Spectroscopic diagnostics and electric field measurements in the near-cathode region of an atmospheric pressure microplasma jet

被引:0
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作者
B. N. Sismanoglu
K. G. Grigorov
R. A. Santos
R. Caetano
M. V.O. Rezende
Y. D. Hoyer
V. W. Ribas
机构
[1] Instituto Tecnológico de Aeronáutica,Departamento de Física
[2] Institute of Electronics,undefined
[3] Bulgarian Academy of Science,undefined
[4] EMEF Carlos Chagas,undefined
[5] Av. Osvaldo Valle Cordeiro 337,undefined
[6] 03 584-000,undefined
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关键词
Optical Emission Spectroscopy; Cathode Surface; Electron Number Density; Excitation Temperature; Cathode Sheath;
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摘要
Linear Stark splitting of the H\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$_{\beta}$\end{document} Balmer line components and spatially resolved optical emission spectroscopy (OES) measurements were used to estimate the electric field gradient in the cathode sheath region (~70 μm long) of an atmospheric pressure direct current argon flow-stabilized microplasma jet. Also, plasma parameters in the negative glow region were investigated by both OES and electrical diagnostics. The microplasma jet was operated for current ranging from 10 to 110 mA. OH (A 2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}${\rm\Sigma}^+$\end{document}, v = 0 \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$\to$\end{document} X 2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}${\rm\Pi}$\end{document}, v’ = 0) rotational bands at 306.357 nm and also the Ar 603.213 nm line were used to determine the gas temperature, which ranges from 600 to 1000 K. Electron number density, ranging from 4.1 × 1014 to 8.5 × 1014 cm-3, was determined through analysis of the H\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$_{\beta}$\end{document} line. Electron excitation temperature was also measured from the ratio of two Mo lines (8500–18 000 K) and from Boltzmann-plot of Ar 4p–4s and 5p–4s transitions (11 000–13 500 K).
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页码:479 / 487
页数:8
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