This presentation shares a collection of findings and insights from recent Ph.D. work focused on modeling acoustic and gravity wave propagation and their evolution in the thermosphere. A high-resolution, finite-volume simulation framework is introduced, based on the multi-component Navier–Stokes equations, and designed to resolve the transport of energy, momentum, and mass in neutral planetary atmospheres. The model captures nonlinear wave dynamics and includes detailed transport processes such as species-dependent diffusion, viscosity, and thermal conduction. The talk will discuss results from 1D and 2D simulations, the role of transport coefficients in wave dissipation, and the challenges of bridging high-fidelity simulations with large-scale atmospheric models. The goal is to offer perspective on small-scale wave dynamics in the thermosphere and encourage discussion across modeling approaches, including those used in global circulation models such as WACCM.