2022
DOI: 10.1088/1361-6595/aca4f2
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Characterization of an atmospheric pressure plasma jet producing the auroral transition O(1S) to O(1D)

Abstract: We present a detailed characterization of an atmospheric pressure plasma jet that produces the metastable oxygen states O(1S) and O(1D) with emission of the “auroral” green line. The device used 99.999% pure argon as a working gas for the plasma generation. Optical emission spectroscopy was used to understand the active species present in the plasma jet and to infer the mechanism of O(1S) creation and destruction. The continuum spectrum was used in conjunction with a method based on machine learning for determ… Show more

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Cited by 3 publications
(8 citation statements)
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“…In atmospheric pressure N 2 discharge, the lifetime of O( 1 S) was estimated to be in the range of 1-20 ms by comparing the intensity ratio of 557.7 nm to the competing line at 297.2 nm with the theoretical ratio [37]. Given the existence of ArO(1S) excimer, if taking the increased transition probability by a factor of 576 calculated in [19] into account, the lifetime of ArO( 1 S) is also on the order of 1-2 ms, which is several tens of times the discharge period in our experiment.…”
Section: Discharge Morphologymentioning
confidence: 99%
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“…In atmospheric pressure N 2 discharge, the lifetime of O( 1 S) was estimated to be in the range of 1-20 ms by comparing the intensity ratio of 557.7 nm to the competing line at 297.2 nm with the theoretical ratio [37]. Given the existence of ArO(1S) excimer, if taking the increased transition probability by a factor of 576 calculated in [19] into account, the lifetime of ArO( 1 S) is also on the order of 1-2 ms, which is several tens of times the discharge period in our experiment.…”
Section: Discharge Morphologymentioning
confidence: 99%
“…The rise in T e in this regime would be likely to cause an increase in the density of Ar atoms in the metastable levels, which can be proved in figure 9(a), as those are typically populated by direct electron impact. Ar metastables (their energy levels are at 11.5-11.8 eV) are expected to increase atomic oxygen density providing that the dissociative excitation of O 2 is principally driven by the reaction [ The dissociation of O 2 is most probably driven by electron impact, as also indicated in [19]. The weak intensity of the 777.4 nm line from the spectrum (figure 2), indicates that the downstream region of this discharge operates at electron energies that are lower than typically observed in DBDs.…”
Section: Analysis Of the 'Two Branches' Feature Corresponding To Two ...mentioning
confidence: 99%
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“…Through this, the impact of inconsistencies in the OES setup, discharge conditions or optical calibration can be reduced. The basic principles and limitations of this method were discussed in [45][46][47]. This paper shows the measured spectra and EEDF results of OES measurements from a CAPP DBD.…”
Section: Introductionmentioning
confidence: 99%