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等离子体气体和压力对激光诱导等离子体发射光谱中铜发射线时空分辨图像的影响

Effect of Plasma Gas and the Pressure on Spatially and Temporally Resolved Images of Copper Emission Lines in Laser Induced Plasma Optical Emission Spectrometry.

作者信息

Weng Julian, Kashiwakura Shunsuke, Wagatsuma Kazuaki

机构信息

Institute for Materials Research, Tohoku University.

出版信息

Anal Sci. 2021 Feb 10;37(2):367-375. doi: 10.2116/analsci.20P203. Epub 2020 Oct 23.

Abstract

This paper investigated two-dimensional spatial and temporal images of a copper emission line in laser-induced breakdown spectroscopy (LIBS), in order to clarify the excitation/de-excitation processes occurring in a laser-induced plasma. The measurements were carried out under different plasma gases (argon, krypton, helium, and nitrogen), pressure levels (100 - 900 Pa) and delay times (100 - 1000 ns) with the aim of monitoring their effects on the behavior of the copper emission. Depending on the plasma gas type and the pressure level, large differences were found in the plasma shape and temporal intensity evolution of the copper emission profile. Namely, krypton produced the most compact plasma emitting larger intensities, compared to argon and helium, and an increase in the gas pressure made these plasmas to shrink, which could be related principally to the stopping power of the applied gases. Through temporally resolved analysis, the delay profiles could be obtained for each plasma gas, indicating that the helium plasma disappeared more rapidly than the argon and krypton plasmas. It was suggested that the variations in the emission intensity would be determined by interactions between gas particles and highly energetic particles in the plasma breakdown as well as interactions between excited gas particles and copper species during plasma expansion. These insights could prove to be useful in the understanding of the background of LIBS as well as the optimization of its practical applications.

摘要

本文研究了激光诱导击穿光谱(LIBS)中铜发射线的二维空间和时间图像,以阐明激光诱导等离子体中发生的激发/去激发过程。测量是在不同的等离子体气体(氩气、氪气、氦气和氮气)、压力水平(100 - 900 Pa)和延迟时间(100 - 1000 ns)下进行的,目的是监测它们对铜发射行为的影响。根据等离子体气体类型和压力水平,发现铜发射轮廓的等离子体形状和时间强度演变存在很大差异。具体而言,与氩气和氦气相比,氪气产生的等离子体最紧凑,发射强度更大,并且气体压力的增加使这些等离子体收缩这主要可能与所施加气体的阻止本领有关。通过时间分辨分析,可以获得每种等离子体气体的延迟轮廓,表明氦等离子体比氩等离子体和氪等离子体消失得更快。有人认为,发射强度的变化将由等离子体击穿过程中气体粒子与高能粒子之间的相互作用以及等离子体膨胀过程中激发的气体粒子与铜物种之间的相互作用决定。这些见解可能有助于理解LIBS的背景及其实际应用的优化。

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