The gravity wave response above deep convection in a squall line simulation

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Abstract

High-frequency gravity waves generated by convective storms likely play an important role in the general circulation of the middle atmosphere. This work utilizes a fully compressible, nonlinear, numerical, two-dimensional simulation of a midlatitude squall line to study vertically propagating waves generated by deep convection. The model includes a deep stratosphere layer with high enough resolution to characterize the wave motions at these altitudes. A spectral analysis of the stratospheric waves provides an understanding of the necessary characteristics of the spectrum for future studies of their effects on the middle atmosphere in realistic mean wind scenarios. The wave spectrum also displays specific characteristics that point to the physical mechanisms within the storm responsible for their forcing. -from Authors

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Alexander, M. J., Holton, J. R., & Durran, D. R. (1995). The gravity wave response above deep convection in a squall line simulation. Journal of the Atmospheric Sciences, 52(12), 2212–2226. https://doi.org/10.1175/1520-0469(1995)052<2212:TGWRAD>2.0.CO;2

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