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TEMPORAL CHARACTERISTICS OF EMISSION SPECTRUM IN ATMOSPHERIC-PRESSURE HELIUM PLASMA

机译:大气压氦等离子体中发射光谱的时间特性

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Optical emission spectrum of discharges under different background air pressure was obtained using an intensified charge-coupled device (ICCD) and a grating spectrometer. Besides, spectral lines of N2+ (B2∑u+→ X2∑u+, 0-0, λ=391.4nm), N2+ (B2∑u+ → X2 ∑u+, 0-1, λ=427.8nm), He (33S1→23P1,λ=706.5nm) and O (35P→35S,λ=777.4nm) were selected to study their time variation. The results showed that under 4.0 Pa background air pressure, He (33S1→23P1, λ=706.5nm) appears earliest, while in the case of under 20 Pa background air pressure, all lines almost show up at the same time. Besides, He (33S1→23P1, λ= 706.5nm) dies out immediately while other lines keep certain intensities after the current pulse. This is attributed to the concentration of metastables and the occurrence probability of Penning ionization. Because of the metastables, Penning ionization is processing and spectral lines of N2+ and O can be detected even after the extinction of discharge.
机译:使用增强型电荷耦合器件(ICCD)和光栅光谱仪获得了在不同背景气压下放电的光发射光谱。此外,N2 +(B2∑u +→X2∑u +,0-0,λ= 391.4nm),N2 +(B2∑u +→X2 ∑u +,0-1,λ= 427.8nm),He(33S1→23P1)的谱线(λ= 706.5nm)和O(35P→35S,λ= 777.4nm)来研究它们的时间变化。结果表明,在4.0 Pa背景气压下,He(33S1→23P1,λ= 706.5nm)最早出现,而在20 Pa背景气压下,所有线条几乎同时出现。此外,He(33S1→23P1,λ= 706.5nm)立即消失,其他线在电流脉冲后仍保持一定强度。这归因于亚稳态的浓度和潘宁电离的发生概率。由于亚稳态,潘宁电离正在处理中,即使在放电消失后也可以检测到N2 +和O的光谱线。

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