1999
DOI: 10.1016/s0009-2614(99)00469-8
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Pressure dependence of two relative ozone formation rate coefficients

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Cited by 52 publications
(67 citation statements)
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“…The results are summarized elsewhere. 1 The experiments involve a ''mass-independent'' isotope effect in ozone formation in scrambled systems and contrastingly different experimental results [25][26][27][28][29] in unscrambled systems. The latter show, instead, dramatic unconventional mass-dependent effects.…”
Section: Introductionmentioning
confidence: 99%
“…The results are summarized elsewhere. 1 The experiments involve a ''mass-independent'' isotope effect in ozone formation in scrambled systems and contrastingly different experimental results [25][26][27][28][29] in unscrambled systems. The latter show, instead, dramatic unconventional mass-dependent effects.…”
Section: Introductionmentioning
confidence: 99%
“…We hypothesize that the high isotope enrichments, reflected in both the δ 18 O and the 17 O values, occur when O 3 oxidation of NO is faster than NO x -O-O 2 isotopic exchange. Isotopic enrichments associated with the formation of O 3 have been extensively studied Guenther et al, 1999;Mauersberger et al, 2003;Thiemens, 1999). At temperature and pressure range of the present experiments, the recombination process should generate O 3 with δ 18 O values between 90-130 ‰ and 17 O values between 30-45 ‰ .…”
Section: Discussion and Model Predictionsmentioning
confidence: 65%
“…The first is the NO 2 -NO equilibrium (Sharma et al, 1970 Guenther et al (1999) and Mauersberger et al (2005). * * * 17 O = 1000 · ln(1+δ 17 O/1000)−0.516 · 1000 · ln(1+δ 18 O/1000) measures the magnitude of mass independent enrichment.…”
Section: Accounting For Isotopes Of Total No X In the Modelmentioning
confidence: 99%
“…There exist mainly two types of experimental observations: an unusual "mass-independent" isotopic fractionation ͑MIF͒ of ozone and a large unconventional highly "mass-dependent" isotope effect observed in the various rate constant ratios. [25][26][27][28][29] Rice-RamspergerKassel-Marcus ͑RRKM͒ theory with a master equation approach for the collisional deactivation of the intermediate excited ozone molecules has been applied to study both phenomena. [32][33][34] It was found that the MIF can be explained when an -effect, a non-RRKM effect, [30][31][32][33][34] which reduces dynamically the low-pressure rate constant of the recombination to form symmetric molecules by a factor of compared to that for the asymmetric ones, and a weak collision effect [32][33][34] for the deactivation of excited ozone molecules is also included in the theory.…”
Section: Introductionmentioning
confidence: 99%