Determination of Atomic Oxygen in Atmospheric Plasma from Oxygen Isotope Exchange

Oxygen scrambling is observed when a 1:1 mixture of 16O2 and 18O2 in nitrogen/helium buffer (total O2: 5–20%) is treated at atmospheric pressure in a surface discharge plasma reactor. The statistical isotope distribution (16O2/18O2/16O18O = 1:1:2) is achieved with a very low SIE (i.e., the energy pe...

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Published in:Plasma processes and polymers Vol. 8; no. 9; pp. 859 - 866
Main Authors: Schiorlin, Milko, Marotta, Ester, Kim, Hyun-Ha, Paradisi, Cristina, Ogata, Atsushi
Format: Journal Article
Language:English
Published: Weinheim WILEY-VCH Verlag 22-09-2011
WILEY‐VCH Verlag
Wiley-VCH
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Summary:Oxygen scrambling is observed when a 1:1 mixture of 16O2 and 18O2 in nitrogen/helium buffer (total O2: 5–20%) is treated at atmospheric pressure in a surface discharge plasma reactor. The statistical isotope distribution (16O2/18O2/16O18O = 1:1:2) is achieved with a very low SIE (i.e., the energy per unit volume). This process, implemented by kinetic simulations, is proposed as a chemical probe for the determination of the average O‐atom density in atmospheric plasmas. It was found that, within the explored composition range (5–20% O2 in N2/He buffer), the average O‐atom density increases with SIE, while it decreases with increasing content of O2 in the gas being treated. In contrast, an opposite trend is observed for ozone production, which increases with the concentration of O2 in the treated gas. These observations are consistent with the known reaction of O‐atoms with O2 to form ozone, which, at constant total pressure, is expected to favor ozone production as the concentration of O2 is increased. Oxygen scrambling in mixtures of 16O2 and 18O2 diluted in N2/He at atmospheric pressure and room temperature was studied in a surface discharge plasma reactor as a function of energy input. This process, implemented by kinetic simulations, is proposed as a chemical probe for the determination of oxygen atom density, averaged in space and time, in atmospheric plasmas.
Bibliography:Doctoral School in Molecular Sciences of the University of Padova
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ArticleID:PPAP201100024
ObjectType-Article-2
SourceType-Scholarly Journals-1
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ISSN:1612-8850
1612-8869
1612-8869
DOI:10.1002/ppap.201100024