2023/10/02 by T. Faran, Christopher D. Matzner, Faran, Tamar +3
Earth and Planetary Sciences · Physics and Astronomy · #Astro and Planetary Science #Atmospheric and Oceanic Physics (physics.ao-ph) #FOS: Physical sciences #Fluid Dynamics (physics.flu-dyn) #Geophysics and Gravity Measurements #High Energy Astrophysical Phenomena (astro-ph.HE) #Solar and Space Plasma Dynamics
paper · pdf · doi:10.48550/arxiv.2310.01481
openalex publication_date 2023/10/02 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Nonlinear acoustic evolution is often discussed in the context of wave-steepening that leads to shock formation, and is of special interest in applications where the shock continues to strengthen due to a narrowing of its channel or the stratification of the medium. Accurate scalings govern low amplitude waves and strong shocks, but connecting these phases, or describing waves that are nonlinear from the outset, generally requires simulation. We address this problem using the fact that waves within a plane-parallel, isentropic and gravitationally stratified atmosphere are described by exact simple-wave solutions, thanks to the conservation of Riemann invariants in a freely falling reference frame. Our solutions enable us to discriminate waves that reflect from those that form shocks, and to capture wave and shock evolution using an ordinary differential equation. For several relevant values of the adiabatic index γ the solutions are explicit; furthermore, nonlinear wave reflection from a free surface can be described analytically for γ=3. Comparison to hydrodynamic simulations shows that our analytic shock approximation is accurate up to moderate (∼ few--15) Mach numbers, where the accuracy increases with the adiabatic index. Our solutions also imply that an initially subsonic pulse is unable to unbind mass from the atmosphere without significantly increasing its entropy.