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

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 …

Improvements of the mixing-length theory (MLT) of turbulent convection in stellar
atmospheres are developed theoretically. It is pointed out that inaccuracies are introduced …

We present a self-consistent model for stellar turbulent convection that is similar in spirit to
the CM model (Canuto & Mazzitelli 1991) since it accounts for the full spectrum of the …

We consider the effect of viscosity on Rayleigh-Taylor (RT) and Richtmyer-Meshkov (RM)
instabilities by deriving a moment equation for fluids with arbitrary density and viscosity …

An experimental and numerical systematic study of the growth of the Richtmyer–Meshkov
instability-induced mixing following a re-shock is made, where the initial shock moves from …

Abstract We apply the Canuto-Goldman (CG) analytical model to turbulence generated by
the class of instabilities which have a power-law growth rate. For the case of Rayleigh-Taylor …

The existence of universal power laws at low wavenumbers (K) in the energy spectrum (E u)
of the turbulent longitudinal velocity (u) is examined theoretically and experimentally for the …

A review of the literature on natural convection in a horizontal layer heated from below
shows the need for reliable data at high Rayleigh number (Ra) to determine the asymptotic …

We study the shock-driven turbulent mixing that occurs when a perturbed planar density
interface is impacted by a planar shock wave of moderate strength and subsequently …