Abstract

Abstract. In this work, we analyze the seasonal dependence of ozone trends in the stratosphere using four long-term merged data sets, SAGE-CCI-OMPS, SAGE-OSIRIS-OMPS, GOZCARDS, and SWOOSH, which provide more than 30 years of monthly zonal mean ozone profiles in the stratosphere. We focus here on trends between 2000 and 2018. All data sets show similar results, although some discrepancies are observed. In the upper stratosphere, the trends are positive throughout all seasons and the majority of latitudes. The largest upper-stratospheric ozone trends are observed during local winter (up to 6 % per decade) and equinox (up to 3 % per decade) at mid-latitudes. In the equatorial region, we find a very strong seasonal dependence of ozone trends at all altitudes: the trends vary from positive to negative, with the sign of transition depending on altitude and season. The trends are negative in the upper-stratospheric winter (−1 % per decade to −2 % per decade) and in the lower-stratospheric spring (−2 % per decade to −4 % per decade), but positive (2 % per decade to 3 % per decade) at 30–35 km in spring, while the opposite pattern is observed in summer. The tropical trends below 25 km are negative and maximize during summer (up to −2 % per decade) and spring (up to −3 % per decade). In the lower mid-latitude stratosphere, our analysis points to a hemispheric asymmetry: during local summers and equinoxes, positive trends are observed in the south (+1 % per decade to +2 % per decade), while negative trends are observed in the north (−1 % per decade to −2 % per decade). We compare the seasonal dependence of ozone trends with available analyses of the seasonal dependence of stratospheric temperature trends. We find that ozone and temperature trends show positive correlation in the dynamically controlled lower stratosphere and negative correlation above 30 km, where photochemistry dominates. Seasonal trend analysis gives information beyond that contained in annual mean trends, which can be helpful in order to better understand the role of dynamical variability in short-term trends and future ozone recovery predictions.

Highlights

  • The stratospheric ozone layer plays an important role in the energy budget and dynamics of the middle atmosphere by absorbing a great part of harmful ultraviolet solar radiation

  • In the lower stratosphere (19–23 km), the pattern of statistically significant negative trends of about −2 % per decade to −3 % per decade is present in all merged data sets during the spring and summer months (MAM and JJA), while they are less pronounced in other months

  • A hypothesized explanation of this feature might be the acceleration of the upper branch of the Brewer–Dobson circulation, which controls the meridional transport of trace gases from the tropical region to the poles (Brewer, 1949; Dobson, 1956)

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Summary

Introduction

The stratospheric ozone layer plays an important role in the energy budget and dynamics of the middle atmosphere by absorbing a great part of harmful ultraviolet solar radiation. Upper-stratospheric ozone declined by about 4 % per decade to 8 % per decade in the upper stratosphere from 1980 to the late 1990s (Steinbrecht et al, 2017; WMO, 2018). The Antarctic ozone hole is showing some signs of recovery (Solomon et al, 2016), and the first signatures of global recovery have been observed in the upper stratosphere (Bourassa et al, 2014; Kyrölä et al, 2013; Newchurch et al, 2003; Tummon et al, 2015; WMO, 2018). No significant trend has been detected in global total column ozone and, even though upper-stratospheric ozone is recovering, negative trends have been reported in the lower

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