Spectroscopic diagnostic of helium-hydrogen RF plasma under the influence of radiation trapping

被引:0
作者
Sawada K. [1 ]
Goto M. [2 ]
Ezumi N. [3 ]
机构
[1] Faculty of Engineering, Shinshu University, Nagano 380-8553
[2] National Institute for Fusion Science, Toki 509-5292
[3] Nagano National College of Technology, Nagano 381-8550
基金
日本学术振兴会;
关键词
Collisional-radiative model; Helium-hydrogen plasma; Radiation trapping; Spectroscopic diagnostic;
D O I
10.1585/pfr.6.1401010
中图分类号
学科分类号
摘要
The electron temperature and density, atomic hydrogen density and temperature in a helium-hydrogen RF plasma are determined from the visible emission line intensities of both atoms by considering photoexcitation from the ground state accompanied by radiation trapping in the plasma. From the observed helium line intensity, and the hydrogen Balmer γ line intensity which is little affected by photoexcitation, parameters other than the atomic hydrogen temperature are determined using a helium atom collisional-radiative model [Sawada et al., Plasma Fusion Res. 5, 001 (2010)], which includes photoexcitation for helium singlet P states, and a hydrogen atom collisional-radiative model in which photoexcitation is ignored. The atomic hydrogen temperature is determined to reproduce the Balmer α and β line intensities by using an iterative hydrogen atom collisional-radiative model [Sawada, J. Plasma Phys. 72, 1025 (2006)] that calculates the photoexcitation rates. © 2011 The Japan Society of Plasma Science and Nuclear Fusion Research.
引用
收藏
相关论文
共 22 条
[1]  
Sawada K., J. Plasma Phys., 72, (2006)
[2]  
Sawada K., Yamada Y., Miyachika T., Ezumi N., Iwamae A., Goto M., Plasma Fusion Res., 5, (2010)
[3]  
Fujimoto T., Plasma Spectroscopy, (2004)
[4]  
Fujimoto T., JQSRT, 21, (1978)
[5]  
Goto M., JQSRT, 76, (2003)
[6]  
Goto M., Morita S., Sawada K., Fujimoto T., Yamamoto S., Phys. Plasmas, 10, (2003)
[7]  
Fursa D.V., Bray I., Phys. Rev. A, 52, (1995)
[8]  
Bray I., Fursa D.V., J. Phys. B, 28, (1995)
[9]  
Fursa D.V., Bray I., J. Phys. B, 30, (1997)
[10]  
Bartschat K., J. Phys. B, 31, (1998)