LIU Yaoge (刘耀阁), HAO Yanpeng (郝艳捧), ZHENG Bin (郑彬). Temporally-Resolved Emission Spectroscopic Diagnostics of the Atmospheric Pressure Glow Discharge in Helium[J]. Plasma Science and Technology, 2013, 15(9): 896-899. DOI: 10.1088/1009-0630/15/9/12
Citation:
LIU Yaoge (刘耀阁), HAO Yanpeng (郝艳捧), ZHENG Bin (郑彬). Temporally-Resolved Emission Spectroscopic Diagnostics of the Atmospheric Pressure Glow Discharge in Helium[J]. Plasma Science and Technology, 2013, 15(9): 896-899. DOI: 10.1088/1009-0630/15/9/12
LIU Yaoge (刘耀阁), HAO Yanpeng (郝艳捧), ZHENG Bin (郑彬). Temporally-Resolved Emission Spectroscopic Diagnostics of the Atmospheric Pressure Glow Discharge in Helium[J]. Plasma Science and Technology, 2013, 15(9): 896-899. DOI: 10.1088/1009-0630/15/9/12
Citation:
LIU Yaoge (刘耀阁), HAO Yanpeng (郝艳捧), ZHENG Bin (郑彬). Temporally-Resolved Emission Spectroscopic Diagnostics of the Atmospheric Pressure Glow Discharge in Helium[J]. Plasma Science and Technology, 2013, 15(9): 896-899. DOI: 10.1088/1009-0630/15/9/12
School of Electric Power, South China University of Technology, Guangzhou 510640, China
Funds: supported by National Natural Science Foundation of China (No. 50807018), and the State Key Laboratory of Electrical Insulation and Power Equipment (EIPE 12203)
Temporally-resolved spectroscopic diagnostics of dielectric barrier discharges (DBDs) in atmospheric-pressure helium was carried out to study the discharge mechanism. Using an intensified charge-coupled device (ICCD) and a grating spectrometer, we obtained the emission spectra of homogeneous discharges and presented them in 3D graphs. We also studied the time variation of typical emissions from He, O and first negative bands of N +2 . The results showed that the spectral lines do not develop synchronously as N +2 (B2 Σ u +X 2 Σ +g , 0∼0, λ=391.4 nm) and N +2 (B 2 Σ +u → X 2Σ +g, 0∼1, λ=427.8 nm) appear earlier and last for a longer time than He (3 3 S 1 → 2 3 P 1, λ=706.5 nm) and O (3 5 P→3 5 S, λ=777.4 nm). A certain number of He metastables produced in the initial stage of discharge. Even between adjacent pulses, the emissions from N +2 can still keep certain intensities while those from He and O extinguish. Since long-lifetime He metastables are produced and exist in the discharging space, it is the Penning ionization that keeps the long decay of N +2 emissions.