis method were 50% poorer than the global models except for subspace models obtained using multiplicative scatter corrected spectra with which were 12% better. However, the subspace approach provides novel methods for discovering data pattern that may exist in large spectral libraries. (C) 2016 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).
机译:我们提出了四种在大型光谱库中查找局部子空间的方法。提出的四种方法包括:(a)余弦角频谱匹配; (b)命中质量指数频谱匹配; (c)自组织图和(d)原型分析方法。然后评估全局和子空间校准模型的预测精度。在非洲土壤信息服务项目下,这些方法在包含来自19个不同国家的1907个土壤样品的中红外光谱库中进行了测试。为整个库和子空间​​开发了pH,Mehlich-3 Ca,Mehlich-3 Al,总碳和粘土属性的校准模型。预测的均方根误差用于评估子空间和全局模型的预测性能。预测的均方根误差是使用三分之一验证集来计算的。使用一阶和二阶导数Savitzky-Golay算法,乘法散射校正,标准正态变量和标准正态变量,然后采用去趋势方法,测试了用不同方法预处理光谱的效果。总之,结果表明,全局模型优于子空间模型。因此,我们得出结论,除少数情况外,全局模型比局部模型更准确。例如,原型模型方法中局部模型的沙子和黏土均方根误差值比全局模型差50%,但使用乘积散射校正光谱获得的子空间模型要好12%。但是,子空间方法提供了新颖的方法来发现大型频谱库中可能存在的数据模式。 (C)2016作者。由Elsevier B.V.发布。这是CC BY许可下的开放获取文章(http://creativecommons.org/licenses/by/4.0/)。

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