. "Study of nitrogen flowing afterglow with mercury vapor injection"@en . . . "CZ - \u010Cesk\u00E1 republika" . "nitrogen post-discharge, mercury titration, excitation energy transfer"@en . "0021-9606" . "Trunec, David" . "P(ED2.1.00/03.0086), S" . . "RIV/00216305:26310/14:PU110503" . "Kr\u010Dma, Franti\u0161ek" . . "10.1063/1.4898367" . . . "Study of nitrogen flowing afterglow with mercury vapor injection" . "RIV/00216305:26310/14:PU110503!RIV15-MSM-26310___" . . "The reaction kinetics in nitrogen flowing afterglow with mercury vapor addition was studied by optical emission spectroscopy. The DC flowing post-discharge in pure nitrogen was created in a quartz tube at the total gas pressure of 1000 Pa and discharge power of 130 W. The mercury vapors were added into the afterglow at the distance of 30 cm behind the active discharge. The optical emission spectra were measured along the flow tube. Three nitrogen spectral systems - the first positive, the second positive, and the first negative, and after the mercury vapor addition also the mercury resonance line at 254 nm in the spectrum of the second order were identified. The measurement of the spatial dependence of mercury line intensity showed very slow decay of its intensity and the decay rate did not depend on the mercury concentration. In order to explain this behavior, a kinetic model for the reaction in afterglow was developed. This model showed that the state Hg(6 3P1), which is the upper state of mercury U" . . . "141" . "9"^^ . . . "The reaction kinetics in nitrogen flowing afterglow with mercury vapor addition was studied by optical emission spectroscopy. The DC flowing post-discharge in pure nitrogen was created in a quartz tube at the total gas pressure of 1000 Pa and discharge power of 130 W. The mercury vapors were added into the afterglow at the distance of 30 cm behind the active discharge. The optical emission spectra were measured along the flow tube. Three nitrogen spectral systems - the first positive, the second positive, and the first negative, and after the mercury vapor addition also the mercury resonance line at 254 nm in the spectrum of the second order were identified. The measurement of the spatial dependence of mercury line intensity showed very slow decay of its intensity and the decay rate did not depend on the mercury concentration. In order to explain this behavior, a kinetic model for the reaction in afterglow was developed. This model showed that the state Hg(6 3P1), which is the upper state of mercury U"@en . . . "15" . "Maz\u00E1nkov\u00E1, V\u011Bra" . "26310" . . "[F8C4E609CBF0]" . . "The Journal of Chemical Physics" . "2"^^ . . "3"^^ . "48308" . "Study of nitrogen flowing afterglow with mercury vapor injection" . "Study of nitrogen flowing afterglow with mercury vapor injection"@en .