Quasi-biennial oscillations of ozone and diabatic circulation in the equatorial stratosphere

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Abstract

The quasi-biennial oscillation (QBO) in ozone in the equatorial stratosphere is obtain by analyzing the Stratospheric Aerosol and Gas Experiment (SAGE) data from 1984 to 1989. The phase of the ozone QBO in the lower stratosphere is found to precede the zonal wind QBO by several months as opposed to the theoretically expected in-phase relationship between the two. A mechanistics model is developed to explore possible reasons for this disagreement. The model is capable of simulating the actual time evolution of the ozone QBO by introducing the observed zonal wind profile as input. The modeled results confirm the conventional view that the ozone QBO is generated by the vertical ozone advection that is driven to maintain the temperature structure against radiative damping. However, a series of experiments emphasizes the importance of the feedback of the ozone QBO to the diabatic heating through the absorption of solar radiation. -from Author

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Hasebe, F. (1994). Quasi-biennial oscillations of ozone and diabatic circulation in the equatorial stratosphere. Journal of the Atmospheric Sciences, 51(5), 729–745. https://doi.org/10.1175/1520-0469(1994)051<0729:QBOOOA>2.0.CO;2

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