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Preliminary results of optical emission spectroscopy by line ratio method in the RF negative ion source at ASIPP

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【作者】 王艳刘智民梁立振胡纯栋

【Author】 Yan WANG;Zhimin LIU;Lizhen LIANG;Chundong HU;Institute of Plasma Physics, Chinese Academy of Sciences;University of Science and Technology of China;

【机构】 Institute of Plasma Physics, Chinese Academy of SciencesUniversity of Science and Technology of China

【摘要】 Optical emission spectroscopy(OES) using the trace rare gases of Ar and Xe have been carried out in a radio frequency(RF) driven negative ion source at Institute of Plasma Physics, Chinese Academy of Science(ASIPP), in order to determine the electron temperature and density of the hydrogen plasma.The line-ratio methods based on population models are applied to describe the radiation process of the excited state particles and establish their relations with the plasma parameters.The spectral lines from the argon and xenon excited state atoms with the wavelength of 750.4 and 828.0 nm are used to calculate the electron temperature based on the corona model.The argon ions emission lines with the wavelength of 480 and 488 nm are selected to calculate the electron density based on the collisional radiative model.OES has given the preliminary results of the electron temperature and density by varying the discharge gas pressure and RF power.According to the experimental results, the typical plasma parameters is Te ≈ 2-4 eV and ne ≈ 1 × 1017-8 × 1017 m-3 in front of plasma grid.

【Abstract】 Optical emission spectroscopy(OES) using the trace rare gases of Ar and Xe have been carried out in a radio frequency(RF) driven negative ion source at Institute of Plasma Physics, Chinese Academy of Science(ASIPP), in order to determine the electron temperature and density of the hydrogen plasma.The line-ratio methods based on population models are applied to describe the radiation process of the excited state particles and establish their relations with the plasma parameters.The spectral lines from the argon and xenon excited state atoms with the wavelength of 750.4 and 828.0 nm are used to calculate the electron temperature based on the corona model.The argon ions emission lines with the wavelength of 480 and 488 nm are selected to calculate the electron density based on the collisional radiative model.OES has given the preliminary results of the electron temperature and density by varying the discharge gas pressure and RF power.According to the experimental results, the typical plasma parameters is Te ≈ 2-4 eV and ne ≈ 1 × 1017-8 × 1017 m-3 in front of plasma grid.

【基金】 supported in part by National Natural Science Foundation of China(Nos.11505224,11575240);National Key R&D Program of China(No.2017YFE300101);the Key Program of Research and Development of Hefei Science Center,CAS(No.2016HSC-KPRD002)
  • 【文献出处】 Plasma Science and Technology ,等离子体科学和技术(英文版) , 编辑部邮箱 ,2019年04期
  • 【分类号】O657.3
  • 【下载频次】13
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