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

We find that wintertime temperature anomalies near 4 hPa and 50 degrees 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 similar to 5 hPa and dropping to 0 at similar to 50 and similar to 0.5 hPa, 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 10 hPa. 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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Related Dataset #1 : MLR data to "An Upper-branch Brewer Dobson Circulation index for attribution of stratospheric variability and improved ozone and temperature trend analysis"

Related Software #1 : Seaborn: V0.7.0 (January 2016)

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Publication Date 2016-12-15T00:00:00
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Metadata Date 2025-07-11T19:53:07.380742
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Metadata Language eng; USA
Suggested Citation . (2016). An upper-branch Brewer-Dobson circulation index for attribution of stratospheric variability and improved ozone and temperature trend analysis. UCAR/NCAR - Library. https://n2t.org/ark:/85065/d7765h3t. Accessed 04 January 2026.

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