ATMOSPHERIC CHEMISTRY 135
with ozone to form ClO. This ClO may react with itself to
form the dimer, (ClO) 2 :
ClO ClO M → (ClO) 2 M (59)
Under high-ClO-concentration conditions, the following
catalytic cycle could be responsible for the destruction of
ozone:
2 × (Cl O 3 → ClO O 2 ) (51)
ClO ClO M → (ClO) 2 M (59)
(ClO) 2 h → Cl ClOO (60)
ClOO M → Cl O 2 (61)
2O 3 → 3O 2 (Net)
This ClO-driven catalytic cycle can effectively destroy O 3 ,
but it requires the presence of sunlight to photolyze Cl 2 and
(ClO) 2. The presence of sunlight will lead to an increase in
temperature that releases HNO 3 back to the gas phase. The
photolysis of HNO 3 can release NO 2 , which can react with
ClO by reaction (58) to re-form ClONO 2. This can termi-
nate the unusual chlorine-catalyzed destruction of ozone that
occurs in polar regions.
Anderson (1995) suggests that the same processes occur
in both the Arctic and Antarctic polar regions. The main
distinction is that it does not get as cold in the Arctic, and
the polar stratospheric clouds do not persist as long after the
polar sunrise. As the temperature rises above 195 K, nitric
acid is released back into the gas phase only shortly after
Cl 2 photolysis begins. As nitric acid is photolyzed, forming
NO 2 , the ClO reacts with NO 2 to form ClONO 2 and termi-
nate the chlorine-catalyzed destruction of ozone. Anderson
(1995) suggests that the temperatures warmed in late January
1992, and ozone loss was only 20 to 30% at the altitudes of
peak ClO. The temperatures remained below 195 K until late
February 1993, and significantly more ozone will be lost.
The delay between the arrival of sunlight and the rise of
temperatures above 195 K are crucial to the degree of ozone
loss in the Arctic.
Summary
The observations made in the polar regions provided the key
link between chlorine-containing compounds in the strato-
sphere and destruction of stratospheric ozone. These experi-
mental results led to the Montreal Protocol agreements and
their subsequent revisions to accelerate the phase-out of
the use of CFCs. A tremendous amount of scientific effort
over many years has led to our current understanding of the
effects of Cl-containing species on the stratosphere.
CLOSING REMARKS
Our knowledge and understanding has improved consider-
ably in recent years. Much of the reason for this improved
knowledge is the result of trying to understand how we are
affecting our environment. From the foregoing discussion, it
POLAR NIGHT SUNLIGHT
- COOLING
- DESCENT
PSC
CHEMISTRY
Cl 2 + 2Cl ClO.Cl 3 O 2
HNO 2 NO 2
ClO + NO 2 ClO + NO 2
CH 4 + Cl HCl + CH 3
ClO + 2Cl NO + ClO Cl + NO^2
2 O 3
ClONO 2
ClONO 2
O 3 LOSS
TIME
0
1
2
3
MIXING RATIO (ppbv)
RECOVERY
HCl
HCl
FIGURE 11 Schematic of the time evolution of the chlorine chemistry, illustrating the
importance of the initial HCl/ClONO 2 ratio, the sudden formation of ClO with returning
sunlight, the way in which ClONO 2 levels can build up to mixing ratios in excess of its initial
values, and the slow recovery of HCl levels. From Webster et al. (1993). With permission.
C001_008_r03.indd 135C001_008_r03.indd 135 11/18/2005 10:15:24 AM11/18/2005 10:15:24 AM