Kinetics of the IO Radical. 1
40 kcal mol-1 32
J. Phys. Chem. A, Vol. 101, No. 30, 1997 5525
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)
suggests that this channel would be ≈13 kcal
mol-1 endothermic and, thus, unimportant. The lack of any
pressure dependence in the rate coefficient also suggests that
stabilization of IClO2 is not important in our system. However,
all of our measurements were done at <15 Torr; therefore, this
species cannot be completely ruled out at higher pressures.
Mauldin et al.30 observed an unknown product in the BrO +
BrO reaction at 223 K and 300 Torr N2 and tentatively identified
it as Br2O2. Similar observations have been reported suggesting
that formation of IClO2 may also be possible.33
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Our experiments cannot distinguish between channels 5b and
the channels that produce atomic I and Cl. In the atmosphere,
the production of I + OClO in reaction 5 will not lead to a net
ozone loss. We attempted to monitor OClO by LIF; however,
our detection sensitivity was an order of magnitude too poor to
observe the concentrations of OClO that could be produced
under our experimental conditions.
Atmospheric Implications. The modeling study of Solomon
et al.8 assumed k5 ) 1 × 10-10 cm3 molecule-1 s-1. Using
this rate coefficient, a total iodine abundance of 1 pptv in the
stratosphere was necessary to completely account for the
observed trend in low-altitude, midlatitude O3 loss during the
past two decades. Our measured value at temperatures char-
acteristic of the stratosphere is approximately a factor of 5 lower
than the assumed value. Thus, the interaction of iodine with
chlorine will be five times less efficient at destroying ozone
than predicted if we assume reaction 5 does not produce OClO.
The contribution of this reaction to stratospheric ozone loss is
discussed in detail in the next paper.
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Note Added in Proof. Yuri Bedjanian, Georges Le Bras
and Gilles Poulet have measured the 298 K rate coefficient k5-
(298 K) ) (1.1 ( 0.2) × 10-11 cm3 molecule-1 s-1 using a
mass spectrometric discharge flow system (J. Phys. Chem. A
1997, 101, 4088). They also report branching ratios of (0.55
( 0.03), (0.25 ( 0.02), and (0.20 ( 0.02) for channels 5b, 5f,
and 5c, respectively. These results are in excellent agreement
with those reported in this paper.
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Acknowledgment. The authors thank Dr. S. Solomon for
useful discussions concerning this work. We also acknowledge
Dr. Bedjanian for both sending us preprints prior to publication
and his insightful comments. This work was funded in part by
NASA’s Mission to Planet Earth Program through the Upper
Atmospheric Research Program.
References and Notes
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