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Enhanced x-ray resolving power achieved behind the focal circles of Cauchois spectrometers

机译:在Cauchois光谱仪的焦圈后面获得增强的X射线分辨能力

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摘要

Maintaining high resolving power is a primary challenge in hard x-ray spectroscopy of newly developed bright and transient x-ray sources such as laser-produced plasmas. To address this challenge, the line widths in x-ray spectra with energies in the 17 keV to 70 keV range were recorded by positioning the detectors on and behind the focal circles of Cauchois type transmission-crystal spectrometers. To analyze and understand the observed line widths, we developed a geometrical model that accounts for source broadening and various instrumental broadening mechanisms. The x-ray sources were laboratory Mo or W electron-bombarded anodes, and the spectra were recorded on photostimulable phosphor image plates. For these relatively small x-ray sources, it was found that when the detector was placed on or near the focal circle, the line widths were dominated by the effective spatial resolution of the detector. When the detector was positioned beyond the focal circle, the line widths were determined primarily by source-size broadening. Moreover, the separation between the spectral lines increased with distance behind the focal circle faster than the line widths, resulting in increased resolving power with distance. Contributions to line broadenings caused by the crystal thickness, crystal rocking curve width, geometrical aberrations, and natural widths of the x-ray transitions were in all cases smaller than detector and source broadening, but were significant for some spectrometer geometries. The various contributions to the line widths, calculated using simple analytical expressions, were in good agreement with the measured line widths for a variety of spectrometer and source conditions. These modeling and experimental results enable the design of hard x-ray spectrometers that are optimized for high resolving power and for the measurement of the x-ray source size from the line widths recorded behind the focal circle.
机译:在新近开发的明亮和瞬态X射线源(例如激光产生的等离子体)的硬X射线光谱学中,保持高分辨力是主要挑战。为了解决这一难题,通过将检测器放置在Cauchois型透射晶体光谱仪的焦圈上和后面,记录了能量在17 keV至70 keV范围内的X射线光谱中的线宽。为了分析和理解观察到的线宽,我们开发了一个几何模型,该模型考虑了源扩展和各种仪器扩展机制。 X射线源是实验室用Mo或W电子轰击阳极,其光谱记录在可光激发荧光粉成像板上。对于这些相对较小的X射线源,发现将检测器放置在焦距上或焦距附近时,线宽受检测器的有效空间分辨率支配。当检测器放置在焦距之外时,线宽主要取决于光源尺寸的加宽。而且,谱线之间的间隔随着在焦点圆后面的距离增加而快于线宽,从而导致随着距离的增大分辨能力。在所有情况下,由晶体厚度,晶体摇摆曲线宽度,几何像差和X射线跃迁的自然宽度引起的线展宽的贡献均小于检测器和源展宽,但对于某些光谱仪几何形状而言却很重要。使用简单的分析表达式计算得出的对线宽的各种贡献与各种光谱仪和光源条件下测得的线宽非常吻合。这些建模和实验结果使硬X射线光谱仪的设计成为可能,这些光谱仪针对高分辨能力和从焦距圈后面记录的线宽测量X射线源尺寸进行了优化。

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