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铜的X射线光谱分析:一个老课题的新成果

X-Ray Spectrometry of Copper: New Results on an Old Subject.

作者信息

Deutsch M, Förster E, Hölzer G, Härtwig J, Hämäläinen K, Kao C-C, Huotari S, Diamant R

机构信息

Physics Dept., Bar-Ilan University, Ramat-Gann 52900, Israel.

Institute for Optics and Quantum Electronics, Friedrich-Schiller-University Jena, D-07743 Jena, Germany.

出版信息

J Res Natl Inst Stand Technol. 2004 Feb 1;109(1):75-98. doi: 10.6028/jres.109.006. Print 2004 Jan-Feb.

DOI:10.6028/jres.109.006
PMID:27366598
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC4849622/
Abstract

We review recent, and some less recent, measurements of several emission spectra of copper. The results are discussed with special emphasis on elucidating the structure of the Kα 1,2 and Kβ 1,3 diagram lines and their underlying transitions. These lines are found to contain ≈30 % contribution from 3d spectator hole transitions. Other multielectronic transitions, the 2p spectator hole (satellites) and 1s spectator hole (hypersatellites) transitions were also measured. They are discussed paying special attention to the evolution of the lineshapes and intensities from the excitation threshold to saturation. Trends in the measured quantities depending on the spectator hole's shell and subshell are also discussed.

摘要

我们回顾了近期以及一些稍早时期对铜的几种发射光谱的测量结果。讨论这些结果时特别强调了阐明Kα 1,2和Kβ 1,3标识谱线的结构及其潜在跃迁。发现这些谱线中约30%的贡献来自3d旁观空穴跃迁。还测量了其他多电子跃迁,即2p旁观空穴(卫星峰)和1s旁观空穴(超卫星峰)跃迁。讨论这些跃迁时特别关注了从激发阈值到饱和状态下谱线形状和强度的演变。还讨论了测量量随旁观空穴所在壳层和子壳层变化的趋势。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/ace011193853/j91deuf16.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/7c206a3f9f30/j91deuf11.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/a2c4dc404668/j91deuf15.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/2d5c92f1c409/j91deuf1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/1e529fdfe5a4/j91deuf2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/4c78d999c7ff/j91deuf3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/57c317eebd79/j91deuf4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/407e39dddad1/j91deuf5.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/b4e1a1902f3d/j91deuf6.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/188d97bb9632/j91deuf7.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/24863b6bec53/j91deuf8.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/86480b99e049/j91deuf9.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/b6a1538dd31b/j91deuf10.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/7c206a3f9f30/j91deuf11.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/baab4fea4acc/j91deuf12.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/a223d844969b/j91deuf13.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/f17b10ec3c18/j91deuf14.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/189a/4849622/ace011193853/j91deuf16.jpg

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