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Monitoring active species in an atmospheric pressure dielectric-barrier discharge: Observation of the Herman-infrared system

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61388955%3A_____%2F17%3A00474532" target="_blank" >RIV/61388955:_____/17:00474532 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1002/ctpp.201600061" target="_blank" >http://dx.doi.org/10.1002/ctpp.201600061</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1002/ctpp.201600061" target="_blank" >10.1002/ctpp.201600061</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Monitoring active species in an atmospheric pressure dielectric-barrier discharge: Observation of the Herman-infrared system

  • Original language description

    An electronic and spectroscopic study of dielectric-barrier discharge transition from the Townsend to the filamentary mode is presented. The discharge is generated under pure nitrogen flow at atmospheric pressure in a reactor with parallel configuration of cylindrical electrodes covered with Al2O3 dielectrics, applying a frequency of 4.85 kHz. The goal of the study was to find optimal conditions for observation of the Herman-infrared (HIR) transition (C ''(5)Pi(+)(u)Sigma(+)(g)) in a perspective to develop and test a ro-vibrational model for this quintet band. We have focused on finding the maximum emissivity of the HIR transition in the homogeneous discharge regime as it offers a more suitable source for calibrating the HIR model. Besides the capability of generating a spatially homogeneous type of radiation, our discharge design also allowed the observation of HIR without detectable interference from the first positive system of nitrogen which is not common for atmospheric pressure discharges. In the study, a time-resolved observation of the NO gamma system, the second positive and the HIR nitrogen systems were performed and their emissivities analysed as a function of the discharge period and power. The optimum for the observation of the HIR system was found at 2.94 W (power density of 6 W/cm(3)), corresponding to the Townsend discharge just before its transition to the filamentary one.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10403 - Physical chemistry

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2017

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Contributions to Plasma Physics

  • ISSN

    0863-1042

  • e-ISSN

  • Volume of the periodical

    57

  • Issue of the periodical within the volume

    2

  • Country of publishing house

    DE - GERMANY

  • Number of pages

    9

  • Pages from-to

    67-75

  • UT code for WoS article

    000398735300004

  • EID of the result in the Scopus database

    2-s2.0-85013288091