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A passive method for determining plasma dissociation degree using vacuum UV self-absorption spectroscopy

机译:一种使用真空UV自吸收光谱法测定血浆解离程度的无源方法

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There has been a continued interest in utilizing streamer and spark discharges for new technologies that require low temperature plasma generation at atmospheric pressure, but diagnostics of these plasmas typically require external sources of probing radiation such as UV lamps or laser systems. Specifically, it is desired to measure the dissociated gas density from pulsed surface flashover plasmas, without the use of potentially invasive optical techniques such as two-photon absorption laser induced fluorescence (TALIF) spectroscopy, which may artificially increase the dissociation degree. We demonstrate a method for determining the dissociated gas density of N and H atoms in an N2/H2 surface flashover plasma by passively monitoring the self-absorption of intrinsic radiation produced by the 2s2 2p2 3s→2s2 2p3 NI transition(s) at 120.0 nm, and the 2p→ls HI Lyman-a transition at 121.57 nm. This radiation is partially trapped by the spark plasma, assumed to be of Gaussian cylindrical shape with 500 μπι diameter. The resulting emission line shapes can be calculated by inferring the plasma temperature, gas mixture, and the estimated dissociated atom density of each species in the plasma volume of measurement. For example, 80%/20% N2/H2 discharges with a measured electron temperature of ∼3.0 eV produce peak dissociated concentrations of 2% and 9% for atomic N and H, respectively, during the spark phase ∼100 ns after voltage collapse. By assuming the quasi-contiguous approximation of the Holtsmark micro-field due to local electron perturbation of the HI radiators, the Stark line width of Lyman-a radiation yields electron densities on the order of 1018 cm3 during the spark phase. This self-absorption method has been extended to provide density information of surface flashover plasmas in air environments by pas- ively monitoring the 2s2 2p3 3s→2s2 2p4 OI transitions) at 130.2 nm / 130.5 nm / 130.6 nm, which yield peak dissociated concentrations of 20% and 7% for atomic O and N, respectively.
机译:对于在大气压力下需要低温等离子体产生的新技术,对新技术进行了持续的兴趣,但这些等离子体的诊断通常需要探测辐射等外部来源,例如UV灯或激光系统。具体地,希望从脉冲表面闪络等离子体中测量离子气体密度,而不使用诸如双光子吸收激光诱导的荧光(TALIF)光谱的潜在侵入性光学技术,其可以人为地增加解离程度。通过被动监测所产生的内在辐射的自吸收的自吸收,通过被动监测所产生的内在辐射的自吸收,确定在N 2-/ IM> / H 2 表面闪络等离子体中的解离气体密度的方法通过2S 2 2p 2 3 s→2s 2 2p 3 ni过渡,在120.0 nm, 2P→LS Hi Lyman-A转换为121.57 nm。该辐射被火花等离子体部分捕获,假设具有500μm直径的高斯圆柱形。通过推断等离子体温度,气体混合物和估计的每种物种的测量体积的估计的离解原子密度可以计算得到的发射线形状。例如,80%/ 20%N 2 / H 2 测量的电子温度为〜3.0eV的测量,产生2%和9%的峰值离解浓度为原子n分别在电压崩溃后的火花阶段~100ns期间分别。通过假设HOLTSMAW微场的准连续近似由于HI辐射器的局部电子扰动,Lyman-A辐射的STARK线宽产生10 18 CM 3 。这种自吸收方法已经扩展到通过对2S 2 2 3 3s→2s 2来提供空气环境中表面闪极等离子体的密度信息。 2p 4 oi转变),在130.2nm / 130.5nm / 130.6nm,其分别产生20%和7%的峰分离浓度,用于原子O和n。

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