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Characterization of an Atmospheric-Pressure Argon Plasma Generated by 915 MHz Microwaves Using Optical Emission Spectroscopy

机译:915 MHz微波产生的大气压氩等离子体的发射光谱表征

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The paper presents the investigations of an atmospheric-pressure argon plasma generated at 915 MHz microwaves using the optical emission spectroscopy (OES). The 915 MHz microwave plasma was inducted and sustained in a waveguide-supplied coaxial-line-based nozzleless microwave plasma source. The aim of presented investigations was to estimate parameters of the generated plasma, that is, excitation temperature of electrons Texc, temperature of plasma gas Tg, and concentration of electrons ne. Assuming that excited levels of argon atoms are in local thermodynamic equilibrium, Boltzmann method allowed in determining the Texc temperature in the range of 8100–11000 K. The temperature of plasma gas Tg was estimated by comparing the simulated spectra of the OH radical to the measured one in LIFBASE program. The obtained Tg temperature ranged in 1200–2800 K. Using a method based on Stark broadening of the Hβ line, the concentration of electrons ne was determined in the range from 1.4 × 1015 to 1.7 × 1015 cm−3, depending on the power absorbed by the microwave plasma.
机译:本文介绍了使用光发射光谱法(OES)对在915 MHz微波下产生的大气压氩等离子体进行的研究。在波导提供的基于同轴线的无喷嘴微波等离子体源中感应并维持915 MHz微波等离子体。提出的研究的目的是估计所产生的等离子体的参数,即电子的激发温度Texc,等离子体气体的温度Tg和电子的浓度ne。假设氩原子的激发能级处于局部热力学平衡状态,则玻尔兹曼方法可以确定Texc温度在8100–11000 K范围内,通过比较OH自由基的模拟光谱和实测温度来估算等离子体气体Tg的温度。 LIFBASE程序中的一个。所获得的Tg温度范围为1200–2800.K,使用基于Hβ线的斯塔克加宽的方法,根据吸收的功率确定电子ne的浓度范围为1.4×1015至1.7×1015 cm-3通过微波等离子体。

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