Influence of temperature-dependent density inhomogeneity on the stability of atmospheric stratified fluids

Abstract

The stability of atmospheric stratified fluids is revisited to study the influence of the temperature-dependent density inhomogeneity due to thermal expansion in the Earth's lower atmosphere (with heights $0$ to $50$ km) under the action of gravity. Previous theory in the literature [Phys. Lett. A 480 (2023) 128990] is modified and advanced. It is found that the Brunt-V{ä}is{ä}l{ä} frequency associated with internal gravity waves is modified, leading to new instability conditions of vertically stratified fluids. The possibility of the onset of Rayleigh-B{é}nard convective instability is also discussed, and the influences of the modified Brunt-V{ä}is{ä}l{ä} frequency and the density and temperature gradients on the instability growth rates are studied.

9 pages, 3 figures; added discussions in Sec. VI; This version is to appear in Physica Scripta (2024)

References in corpus (3)

• Internal wave coupling processes in Earth's atmosphere
• Semi-organized structures and turbulence in the atmospheric convection
• Thermal expansion of atmosphere and stability of vertically stratified fluids

Cited by in corpus (2)

• Analytical and Numerical Linear Analyses of Convection Revisited
• Rayleigh-Bénard convective motion of stratified fluids in the Earth's troposphere