Stability and excitation dynamics of an argon micro-scaled atmospheric pressure plasma jet

dc.bibliographicCitation.firstPage065018eng
dc.bibliographicCitation.issue6eng
dc.bibliographicCitation.journalTitlePlasma sources science and technologyeng
dc.bibliographicCitation.volume24eng
dc.contributor.authorDünnbier, M.
dc.contributor.authorBecker, M.M.
dc.contributor.authorIseni, S.
dc.contributor.authorBansemer, R.
dc.contributor.authorLoffhagen, D.
dc.contributor.authorReuter, S.
dc.contributor.authorWeltmann, K.-D.
dc.date.accessioned2022-08-11T06:32:40Z
dc.date.available2022-08-11T06:32:40Z
dc.date.issued2015
dc.description.abstractA megahertz-driven plasma jet at atmospheric pressure—the so-called micro-scaled atmospheric pressure plasma jet (μAPPJ)—operating in pure argon has been investigated experimentally and by numerical modelling. To ignite the discharge in argon within the jet geometry, a self-made plasma tuning unit was designed, which additionally enables measurements of the dissipated power in the plasma itself. Discharges in the α-mode up to their transition to the γ-mode were studied experimentally for varying frequencies. It was found that the voltage at the α–γ transition behaves inversely proportional to the applied frequency f and that the corresponding power scales with an f  3/2law. Both these findings agree well with the results of time-dependent, spatially one-dimensional fluid modelling of the discharge behaviour, where the f  3/2 scaling of the α–γ transition power is additionally verified by the established concept of a critical plasma density for sheath breakdown. Furthermore, phase resolved spectroscopy of the optical emission at 750.39 nm as well as at 810.37 nm and 811.53 nm was applied to analyse the excitation dynamics of the discharge at 27 MHz for different applied powers. The increase of the power leads to an additional maximum in the excitation structure of the 750.39 nm line emission at the α–γ transition point, whereas the emission structure around 811 nm does not change qualitatively. According to the fluid modelling results, this differing behaviour originates from the different population mechanisms of the corresponding energy levels of argon.eng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/9984
dc.identifier.urihttp://dx.doi.org/10.34657/9022
dc.language.isoengeng
dc.publisherBristol : IOP Publ.eng
dc.relation.doihttps://doi.org/10.1088/0963-0252/24/6/065018
dc.relation.essn1361-6595
dc.rights.licenseCC BY 3.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/eng
dc.subject.ddc530eng
dc.subject.otherargon atmospheric pressure plasma jeteng
dc.subject.otherdissipated powereng
dc.subject.otherexcitation dynamicseng
dc.subject.otherexperiment and modelingeng
dc.subject.otherα-γ-mode transitioneng
dc.titleStability and excitation dynamics of an argon micro-scaled atmospheric pressure plasma jeteng
dc.typeArticleeng
dc.typeTexteng
tib.accessRightsopenAccesseng
wgl.contributorINPeng
wgl.subjectPhysikeng
wgl.typeZeitschriftenartikeleng
Files
Original bundle
Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
Stability_and_excitation.pdf
Size:
2.47 MB
Format:
Adobe Portable Document Format
Description:
Collections