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Atmospheric Chemistry and Physics An interactive open-access journal of the European Geosciences Union
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Volume 16, issue 24 | Copyright
Atmos. Chem. Phys., 16, 15485-15500, 2016
https://doi.org/10.5194/acp-16-15485-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.

Research article 15 Dec 2016

Research article | 15 Dec 2016

An upper-branch Brewer–Dobson circulation index for attribution of stratospheric variability and improved ozone and temperature trend analysis

William T. Ball1,2, Aleš Kuchař3, Eugene V. Rozanov1,2, Johannes Staehelin1, Fiona Tummon1, Anne K. Smith4, Timofei Sukhodolov1,2, Andrea Stenke1, Laura Revell1,5, Ancelin Coulon1, Werner Schmutz2, and Thomas Peter1 William T. Ball et al.
  • 1Institute for Atmospheric and Climate Science, Swiss Federal Institute of Technology Zurich, Universitaetstrasse 16, 8092 Zurich, Switzerland
  • 2Physikalisch-Meteorologisches Observatorium Davos World Radiation Centre, Dorfstrasse 33, 7260 Davos Dorf, Switzerland
  • 3Department of Atmospheric Physics, Faculty of Mathematics and Physics, Charles University, V Holesovickach 2, 180 00 Prague 8, Czech Republic
  • 4National Center for Atmospheric Research, Boulder, Colorado
  • 5Bodeker Scientific, Alexandra, New Zealand

Abstract. We find that wintertime temperature anomalies near 4hPa and 50°N/S are related, through dynamics, to anomalies in ozone and temperature, particularly in the tropical stratosphere but also throughout the upper stratosphere and mesosphere. These mid-latitude anomalies occur on timescales of up to a month, and are related to changes in wave forcing. A change in the meridional Brewer–Dobson circulation extends from the middle stratosphere into the mesosphere and forms a temperature-change quadrupole from Equator to pole. We develop a dynamical index based on detrended, deseasonalised mid-latitude temperature. When employed in multiple linear regression, this index can account for up to 60% of the total variability of temperature, peaking at  ∼ 5hPa and dropping to 0 at  ∼ 50 and  ∼ 0.5hPa, respectively, and increasing again into the mesosphere. Ozone similarly sees up to an additional 50% of variability accounted for, with a slightly higher maximum and strong altitude dependence, with zero improvement found at 10hPa. Further, the uncertainty on all equatorial multiple-linear regression coefficients can be reduced by up to 35 and 20% in temperature and ozone, respectively, and so this index is an important tool for quantifying current and future ozone recovery.

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We find monthly, mid-latitude temperature changes above 40 km are related to ozone and temperature variations throughout the middle atmosphere. We develop an index to represent this atmospheric variability. In statistical analysis, the index can account for up to 60 % of variability in tropical temperature and ozone above 27 km. The uncertainties can be reduced by up to 35 % and 20 % in temperature and ozone, respectively. This index is an important tool to quantify current and future ozone recovery.
We find monthly, mid-latitude temperature changes above 40 km are related to ozone and...
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