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Statements

Subject Item
n2:RIV%2F00216305%3A26310%2F14%3APU110503%21RIV15-MSM-26310___
rdf:type
skos:Concept n10:Vysledek
dcterms:description
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 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
dcterms:title
Study of nitrogen flowing afterglow with mercury vapor injection Study of nitrogen flowing afterglow with mercury vapor injection
skos:prefLabel
Study of nitrogen flowing afterglow with mercury vapor injection Study of nitrogen flowing afterglow with mercury vapor injection
skos:notation
RIV/00216305:26310/14:PU110503!RIV15-MSM-26310___
n3:aktivita
n15:S n15:P
n3:aktivity
P(ED2.1.00/03.0086), S
n3:cisloPeriodika
15
n3:dodaniDat
n9:2015
n3:domaciTvurceVysledku
n7:7469985 n7:2888165
n3:druhVysledku
n16:J
n3:duvernostUdaju
n19:S
n3:entitaPredkladatele
n14:predkladatel
n3:idSjednocenehoVysledku
48308
n3:idVysledku
RIV/00216305:26310/14:PU110503
n3:jazykVysledku
n12:eng
n3:klicovaSlova
nitrogen post-discharge, mercury titration, excitation energy transfer
n3:klicoveSlovo
n13:nitrogen%20post-discharge n13:mercury%20titration n13:excitation%20energy%20transfer
n3:kodStatuVydavatele
CZ - Česká republika
n3:kontrolniKodProRIV
[F8C4E609CBF0]
n3:nazevZdroje
The Journal of Chemical Physics
n3:obor
n18:BL
n3:pocetDomacichTvurcuVysledku
2
n3:pocetTvurcuVysledku
3
n3:projekt
n4:ED2.1.00%2F03.0086
n3:rokUplatneniVysledku
n9:2014
n3:svazekPeriodika
141
n3:tvurceVysledku
Trunec, David Krčma, František Mazánková, Věra
s:issn
0021-9606
s:numberOfPages
9
n11:doi
10.1063/1.4898367
n17:organizacniJednotka
26310