Possible dynamical mechanisms for Southern Hemisphere climate change due to the ozone hole

Orr, Andrew ORCID:; Bracegirdle, Thomas J. ORCID:; Hosking, J. Scott ORCID:; Jung, Thomas; Haigh, Joanna D.; Phillips, Tony ORCID:; Feng, Wuhu. 2012 Possible dynamical mechanisms for Southern Hemisphere climate change due to the ozone hole. Journal of the Atmospheric Sciences, 69 (10). 2917-2932.

Before downloading, please read NORA policies.
Copyright 2012 American Meteorological Society
jas-d-11-0210%2E1.pdf - Published Version

Download (2MB)


The authors report a hypothesis for the dynamical mechanisms responsible for the strengthening of the Southern Hemisphere circumpolar winds from the lower stratosphere to the surface due to the ozone hole. A general circulation model forced by stratospheric ozone depletion representative of the ozone hole period successfully reproduced these observed changes. Investigation of the dynamical characteristics of the model therefore provides some insight into the actual mechanisms. From this the authors suggest the following: 1) An initial (radiative) strengthening of the lower-stratospheric winds as a result of ozone depletion conditions the polar vortex so that fewer planetary waves propagate up from the troposphere, resulting in weaker planetary wave driving. 2) This causes further strengthening of the vortex, which results in an additional reduction in upward-propagating planetary waves and initiates a positive feedback mechanism in which the weaker wave driving and the associated strengthened winds are drawn downward to the tropopause. 3) In the troposphere the midlatitude jet shifts poleward in association with increases in the synoptic wave fluxes of heat and momentum, which are the result of a positive feedback mechanism consisting of two components: 4) increases in low-level baroclinicity, and the subsequent generation of baroclinic activity (associated with a poleward heat flux), are collocated with the jet latitudinal position, and 5) strengthening anticyclonic shear increases the refraction of wave activity equatorward (associated with a poleward momentum flux). Finally, 6) confinement of planetary waves in the high-latitude troposphere is an important step to couple the stratospheric changes to the tropospheric response.

Item Type: Publication - Article
Digital Object Identifier (DOI):
Programmes: BAS Programmes > Polar Science for Planet Earth (2009 - ) > Climate
ISSN: 0022-4928
NORA Subject Terms: Atmospheric Sciences
Date made live: 19 Dec 2012 10:58 +0 (UTC)

Actions (login required)

View Item View Item

Document Downloads

Downloads for past 30 days

Downloads per month over past year

More statistics for this item...