Hydrodynamic instabilities such as Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM)
instabilities usually appear in conjunction with the Kelvin–Helmholtz (KH) instability and are …

Abstract Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM) instabilities are well-known
pathways towards turbulent mixing layers, in many cases characterized by significant mass …

In diverse areas of science and technology, including inertial confinement fusion (ICF),
astrophysics, geophysics, and engineering processes, turbulent mixing induced by …

We present an approach for compressing volumetric scalar fields using implicit neural
representations. Our approach represents a scalar field as a learned function, wherein a …

Spontaneous mixing of fluids at unstably stratified interfaces occurs in a wide variety of
atmospheric, oceanic, geophysical and astrophysical flows. The Rayleigh–Taylor instability …

Basic fluid equations are the main ingredient in the development of theories of Rayleigh–
Taylor buoyancy-induced instability. Turbulence arises in the late stage of the instability …

An alternative methodology is described for large-eddy simulation (LES) of flows involving
shocks, turbulence, and mixing. In lieu of filtering the governing equations, it is postulated …

This paper investigates the influence of different three-dimensional multi-mode initial
conditions on the rate of growth of a mixing layer initiated via a Richtmyer–Meshkov …

When a heavy fluid is placed above a light fluid, tiny vertical perturbations in the interface
create a characteristic structure of rising bubbles and falling spikes known as Rayleigh …

We present a model describing the evolution of Fanaroff–Riley type I and II radio active
galactic nuclei (AGNs) and the transition between these classes. We quantify galactic …