Thermally forced gravity waves in an atmosphere at rest

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Abstract

For the rigid lid solution, vertically trapped gravity waves propagate away from the source with a speed that depends on the Brunt-Vaisala frequency and the vertical wavenumber of the heating. The amplitude of the disturbance field in the region of the forcing approaches a constant value. Two modes are of particular interest: 1) a deep fast-moving mode which is responsible for subsidence warming through the depth of the troposphere; 2) a slower moving mode which corresponds to midlevel inflow and lower- and upper-level outflows. A solution is also obtained for a semi-infinite region. Although gravity wave energy can now propagate upward, the structure of the low-level fields still shows many similarities with the rigid lid solution. -from Authors

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Nicholls, M. E., Pielke, R. A., & Cotton, W. R. (1991). Thermally forced gravity waves in an atmosphere at rest. Journal of the Atmospheric Sciences, 48(16), 1869–1884. https://doi.org/10.1175/1520-0469(1991)048<1869:TFGWIA>2.0.CO;2

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