Excitation of Mercury Atoms in Nitrogen Post-Discharge

dc.contributor.authorKrčma, Františekcs
dc.contributor.authorBocková, Ivanacs
dc.contributor.authorMazánková, Věracs
dc.contributor.authorSoural, Ivocs
dc.contributor.authorHrdlička, Alešcs
dc.contributor.authorKanický, Viktorcs
dc.coverage.issue1cs
dc.coverage.volume516cs
dc.date.issued2014-06-03cs
dc.description.abstractThe work presents results obtained during spectroscopic observations of nitrogen DC flowing post-discharges at the total gas pressure of 1000 Pa and at the discharge current of 100 mA. Mercury traces were introduced into the system using auxiliary pure nitrogen flow enriched by mercury vapor. A very low mercury concentration of 3.7 ppb was introduced into the system before the active discharge. The strong quenching of nitrogen pink afterglow was observed but no mercury lines were recorded. Moreover, the vibrational distributions of nitrogen excited states were nearly unchanged. Based on these results, the new experimental set up was created. The introduction point of mercury vapor with higher concentration of 600 ppm was movable during the post discharge up to decay time of 40 ms. Besides three nitrogen spectral systems (first and second positive and first negative), NO-beta and NO-gamma bands, the mercury line at 254 nm was recorded at these conditions. Its intensity was dependent on the mercury vapor introduction position as well as on the mercury concentration. No other mercury lines were observed. The creation of mercury 3P1 state that is the upper state of the observed mercury spectral line is possible by the resonance excitation energy transfer form vibrationally excited nitrogen ground state N2 (X, v = 19). The observed results should form a background for the development of a new titration technique used for the highly vibrationally excited nitrogen ground state molecules determination.en
dc.description.abstractThe work presents results obtained during spectroscopic observations of nitrogen DC flowing post-discharges at the total gas pressure of 1000 Pa and at the discharge current of 100 mA. Mercury traces were introduced into the system using auxiliary pure nitrogen flow enriched by mercury vapor. A very low mercury concentration of 3.7 ppb was introduced into the system before the active discharge. The strong quenching of nitrogen pink afterglow was observed but no mercury lines were recorded. Moreover, the vibrational distributions of nitrogen excited states were nearly unchanged. Based on these results, the new experimental set up was created. The introduction point of mercury vapor with higher concentration of 600 ppm was movable during the post discharge up to decay time of 40 ms. Besides three nitrogen spectral systems (first and second positive and first negative), NO-beta and NO-gamma bands, the mercury line at 254 nm was recorded at these conditions. Its intensity was dependent on the mercury vapor introduction position as well as on the mercury concentration. No other mercury lines were observed. The creation of mercury 3P1 state that is the upper state of the observed mercury spectral line is possible by the resonance excitation energy transfer form vibrationally excited nitrogen ground state N2 (X, v = 19). The observed results should form a background for the development of a new titration technique used for the highly vibrationally excited nitrogen ground state molecules determination.en
dc.formattextcs
dc.format.extent012005-012005cs
dc.format.mimetypeapplication/pdfcs
dc.identifier.citationJournal of Physics: Conference Series. 2014, vol. 516, issue 1, p. 012005-012005.en
dc.identifier.doi10.1088/1742-6596/516/1/012005cs
dc.identifier.issn1742-6596cs
dc.identifier.orcid0000-0003-4418-3323cs
dc.identifier.orcid0000-0002-4339-6020cs
dc.identifier.other50742cs
dc.identifier.urihttp://hdl.handle.net/11012/137096
dc.language.isoencs
dc.publisherIOP Publishingcs
dc.relation.ispartofJournal of Physics: Conference Seriescs
dc.relation.urihttp://iopscience.iop.org/article/10.1088/1742-6596/516/1/012005cs
dc.rightsCreative Commons Attribution 3.0 Unportedcs
dc.rights.accessopenAccesscs
dc.rights.sherpahttp://www.sherpa.ac.uk/romeo/issn/1742-6596/cs
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/cs
dc.subjectnitrogen post dischargeen
dc.subjectmercury tracesen
dc.subjectkinetic processesen
dc.subjectenergy transfer reactionsen
dc.subjectnitrogen post discharge
dc.subjectmercury traces
dc.subjectkinetic processes
dc.subjectenergy transfer reactions
dc.titleExcitation of Mercury Atoms in Nitrogen Post-Dischargeen
dc.title.alternativeExcitation of Mercury Atoms in Nitrogen Post-Dischargeen
dc.type.driverarticleen
dc.type.statusPeer-revieweden
dc.type.versionpublishedVersionen
sync.item.dbidVAV-50742en
sync.item.dbtypeVAVen
sync.item.insts2025.10.14 14:07:52en
sync.item.modts2025.10.14 10:04:35en
thesis.grantorVysoké učení technické v Brně. Fakulta chemická. Ústav fyzikální a spotřební chemiecs

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