Nonlinear evolution of internal gravity waves in the Earth's ionosphere: Analytical and numerical approach
T. D. Kaladze, A. P. Misra, A. Roy, D. Chatterjee

TL;DR
This paper investigates the nonlinear behavior of internal gravity waves in the Earth's ionosphere, revealing how magnetic fields and conductivity influence vortex formation, stability, and energy dissipation through analytical and numerical methods.
Contribution
It advances existing theory by incorporating magnetic field effects and analyzes vortex dynamics and energy loss mechanisms in the ionosphere.
Findings
Formation of solitary dipolar vortices supported by ionospheric fluids.
Vortex structures can move supersonically without energy loss in absence of Pedersen conductivity.
Presence of Pedersen conductivity causes decay and potential disappearance of vortices.
Abstract
The nonlinear propagation of internal gravity waves in the weakly ionized, incompressible Earth's ionosphere is studied using the fluid theory approach. Previous theory in the literature is advanced by the effects of the terrestrial inhomogeneous magnetic field embedded in weakly ionized ionospheric layers ranging in altitude from about to km. It is shown that the ionospheric conducting fluids can support the formation of solitary dipolar vortices (or modons). Both analytical and numerical solutions of the latter are obtained and analyzed. It is found that in absence of the Pedersen conductivity, different vortex structures with different space localization can be formed which can move with the supersonic velocity without any energy loss. However, its presence can cause the amplitude of the solitary vortices to decay with time and the vortex structure can completely disappear…
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