JP9.6
A model study of the effect of ozone depletion on lower-stratospheric structure
Mark A. Olsen, NASA/GSFC, Greenbelt, MD; and R. Stolarski, M. L. Gupta, J. E. Nielsen, and S. Pawson
We have run two twenty-year integrations of a global circulation model using 1978-1980 and 1998-2000 monthly mean ozone climatologies. The ozone climatology is used solely in the radiation scheme of the model. Several key differences between the model runs will be presented. The temperature and potential vorticity (PV) structure of the lower stratosphere, particularly in the Southern Hemisphere, is significantly changed using the 1998-2000 ozone climatology. In the Southern Hemisphere summer, the lapse rate and PV-defined polar tropopauses both lie several hundred meters higher than the 1978-1980 climatological run. The 380 K potential temperature surface is likewise at a greater altitude. The mass of the extratropical lowermost stratosphere (between the tropopause and 380 K surface) remains unchanged. The altitude differences are not observed in the Northern Hemisphere. The different ozone fields do not produce a significant change in the annual extratropical stratosphere-troposphere exchange of mass although slight variations in the spatial distribution of the exchange exist. We are also investigating a delay in the breakup of the Southern Hemisphere polar vortex due to the differing ozone climatologies.
Joint Poster Session 9, Stratosphere chemistry/radiation/climate feedback processes--POSTER (Joint with Middle Atmosphere, Fluid Dynamics and Climate Variation)
Friday, 17 June 2005, 8:30 AM-10:30 AM, Riverside
Previous paper