TY - JOUR
T1 - REACTIONS OF O2 + :O2 WITH CO2, O3, AND O2 plus :O3 WITH H2O AND CH4 AND THEIR ROLE IN STRATOSPHERIC ION CHEMISTRY.
AU - Dotan, I.
AU - Davidson, J. A.
AU - Fehsenfeld, F. C.
AU - Albritton, D. L.
N1 - Copyright:
Copyright 2017 Elsevier B.V., All rights reserved.
PY - 1978
Y1 - 1978
N2 - Thr reactions of O//2** plus :O//2 ions with the minor stratospheric neutrals CO//2, O//3, and CH//4 have been studied in a variable temperature flowing afterglow to test whether they represent reaction paths that can compete with the one leading to H//3O** plus :nH//2O ions and hence can offer the possibility of different terminal ions. The reaction of O//2** plus :O//2 with CH//4 was found to be too slow to be competitive. The measured equilibrium constants of the reactions with CO//2 and O//3 indicated that only the latter, which had an O//2** plus :O//3 product, could play a stratospheric role. The O//2** plus :O//3 ion chemistry was also examined. It was found that the reaction with CH//4 was immeasurably slow but that the reaction with H//2O was fast, yielding O//2** plus :H//2O ions. Since this product ion is part of the sequence of reactions that lead to the H//3O** plus :nH//2O ions, it is concluded that CO//2, O//3, and CH//4 do not afford alternative reaction paths that could rationalize the recent in situ observation of non-H// 3O** plus :nH//2O ions in the lower stratosphere.
AB - Thr reactions of O//2** plus :O//2 ions with the minor stratospheric neutrals CO//2, O//3, and CH//4 have been studied in a variable temperature flowing afterglow to test whether they represent reaction paths that can compete with the one leading to H//3O** plus :nH//2O ions and hence can offer the possibility of different terminal ions. The reaction of O//2** plus :O//2 with CH//4 was found to be too slow to be competitive. The measured equilibrium constants of the reactions with CO//2 and O//3 indicated that only the latter, which had an O//2** plus :O//3 product, could play a stratospheric role. The O//2** plus :O//3 ion chemistry was also examined. It was found that the reaction with CH//4 was immeasurably slow but that the reaction with H//2O was fast, yielding O//2** plus :H//2O ions. Since this product ion is part of the sequence of reactions that lead to the H//3O** plus :nH//2O ions, it is concluded that CO//2, O//3, and CH//4 do not afford alternative reaction paths that could rationalize the recent in situ observation of non-H// 3O** plus :nH//2O ions in the lower stratosphere.
UR - http://www.scopus.com/inward/record.url?scp=0018002686&partnerID=8YFLogxK
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AN - SCOPUS:0018002686
SN - 0148-0227
VL - 83
SP - 4036
EP - 4038
JO - Journal of Geophysical Research
JF - Journal of Geophysical Research
IS - C8
ER -