Atmos. Chem. Phys. Discuss., 10, 14875-14896, 2010
www.atmos-chem-phys-discuss.net/10/14875/2010/
doi:10.5194/acpd-10-14875-2010
© Author(s) 2010. This work is distributed
under the Creative Commons Attribution 3.0 License.
Review Status
This discussion paper has been under review for the journal Atmospheric Chemistry and Physics (ACP). Please refer to the corresponding final paper in ACP.
Correlating tropospheric column ozone with tropopause folds: the Aura-OMI satellite data
Q. Tang and M. J. Prather
Department of Earth System Science, University of California, Irvine, California, 92617, USA

Abstract. The geographic and temporal variations in tropospheric and stratospheric ozone columns from individual swath measurements of the Ozone Monitoring Instrument (OMI) on the NASA Aura spacecraft are reasonably well simulated by the University of California, Irvine (UCI) chemistry transport model (CTM) using 1°×1°×40-layer meteorological fields for year 2005. From the CTM we find that high-frequency spatial variations in tropospheric column ozone (TCO), including around the jet streams, are not generally correlated with variations in stratospheric ozone column, but instead are collocated with folding events involving stratospheric-origin, high-ozone layers below the tropopause. The CTM fold events are verified in many cases with available ozone sondes. Using the OMI Level 2 profiles, and defining tropopause height from our CTM using the European Centre for Medium-Range Weather Forecasts (ECMWF) fields, we find that most of the variations in TCO near CTM folding events are also not correlated with those in stratospheric ozone column. The absolute tropospheric columns from OMI and CTM agree swath-by-swath, pixel-by-pixel within ±5 Dobson Units (DU) for most cases. Notable exceptions are in the tropics where neither the high ozone from biomass burning nor the low ozone in the convergence zones over the Pacific is found in the OMI observations, likely because of OMI's insensitivity to the lower troposphere. A separate bias is identified with the OMI profiles near the southern sub-tropical jet. The CTM has a high bias in stratospheric column outside the tropics, due to problems previously identified with the stratospheric circulation in the 40-layer meteorological fields. Overall, we identify ozone folds with short-lived features in TCO that have scales of a few hundred kilometers as observed by OMI.

Citation: Tang, Q. and Prather, M. J.: Correlating tropospheric column ozone with tropopause folds: the Aura-OMI satellite data, Atmos. Chem. Phys. Discuss., 10, 14875-14896, doi:10.5194/acpd-10-14875-2010, 2010.
 
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