Abstract

Abstract. Chemistry-Climate Model Validation phase 2 (CCMVal-2) model simulations are used to analyze Antarctic ozone increases in 2000–2100 during local spring and early summer, both vertically integrated and at several pressure levels in the lower stratosphere. Multi-model median trends of monthly zonal mean total ozone column (TOC), ozone volume mixing ratio (VMR), wind speed and temperature poleward of 60° S are investigated. Median values are used to account for large variability in models, and the associated uncertainty is calculated using a bootstrapping technique. According to the trend derived from the twelve CCMVal-2 models selected, Antarctic TOC will not return to a 1965 baseline, an average of 1960–1969 values, by the end of the 21st century in September–November, but will return in ~2080 in December. The speed of December ozone depletion before 2000 was slower compared to spring months, and thus the decadal rate of December TOC increase after 2000 is also slower. Projected trends in December ozone VMR at 20–100 hPa show a much slower rate of ozone recovery, particularly at 50–70 hPa, than for spring months. Trends in temperature and winds at 20–150 hPa are also analyzed in order to attribute the projected slow increase of December ozone and to investigate future changes in the Antarctic atmosphere in general, including some aspects of the polar vortex breakup.

Highlights

  • IntroductionOne available method to investigate how a reduction in atmospheric halogen loading to natural “background” lev-

  • One available method to investigate how a reduction in atmospheric halogen loading to natural “background” lev-It has been over 25 yr since the first measurements of significant stratospheric ozone depletion over Antarctica (Farman et al, 1985) was linked with an increase in anthropogenic els will lead to stratospheric ozone recovery in the near future is to analyse simulationSs forolmidstEatae-rotfh-the-art coupled chemistry-climate models (CCMs)

  • Widely spread, show a total ozone column (TOC) minimum around the year 2000 for all months, which is in agreement with Eyring et al (2010a)

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Summary

Introduction

One available method to investigate how a reduction in atmospheric halogen loading to natural “background” lev- It has been over 25 yr since the first measurements of significant stratospheric ozone depletion over Antarctica (Farman et al, 1985) was linked with an increase in anthropogenic els will lead to stratospheric ozone recovery in the near future is to analyse simulationSs forolmidstEatae-rotfh-the-art coupled chemistry-climate models (CCMs). Siddaway et al.: Evolution of Antarctic ozone in September–December used to predict the future behavior of stratospheric ozone in response to different forcings (e.g Eyring et al, 2007) They provide simulations of various atmospheric parameters in three-dimensional space coupled with fully interactive stratospheric ozone chemistry. These will affect ozone levels and complicate the attribution of direct ozone recovery from decreased halogens (Eyring et al, 2010b)

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