Abstract. The circulation of the stratosphere, also known as the Brewer–Dobson
circulation, transports water vapor and ozone, with implications for
radiative forcing and climate. This circulation is typically quantified from
model output by calculating the tropical upwelling vertical velocity in the
residual circulation framework, and it is estimated from observations by
using time series of tropical water vapor to infer a vertical velocity.
Recent theory has introduced a method to calculate the strength of the global
mean diabatic circulation through isentropes from satellite measurements of
long-lived tracers. In this paper, we explore this global diabatic
circulation as it relates to the residual circulation vertical velocity,
stratospheric water vapor, and ozone at interannual timescales. We use a
comprehensive climate model, three reanalysis data products, and satellite
ozone data. The different metrics for the circulation have different
properties, especially with regards to the vertical autocorrelation. In the
model, the different residual circulation metrics agree closely and are well
correlated with the global diabatic circulation, except in the lowermost
stratosphere. In the reanalysis products, however, there are more differences
throughout, indicating the dynamical inconsistencies of these products. The
vertical velocity derived from the time series of water vapor in the tropics
is significantly correlated with the global diabatic circulation, but this
relationship is not as strong as that between the global diabatic circulation
and the residual circulation vertical velocity. We find that the global
diabatic circulation in the lower to middle stratosphere (up to 500 K) is
correlated with the total column ozone in the high latitudes and in the
tropics. The upper-level circulation is also correlated with the total column
ozone, primarily in the subtropics, and we show that this is due to the
correlation of both the circulation and the ozone with upper-level
temperatures.