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Ozone Hole may Affect Ocean Circulation

Page history last edited by Malcolm 12 years, 9 months ago

http://www.eurekalert.org/pub_releases/2011-07/agu-ajh071511.php

8. Ozone hole might affect Great Ocean Conveyor

Previous studies have suggested that key aspects of the Southern Ocean are affected by elevated atmospheric carbon dioxide levels. Increasing greenhouse gas (GHG) concentrations, which strengthen surface winds over much of the Southern Ocean, may increase flow rates in the Antarctic Circumpolar Current (ACC), induce a temperature disparity between the northern and central Southern Ocean, and affect the strength of the meridional ocean circulation (MOC), also known as Great Ocean Conveyor. But GHGs are not the only set of chemicals arising from human activity that can trigger these changes. Stratospheric ozone depletion due to ozone depleting substances (ODSs) such as chlorofluorocarbons, whose production and use were heavily regulated by the 1987 Montreal Protocol, results in similar changes.

Using an atmosphere-ocean coupled general circulation model that allows for detailed calculations of stratospheric chemistry, Sigmond et al. simulate past and future changes for the Southern Ocean due to both greenhouse gases and ozone depleting substances. Their model calculations suggest that ODSs, which peaked in concentration in 1995, will be the dominant driver of changes in the ACC until the second quarter of the 21st century, at which point the monotonically increasing GHG levels will take over. Further, the authors find that the peak impact of ODSs on the ACC will occur a few decades after their peak concentration. The authors suggest that future research needs to take into account the effects of ozone depletion—something that is not ordinarily done in investigations of Southern Ocean behavior.

Source: Geophysical Research Letters, doi:10.1029/2011GL047120, 2011
http://dx.doi.org/10.1029/2011GL047120

Title: Drivers of past and future Southern Ocean change: Stratospheric ozone versus greenhouse gas impacts

Authors: M. Sigmond: Department of Physics, University of Toronto, Toronto, Ontario, Canada;

M. C. Reader: School of Earth

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