Tu Xin, Yan Jian-hua, Ma Zeng-yi, Li Xiao-dong, Pan Xin-chao, Cen Ke-fa, Cheron Bruno
Institute for Thermal Power Engineering, State Key Laboratory of Clean Energy Utilization, Zhejiang University, Hangzhou 310027, China.
Guang Pu Xue Yu Guang Pu Fen Xi. 2006 Dec;26(12):2161-5.
The molecular emission spectra lines of the first negative system N2+ (B(2) sigma--> X(2) sigma ) are frequently observed in the plasma source containing nitrogen. (0-0) and (1--1) N2+ first negative system molecular bands around 391. 4 nm can be used to the measure the rotational and vibrational temperatures in a DC argon-nitrogen plasma at atmospheric pressure. The proposed method based on the comparison between this experimental emission spectrum and the computer simulated one is presented. The effect of the apparatus function, vibrational temperature and rotational temperatures on the line structure of numerical simulated spectrum is discussed. The results show that the electron temperature, rotational temperature, vibrational temperature and kinetic temperature of plasma arc are almost the same, which can be interpreted as that DC argon-nitrogen arc plasma at atmospheric pressure is in LTE under their experimental conditions.
在含氮等离子体源中经常观察到N2+(B(2)σ→X(2)σ)第一负系统的分子发射光谱线。391.4nm附近的(0-0)和(1--1) N2+第一负系统分子带可用于测量大气压下直流氩氮等离子体中的转动温度和振动温度。提出了基于该实验发射光谱与计算机模拟光谱比较的方法。讨论了仪器函数、振动温度和转动温度对数值模拟光谱线结构的影响。结果表明,等离子体电弧的电子温度、转动温度、振动温度和动力学温度几乎相同,这可以解释为大气压下直流氩氮电弧等离子体在其实验条件下处于局部热力学平衡状态。