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This figure shows MLS maps on four selected days which
illustrate the evolution of lower stratospheric ClO and ozone during the
1992 southern hemisphere winter. The data have been vertically-interpolated
to the 465 K potential temperature isentropic surface (approximately 20
km). The thick black contours concentric with the pole on the ClO maps
show the daylight edge of MLS measurements, and the thin white contour
concentric with the pole indicates the edge of polar night. The green contours
indicate temperatures of 195 K (outer contour) and 190 K (inner contour).
Irregular white contours indicate the approximate edge of the polar vortex
(potential vorticity contours of -2.5 and -3.0 x 10-5 K m2
kg-1 s-1). These were the first measurements of Antarctic
ClO made during early and mid winter. They show that enhanced ClO can appear
by the first of June, and remain enhanced throughout the winter in the
sunlit regions of the vortex. Both the outer and inner edges of enhanced
ClO move poleward during mid to late winter. Poleward retreat of the outer
edge is expected due to quenching of ClO by NO2 produced by
the increased photolysis of HNO3 as the sun rises higher in
the sky. Poleward retreat of the inner edge of enhanced ClO is expected
due to the returning sun's photolysis of ClOOCl producing ClO. Note that
the enhanced ClO extends, at times, equatorward of 60o latitude.
During early winter (note the 1 June and 11 July maps) ozone increases
in the lower stratospheric vortex, as can be explained by descent of ozone-rich
air from above. This descent brings in more ozone than is destroyed by
the enhanced ClO during this period. However, by mid-August the chlorine
destruction in this layer dominates the increase due to influx: ozone has
decreased between 11 July and 14 August in the region where there is largest
ClO. Further ozone depletion occurs between mid-August and mid-September,
leading to the formation of the ozone hole. These data indicate that loss
of ozone occurs in the southern vortex before development of the ozone
hole, which is generally taken to start in September. The low ozone abundances
in the tropics at this altitude are normal, and are due to the rising air
motions which bring ozone-poor air up from below (which was likely enhanced
by effects of the Pinatubo volcano). See Waters, et al. GRL 20, 1219-1222
[1993] for more discussion.
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