Atmos. Chem. Phys., 11, 9659-9669, 2011
www.atmos-chem-phys.net/11/9659/2011/
doi:10.5194/acp-11-9659-2011
© Author(s) 2011. This work is distributed
under the Creative Commons Attribution 3.0 License.
Response of the Antarctic stratosphere to warm pool El Niño Events in the GEOS CCM
M. M. Hurwitz1,2,*, I.-S. Song2,3,**, L. D. Oman2, P. A. Newman2, A. M. Molod2,4, S. M. Frith2,5, and J. E. Nielsen2,5
1NASA Postdoctoral Program, NASA Goddard Space Flight Center, Greenbelt, MD, USA
2NASA Goddard Space Flight Center, Greenbelt, MD, USA
3Goddard Earth Sciences and Technology Center (GEST), University of Maryland, Baltimore County, Baltimore, MD, USA
4Earth System Science Interdisciplinary Center (ESSIC), University of Maryland, College Park, College Park, MD, USA
5Science Systems and Applications, Inc., Lanham, MD, USA
*now at: NASA Goddard Earth Sciences Technology and Research (GESTAR), Morgan State University, Baltimore, MD, USA
**now at: Next Generation Model Development Project, Seoul, South Korea

Abstract. The Goddard Earth Observing System Chemistry-Climate Model, Version 2 (GEOS V2 CCM) is used to investigate the response of the Antarctic stratosphere to (1) warm pool El Niño (WPEN) events and (2) the sensitivity of this response to the phase of the QBO. A new formulation of the GEOS V2 CCM includes an improved general circulation model and an internally generated quasi-biennial oscillation (QBO). Two 50-yr time-slice simulations are forced by repeating annual cycles of sea surface temperatures and sea ice concentrations composited from observed WPEN and neutral ENSO (ENSON) events. In these simulations, greenhouse gas and ozone-depleting substance concentrations represent the present-day climate. The modelled responses to WPEN, and to the phase of the QBO during WPEN, are compared with NASA's Modern Era Retrospective-Analysis for Research and Applications (MERRA) reanalysis.

WPEN events enhance poleward tropospheric planetary wave activity in the central South Pacific region during austral spring, leading to relative warming of the Antarctic lower stratosphere in November/December. During the easterly phase of the QBO (QBO-E), the GEOS V2 CCM reproduces the observed 4–5 K warming of the polar region at 50 hPa, in the WPEN simulation relative to ENSON.

In the recent past, the response to WPEN events was sensitive to the phase of the QBO: the enhancement in planetary wave driving and the lower stratospheric warming signal were mainly associated with WPEN events coincident with QBO-E. In the GEOS V2 CCM, however, the Antarctic response to WPEN events is insensitive to the phase of the QBO: the modelled response is always easterly QBO-like. The QBO signal does not extend far enough into the lower stratosphere and upper troposphere to modulate convection and thus planetary wave activity in the south central Pacific.


Citation: Hurwitz, M. M., Song, I.-S., Oman, L. D., Newman, P. A., Molod, A. M., Frith, S. M., and Nielsen, J. E.: Response of the Antarctic stratosphere to warm pool El Niño Events in the GEOS CCM, Atmos. Chem. Phys., 11, 9659-9669, doi:10.5194/acp-11-9659-2011, 2011.
 
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