Abstract
Gravity wave temperature amplitudes will increase upward into the middle atmosphere due to decreasing ambient density and will grow rapidly approaching a critical level. Waves will break when their amplitudes are so large that they become convectively unstable. Above the breaking level turbulence will mix tracers in the vertical and the mean flow will accelerate toward the phase speed of the wave as the wave is absorbed. A parameterization of these effects is employed in a two dimensional model of the middle atmosphere. Results from this coupled dynamical-radiative-photochemical model are used to review the effects of breaking gravity waves on the mean circulation and on the meridional distribution of trace species.
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© 1987 D. Reidel Publishing Company, Dordrecht, Holand.
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Brasseur, G., Hitchman, M. (1987). The Effect of Breaking Gravity Waves on the Distribution of Trace Species in the Middle Atmosphere. In: Visconti, G., Garcia, R. (eds) Transport Processes in the Middle Atmosphere. NATO ASI Series, vol 213. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3973-8_15
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DOI: https://doi.org/10.1007/978-94-009-3973-8_15
Publisher Name: Springer, Dordrecht
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