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Temperature and absolute oh density measurement by the relative emission spectroscopy in diffuse atmospheric-pressure RF glow discharges

机译:通过相对发射光谱在弥漫性大气压RF发光放电中的相对发射光谱法测量温度和绝对OH密度测量

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Summary form only given. In recent years, the measurement of absolute densities of reactive species and radicals such as OH is of growing interest for many plasma applications. Many complex techniques, including laser-induced fluorescence (LIF), cavity ring-down spectroscopy, resonant absorption and broadband absorption, have been used to measure absolute OH density. However, the optical emission spectroscopy (OES) has the natural advantage of being non-intrusive, inexpensive, and easy to implement, in comparison with the abovementioned methods.In this contribution, we will extend the use of a selfabsorption model for atomic emission spectroscopy1, 2 to molecular emission spectroscopy, in particular OH(A-X). We propose to analyze the self-absorption effect on rotational lines in the emission spectra of OH(A-X) for the simultaneous measurement of gas temperature and OH(X) density. We apply the model on emission spectra recorded from a 10 cm homogeneous and diffuse glow discharge which is optically thick for the OH(A-X) emission. The effect of gas temperature, rotational temperatures, and spectral resolution of the spectrometer is assessed. The outcomes are compared in detail with OH densities measured by broadband absorption and gas temperatures by OES of N2(C-B) to validate the proposed method. The detection limit of the line integrated OH(X) density with this method is of the order of 2 × 1019 m-2. The accuracy of the density is sensitive to the rotational temperature of the OH(A) state and the nonequilibrium rotational population distribution. The proposed analysis of self-absorbed optical emission spectra is a simple and inexpensive method to determine OH densities, in large volume plasmas although it requires a high-resolution spectrometer.
机译:摘要表格仅给出。近年来,对许多等离子体应用的反应性物种和基团的绝对密度的测量对于越来越感兴趣。许多复杂的技术,包括激光诱导的荧光(LiF),腔循环光谱,谐振吸收和宽带吸收,用于测量绝对OH密度。然而,与上述方法相比,光发射光谱(OES)具有非侵入性,廉价且易于实现的自然优势。在这种贡献中,我们将扩展用于原子发射光谱1的自主吸化模型的使用,2至分子发射光谱,特别是OH(AX)。我们建议分析OH(A-X)发射光谱中的旋转线的自吸收效应,用于同时测量气体温度和OH(X)密度。我们在从10厘米均匀的和漫射辉光放电记录的发射光谱上应用模型,该发射光谱放电是OH(A-X)发射的光学厚。评估气体温度,旋转温度和光谱仪的光谱分辨率的影响。通过N 2(C-B)的宽带吸收和气体温度测量的OH密度将结果详细比较,以验证所提出的方法。通过该方法的线路集成OH(x)密度的检测限为2×1019 m-2的顺序。密度的准确性对OH(a)状态的旋转温度和非Quigibirim旋转人口分布敏感。所提出的自吸光发射光谱分析是一种简单且廉价的方法,用于确定大体积等离子体中的oh密度,尽管它需要高分辨率光谱仪。

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