Atomic and molecular emissions in laser-induced breakdown spectroscopy

被引:96
作者
Parigger, Christian G. [1 ]
机构
[1] Univ Tennessee, Inst Space, Ctr Laser Applicat, Tullahoma, TN 37388 USA
关键词
Atomic spectra; Plasma diagnostics; Laser-induced optical breakdown; Molecular spectra; Intensities and shapes of molecular spectral lines and bands; ELECTRON NUMBER DENSITY; INDUCED PLASMA; TEMPERATURE-MEASUREMENTS; RESOLVED SPECTROSCOPY; HYDROGEN-ALPHA; SPECTRAL-LINES; BALMER LINES; BETA; PROFILES; AIR;
D O I
10.1016/j.sab.2012.11.012
中图分类号
O433 [光谱学];
学科分类号
0703 ; 070302 ;
摘要
This article summarizes measurements and analysis of hydrogen Balmer series atomic lines following laser-induced optical breakdown. Electron number density on the order of 1 x 10(25) m(-3) can be measured using H-alpha Stark width and shift in the analysis of breakdown plasma in 1 to 1.3 x 10(5) Pa, gaseous hydrogen. The H-beta line can be utilized for electron number density up to 7 x 10(23) m(-3). The historic significance is elaborated of accurate H-beta measurements. Electron excitation temperature is inferred utilizing Boltzmann plot techniques that include H-gamma atomic lines and further members of the Balmer series. Laser ablation of aluminum is discussed in view of limits of application of the Balmer series. H-beta and H-gamma lines show presence of molecular carbon in a 2.7 and 6.5 x 10(5) Pa, expanding methane flow. Diagnostic of such diatomic emission spectra is discussed as well. laser-induced breakdown spectroscopy historically embraces elemental analysis, or atomic spectroscopy, and to a lesser extent molecular spectroscopy. Yet occurrence of superposition spectra in the plasma decay due to recombination or due to onset of chemical reactions necessitates consideration of both atomic and molecular emissions following laser-induced optical breakdown. Molecular excitation temperature is determined using so-called modified Boltzmann plots and fitting of spectra from selected molecular transitions. The primary interest is micro-plasma characterization during the first few micro-seconds following optical breakdown, including shadowgraph visualizations. (C) 2012 Elsevier B.V. All rights reserved.
引用
收藏
页码:4 / 16
页数:13
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