Abstract

Abstract. In this study we use ozone and stratospheric ozone tracer simulations from the high-resolution (0.5∘×0.5∘) Goddard Earth Observing System, Version 5 (GEOS-5), in a replay mode to study the impact of stratospheric ozone on tropospheric ozone interannual variability (IAV). We use these simulations in conjunction with ozonesonde measurements from 1990 to 2016 during the winter and spring seasons. The simulations include a stratospheric ozone tracer (StratO3) to aid in the evaluation of the impact of stratospheric ozone IAV on the IAV of tropospheric ozone at different altitudes and locations. The model is in good agreement with the observed interannual variation in tropospheric ozone, except for the post-Pinatubo period (1992–1994) over the region of North America. Ozonesonde data show a negative ozone anomaly in 1992–1994 following the Pinatubo eruption, with recovery thereafter. The simulated anomaly is only half the magnitude of that observed. Our analysis suggests that the simulated stratosphere–troposphere exchange (STE) flux deduced from the analysis might be too strong over the North American (50–70∘ N) region after the Mt. Pinatubo eruption in the early 1990s, masking the impact of lower stratospheric ozone concentration on tropospheric ozone. European ozonesonde measurements show a similar but weaker ozone depletion after the Mt. Pinatubo eruption, which is fully reproduced by the model. Analysis based on the stratospheric ozone tracer identifies differences in strength and vertical extent of stratospheric ozone impact on the tropospheric ozone interannual variation (IAV) between North America and Europe. Over North American stations, the StratO3 IAV has a significant impact on tropospheric ozone from the upper to lower troposphere and explains about 60 % and 66 % of the simulated ozone IAV at 400 hPa and ∼11 % and 34 % at 700 hPa in winter and spring, respectively. Over European stations, the influence is limited to the middle to upper troposphere and becomes much smaller at 700 hPa. The Modern-Era Retrospective analysis for Research and Applications, Version 2 (MERRA-2), assimilated fields exhibit strong longitudinal variations over Northern Hemisphere (NH) mid-high latitudes, with lower tropopause height and lower geopotential height over North America than over Europe. These variations associated with the relevant variations in the location of tropospheric jet flows are responsible for the longitudinal differences in the stratospheric ozone impact, with stronger effects over North America than over Europe.

Highlights

  • Tropospheric ozone plays an important role in the oxidative capacity of the troposphere

  • We examine the vertical extents of stratosphere–troposphere exchange (STE) impact on tropospheric ozone using model simulations and ozonesonde measurements sampled over North America and Europe

  • We focus on the winter (DJF) and spring (MAM) seasons to examine the interannual variations in the strength and vertical extent of stratospheric ozone impact on the tropospheric ozone

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Summary

Introduction

Tropospheric ozone plays an important role in the oxidative capacity of the troposphere. Hess et al (2015) analyzed the effects of stratospheric input to tropospheric ozone variations over the Northern Hemisphere midlatitudes with four ensemble simulations of the free running Whole Atmosphere Community Climate Model (WACCM) for 1953 to 2005. Their model used a standard stratospheric chemical mechanism and simple CH4-NOx chemistry in the troposphere with constant surface emissions of ozone precursors. We use a long-term full chemistry GEOSCCM replay simulation, driven by the essential output of the MERRA-2 meteorology (U , V , T , pressure), with a stratospheric ozone tracer at a horizontal resolution of 0.5◦ This is the suggested minimum model resolution needed to resolve the structure of deep STE events (Ott et al, 2016).

Ozonesondes
MERRA2-GMI
Results
Impact of stratospheric ozone on tropospheric ozone IAV
Case study of 3-D dynamic characteristics
Longitudinal difference in stratospheric ozone influence
Conclusions and discussion
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