skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Transport, radiative, and dynamical effects of the antarctic ozone hole: A GFDL SKYHI' model experiment

Journal Article · · Journal of the Atmospheric Sciences; (United States)
;  [1];  [2]
  1. Princeton Univ., Princeton, NJ (United States)
  2. Environmental Protection Agency, Research Triangle Park, NC (United States)

The GFDL SKYHI' general circulation model has been used to simulate the effect of the Antarctic ozone hole' phenomenon on the radiative and dynamical environment of the lower stratosphere. Both the polar ozone destruction and photochemical restoration chemistries are calculated by parameterized simplifications of the still somewhat uncertain chemical processes. The modeled total column ozone depletions are near 25% in spring over Antarctica, with 1% depletion reaching equatorial latitudes by the end of the 4 1/2-year model experiment. In the lower stratosphere, ozone reductions of 5% reach to the equator. Large coolings of about 8 K are simulated in the lower stratospheric over Antarctica in late spring, while a general cooling of about 1-1.5 K is present throughout the Southern Hemisphere lower stratosphere. The model atmosphere experiences a long-term positive temperature-chemical feedback because significant ozone reductions carry over into the next winter. The overall temperature response to the reduced ozone is essentially radiative in character. However, substantial dynamical changes are induced by the ozone hole effect. The Antarctic middle stratosphere in late spring warms by about 6 K over Antarctica and the lower midlatitude stratosphere warms by approximately 1 K. These warming spots are produced mainly by an increased residual circulation intensity. Also, the Antarctic vortex becomes tighter and more confined as a result of the reduced ozone. These two dynamical effects combine to steepen the meridional slope of quasi-conservative trace constituent isolines. Thus, the entire transport, radiative, and dynamical climatology of the springtime stratosphere is affected to an important degree by the ozone hole phenomenon. Over the entire year, however, these dynamical effects are considerably smaller. 27 refs., 13 figs.

OSTI ID:
7012394
Journal Information:
Journal of the Atmospheric Sciences; (United States), Vol. 51:4; ISSN 0022-4928
Country of Publication:
United States
Language:
English