首页> 外文期刊>Spectrochimica Acta, Part B. Atomic Spectroscopy >Study on the influence of X-ray tube spectral distribution on the analysis of bulk samples and thin films: Fundamental parameters method and theoretical coefficient algorithms
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Study on the influence of X-ray tube spectral distribution on the analysis of bulk samples and thin films: Fundamental parameters method and theoretical coefficient algorithms

机译:X射线管光谱分布对大块样品和薄膜分析的影响:基本参数法和理论系数算法

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摘要

Knowledge of X-ray tube spectral distribution is necessary in theoretical methods of matrix correction, i.e. in both fundamental parameter (FP) methods and theoretical influence coefficient algorithms. Thus, the influence of X-ray tube distribution on the accuracy of the analysis of thin films and bulk samples is presented. The calculations are performed using experimental X-ray tube spectra taken from the literature and theoretical X-ray tube spectra evaluated by three different algorithms proposed by Pella et al. (X-Ray Spectrom. 14 (1985) 125-135), Ebel (X-Ray Spectrom. 28 (1999) 255-266), and Finkelshtein and Pavlova (X-Ray Spectrom. 28 (1999) 27-32). In this study, Fe-Cr-Ni system is selected as an example and the calculations are performed for X-ray tubes commonly applied in X-ray fluorescence analysis (XRF), i.e., Cr, Mo, Rh and W. The influence of X-ray tube spectra on FP analysis is evaluated when quantification is performed using various types of calibration samples. FP analysis of bulk samples is performed using pure-element bulk standards and multielement bulk standards similar to the analyzed material, whereas for FP analysis of thin films, the bulk and thin pure-element standards are used. For the evaluation of the influence of X-ray tube spectra on XRF analysis performed by theoretical influence coefficient methods, two algorithms for bulk samples are selected, i.e. Claisse-Quintin (Can. Spectrosc. 12 (1967) 129-134) and COLA algorithms (G.R. Lachance, Paper Presented at the International Conference on Industrial Inorganic Elemental Analysis, Metz, France, June 3,1981) and two algorithms (constant and linear coefficients) for thin films recently proposed by Sitko (X-Ray Spectrom. 37 (2008) 265-272).
机译:在矩阵校正的理论方法中,即在基本参数(FP)方法和理论影响系数算法中,必须了解X射线管光谱分布。因此,提出了X射线管分布对薄膜和大块样品分析精度的影响。使用从文献中获得的实验X射线管光谱和通过Pella等人提出的三种不同算法评估的理论X射线管光谱进行计算。 (X-Ray Spectrom.14(1985)125-135),Ebel(X-Ray Spectrom.28(1999)255-266)和Finkelshtein和Pavlova(X-Ray Spectrom.28(1999)27-32)。在本研究中,以Fe-Cr-Ni系统为例,对通常用于X射线荧光分析(XRF)的X射线管(即Cr,Mo,Rh和W)进行计算。使用各种类型的校准样品进行定量分析时,将评估FP分析中的X射线管光谱。使用与分析材料相似的纯元素散装标准品和多元素散装标准品进行散装样品的FP分析,而薄膜的FP分析则使用散装和稀薄的纯元素标样。为了评估通过理论影响系数方法执行的X射线管光谱对XRF分析的影响,选择了两种用于散装样品的算法,即Claisse-Quintin(Can.Spectrosc.12(1967)129-134)和COLA算法(GR Lachance,在国际工业无机元素分析会议上发表的论文,法国梅斯,1981年6月3日)和Sitko最近为薄膜提出的两种算法(恒定系数和线性系数)(X射线光谱37(2008年) 265-272)。

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