The quasi‐biennial oscillation: Analysis using ERA‐40 data

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Solar cycle variation of stratospheric ozone: Multiple regression analysis of long‐term satellite data sets and comparisons with models (2006, background): “In support of this possibility, some statistical evidence for an apparent minor dependence of certain properties of the QBO on the 11-year solar cycle has been reported [Salby and Callaghan, 2000; Soukharev and Hood, 2001; Pascoe et al., 2005; see also Hamilton, 2002].”
High‐latitude influence of the quasi‐biennial oscillation (2014, methodology): “E composite differences at the Equator yield a peak-to-peak QBO strength of 30 m s−1 at 23 km, 25 m s−1 at 35 km, and 10 m s−1 at 48 km (Pascoe et al., 2005).”
Characterization of the 11-Year Solar Signal Using a Multiple Regression Analysis of the ERA-40 Dataset (2005, background): “A comprehensive description of the QBO signal in the ERA-40 dataset is provided by Pascoe et al. (2005). In addition to the maximum signal over the equator, there are smaller QBO temperature components present at higher latitudes (20°–50°) of each hemisphere associated with the QBO-induced meridiona”
SOLAR INFLUENCES ON CLIMATE (2010, unknown): “However, it is still not clear to which factor (SSTs, time‐varying solar cycle, or inclusion of a QBO) the improvements can be ascribed.”