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GRATING SECONDARY SPECTRAL DIAGNOSIS OF GAS TEMPERATURE OF ATMOSPHERIC PRESSURE PLASMAS JET IN HELIUM

机译:氦气中大气压力等离子体射流气体温度的二次光谱诊断

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The optical emission spectra of helium atmospheric pressure plasma jets (APPJs) are captured with the optical spectrometers system. In the obtained spectra, the primary grating spectrum is covering the whole wavelength range from 200nm to 900nm as published works. However, in wavelength range from 400nm to 900nm, the difference is that the grating secondary spectrum was overlapped with its primary grating spectrum. Meanwhile, the secondary grating spectrum own very well resolution. So, the grating secondary spectrum data of OH (A2∑+(ν'=0)→X2∏(ν"=0)) were used to calculate the gas temperature of plasmas. Moreover, the trend of the gas temperature of plasma with applied voltage was discussed. The results are helpful for understanding the property parameters of APPJ.
机译:氦大气压等离子体射流(APPJ)的发射光谱是用光谱仪系统捕获的。在已获得的光谱中,主光栅光谱覆盖了200nm至900nm的整个波长范围。但是,在从400nm到900nm的波长范围内,不同之处在于光栅的次级光谱与它的初级光栅光谱重叠。同时,次级光栅光谱具有很好的分辨率。因此,利用OH的光栅二次光谱数据(A2∑ +(ν'= 0)→X2∏(ν“ = 0))来计算等离子体的气体温度。讨论了施加电压,该结果有助于理解APPJ的性能参数。

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