The response of the lower stratosphere to zonally symmetric thermal and mechanical forcing.
Journal of the Atmospheric Sciences
American Meteorological Society
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Ming, A., Hitchcock, A., & Haynes, P. (2016). The response of the lower stratosphere to zonally symmetric thermal and mechanical forcing.. Journal of the Atmospheric Sciences https://doi.org/10.1175/JAS-D-15-0294.1
The response of the atmosphere to zonally symmetric applied heating and mechanical forcing is considered, allowing for the fact that the response may include a change in the wave force (or ‘wave drag’). A scaling argument shows that an applied zonally symmetric heating is effective in driving a steady meridional circulation provided that the wave force (required to satisfy angular momentum constraints) is sufficiently sensitive to changes in the mean flow in the sense that the ratio KN²D ² _(Q) /α f ²L ² _Q is large, where K is a measure of the sensitivity of the wave force, α, N, and f are respectively the radiative damping rate, buoyancy frequency, and Coriolis parameter and L_Q and D_Q are respectively the horizontal and vertical length scales of the heating. Furthermore in the ‘narrow heating’ regime where this ratio is large, the structure of the meridional circulation response is only weakly dependent on the details of the wave force. The scaling arguments are verified by experiments in a dry dynamical circulation model. Consistent with the scaling prediction, the regime does not apply when the width of the imposed heating is increased. The narrow heating regime is demonstrated to be relevant to the double peak in tropical lower stratospheric upwelling considered in a companion paper, supporting the hypothesis that this feature is radiatively driven. Similar arguments are applied to show that a narrow zonally symmetric applied mechanical forcing is primarily balanced by a change in wave force. This provides an explanation for the recently identified compensation between resolved and parametrized waves in driving modelled trends in the Brewer-Dobson circulation.
The authors thank Amanda Maycock for help with the radiation code and for helpful discussions. AM and PHi acknowledge funding support from the European Research Council through the ACCI project (grant number 267760) lead by John Pyle. PHi also acknowledges support from an NSERC postdoctoral fellowship. The authors are grateful to Stephan Fueglistaler and Tom Flannaghan for conversations that stimulated some of this work. We also thank Robin Hogan, Alessio Bozzo and Irina Sandu from ECMWF for their help with reproducing the longwave heating rates as well as Ulrike Langematz and Markus Kunze for the ozone climatology. We received detailed and helpful comments from three anonymous reviewers that improved this manuscript.
European Research Council (267760)
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External DOI: https://doi.org/10.1175/JAS-D-15-0294.1
This record's URL: https://www.repository.cam.ac.uk/handle/1810/253869