Comparative study on spectral characteristics of nanosecond pulsed discharges in atmospheric He and He+2.3%H2O mixture

C. Chen, Dongyu Peng, Botong Liu, Tinglin Zhang, Muyang Qian, Feng Zhou, Rugang Wang
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Abstract

Nanosecond pulsed discharges at atmospheric pressure in a pin-to-pin electrode configuration are well reproducible in time and space, which is beneficial to fundamentals and applications of low temperature plasmas. In this experiment, the discharges in helium (He) and He with 2.3% water vapor (H2O) are driven by a series of 10 ns overvoltage pulses (~13 kV). Special attention is paid on the spectral characteristics obtained in the center of discharges by time resolved optical emission spectroscopy. It is found that in the case of helium the emission of atomic and molecular helium during the afterglow is more intense than that in the active discharge, while in the case of He+2.3%H2O mixture the helium emission is only observed during the discharge pulse and the molecular helium emission disappears. In addition, the emissions of OH(A-X) and Hα present a similar behavior that increases sharply during the falling edge of voltage pulse as the electrons cool down rapidly. The gas temperature is determined to remain low at 540 K by fitting the OH(A-X) band. A comparative study on the emission of radiative species (He, He2, OH and H) is performed between these two cases of discharges to derive their main production mechanisms. In both cases, the dominant primary ion is He+ at the onset of discharges but their charge transfer processes of He+ are quite different. Based on these experimental data and qualitative discussion on the discharge kinetics, as for the present discharge conditions, it is shown that the electron-assisted three-body recombination processes appear to be the significant sources of radiative OH and H species in high-density plasmas.
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大气 He 和 He+2.3%H2O 混合物中纳秒脉冲放电光谱特性的比较研究
在针对针的电极配置中,大气压力下的纳秒脉冲放电在时间和空间上都具有良好的可重复性,这对低温等离子体的基础研究和应用非常有益。在本实验中,氦气(He)和含有 2.3% 水蒸汽(H2O)的氦气放电由一系列 10 毫微秒过压脉冲(约 13 千伏)驱动。通过时间分辨光学发射光谱,特别关注在放电中心获得的光谱特征。研究发现,在氦的情况下,余辉中原子氦和分子氦的发射比活动放电中的发射更强烈,而在 He+2.3%H2O 混合物的情况下,只有在放电脉冲期间才能观察到氦的发射,分子氦的发射则消失了。此外,OH(A-X) 和 Hα 的发射也呈现出类似的情况,在电压脉冲下降沿,电子迅速冷却,发射急剧增加。通过拟合 OH(A-X)带,确定气体温度保持在 540 K 的低水平。对这两种放电情况下辐射物种(He、He2、OH 和 H)的发射进行了比较研究,以得出它们的主要产生机制。在这两种情况下,放电开始时的主要原生离子都是 He+,但 He+的电荷转移过程却大不相同。根据这些实验数据和对放电动力学的定性讨论,就目前的放电条件而言,电子辅助的三体重组过程似乎是高密度等离子体中辐射 OH 和 H 物种的重要来源。
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