Detail publikačního výsledku
Optical Emission Spectroscopy of Nitrogen Post-Discharge with Mercury Traces
MAZÁNKOVÁ, V.; KRČMA, F.; TRUNEC, D.
Originální název
Optical Emission Spectroscopy of Nitrogen Post-Discharge with Mercury Traces
Anglický název
Optical Emission Spectroscopy of Nitrogen Post-Discharge with Mercury Traces
Druh
Abstrakt
Originální abstrakt
The DC flowing post-discharge was created in Quartz tube at the nitrogen pressure of 1000 Pa and discharge current of 100 mA. The mercury vapour was added in the flowing afterglow behind the active discharge and the optical emission spectroscopy was performed. Nitrogen 1st positive, 2nd positive and 1st negative spectral systems and mercury spectral line at 254 nm (in the spectrum of second order) were identified. The results showed dependence of mercury spectral line intensity on the decay time. The kinetic explanation of the mercury line excitation is based on the resonance energy transfer from the nitrogen metastable level N2 (X1Sigmag+, v = 19) to mercury atom. The rate coefficient of this reaction can be calculated from time dependencies of mercury spectral line intensities, but measurement uncertainty must be taken into account. The rate coefficient value was calculated to be in 10-22 m3s-1 order.
Anglický abstrakt
The DC flowing post-discharge was created in Quartz tube at the nitrogen pressure of 1000 Pa and discharge current of 100 mA. The mercury vapour was added in the flowing afterglow behind the active discharge and the optical emission spectroscopy was performed. Nitrogen 1st positive, 2nd positive and 1st negative spectral systems and mercury spectral line at 254 nm (in the spectrum of second order) were identified. The results showed dependence of mercury spectral line intensity on the decay time. The kinetic explanation of the mercury line excitation is based on the resonance energy transfer from the nitrogen metastable level N2 (X1Sigmag+, v = 19) to mercury atom. The rate coefficient of this reaction can be calculated from time dependencies of mercury spectral line intensities, but measurement uncertainty must be taken into account. The rate coefficient value was calculated to be in 10-22 m3s-1 order.
Klíčová slova
Nitrogen post-discharge, mercury titration, energy transfer rate coefficient
Klíčová slova v angličtině
Nitrogen post-discharge, mercury titration, energy transfer rate coefficient
Autoři
MAZÁNKOVÁ, V.; KRČMA, F.; TRUNEC, D.
Rok RIV
2014
Vydáno
28.04.2013
Nakladatel
Eindhoven University
Místo
Eindhoven
Kniha
10th Frontiers in Low Temperature Plasma Diagnostics – Book of Abstracts
Strany od
P1-24
Strany do
P1-24
Strany počet
1