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NEW CORRECTION PROCEDURE FOR X-RAY SPECTROSCOPIC FLUORESCENCE DATA: SIMULATIONS AND EXPERIMENT

机译:X射线光谱荧光数据的新校正程序:模拟和实验

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摘要

X-ray fluorescence spectroscopy is a widely used method for determining the electronicrnconfiguration and local structure of dilute species with high sensitivity. In the dilute limit, andrnfor thin films, the X-ray fluorescence signal is directly proportional to the atomic sub-shellrnabsorption coefficient. However, for concentrated samples, the well-documented self-absorptionrneffect often leads to the severe suppression of XANES (X-ray Absorption Near-Edge Structure)rnand EXAFS (Extended X-ray Absorption Fine-Structure) amplitudes. Thus to recover the realrnvalue of the sub-shell absorption coefficient, it is important to apply correction procedures to thernmeasured fluorescence spectra. In this paper, we describe a new straightforward method torncorrect for self-absorption effects (the difference in the measured fluorescence signal comparedrnto that of the true sub-shell photoabsorption coefficient) in XANES and EXAFS fluorescencernmeasurements. Using a variety of sample and detector configurations, this method is used tornextract the sub-shell absorption coefficient on elemental nickel and thick single-crystals ofrnGd_3Ga_5O_(12) and LaAlO_3.
机译:X射线荧光光谱法是一种用于高灵敏度确定稀物质的电子构型和局部结构的广泛使用的方法。在稀薄薄膜中,X射线荧光信号与原子亚壳吸收系数成正比。但是,对于浓缩样品,有据可查的自吸收效应通常会严重抑制XANES(X射线吸收近边缘结构)rn和EXAFS(扩展X射线吸收精细结构)振幅。因此,要恢复亚壳吸收系数的实数值,对测得的荧光光谱应用校正程序很重要。在本文中,我们描述了一种校正XANES和EXAFS荧光测量中的自吸收效应(所测得的荧光信号与真正的子壳光吸收系数相比所产生的荧光信号的差异)的直接校正方法。使用各种样品和检测器配置,此方法用于提取元素镍和rnGd_3Ga_5O_(12)和LaAlO_3的厚单晶上的亚壳吸收系数。

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  • 来源
    《》|2004年|p.266-273|共8页
  • 会议地点 Steamboat SpringsCO(US);Steamboat SpringsCO(US)
  • 作者单位

    Brookhaven National Laboratory, National Synchrotron Light Source, NY, 11973;

    rnNational Institute of Standards and Technology, Gaithersburg, MD, 20899;

    rnBrookhaven National Laboratory, National Synchrotron Light Source, NY, 11973;

  • 会议组织
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 仪器分析法(物理及物理化学分析法);
  • 关键词

  • 入库时间 2022-08-26 13:46:28

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