Ozone is a minor but important constituent of the earth's atmosphere. While it is essential for life as we know it today, it is also a toxic gas that can result in significant physiological and ecological damage, if exposures exceed critical limits. In both the stratosphere and troposphere, ozone concentration levels depend on multitudes of linked chemical and meteorological mechanisms, which vary profoundly with space and time. Human pollutant emissions often perturb these linkages, resulting in significant increases or decreases in ozone concentration. While many facets of ozone's atmospheric behavior are well understood, a large number of important uncertainties remain, whose resolution will require substantial combined efforts by the meteorological and chemical communities. The American Meteorological Society (AMS) intends to assist in the provision of a forum for such future joint interactions.
Despite many uncertainties, ample evidence exists to substantiate that atmospheric ozone has been affected in important and even critical ways by human activity. In the case of the stratosphere, the existence of the Antarctic ozone hole is unquestionable, and our evidence that it results from human-produced halocarbons is overwhelming. Ozone depletion in the midlatitude stratosphere is less dramatic; however, the general agreement of the large numbers of available column and profile measurements makes it reasonable to speculate that such depletion is indeed occurring and that it is largely human induced.
Anthropogenic activities also significantly influence tropospheric ozone. Humankind is directly responsible for the excessive ozone levels that often occur near the surface in and downwind from populated areas. These effects are also felt throughout significant regions of the free troposphere.
The effects in both the stratosphere and troposphere are sufficiently profound to mandate substantial concern, both on both a local and a global basis.
With regard to the Montreal Protocol, it is encouraging to note that halocarbon limitations under this agreement appear to have resulted, recently, in decreases of some of the shorter-lived halogen-containing species. Owing to the noted uncertainties and complexities associated with stratospheric ozone depletion, however, the effects of this and other international agreements must be monitored continuously and carefully to ensure their effectiveness and to establish the basic understanding required for more effective maintenance during future year
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