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

The Liapunov method for establishing stability has been used in a variety of fluid and
plasma problems. For nondissipative systems, this stability method is related to well-known …

The theory of the Rayleigh-Taylor instability of accelerated fluid layers is systematically
developed from basic fluid equations. Starting with the classical potential flow theory for …

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

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 …

A" z-pinch" is a deceptively simple plasma configuration in which a longitudinal current
produces a magnetic field that tends to confine the plasma. The simple geometry and low …

The Rayleigh–Taylor instability, which occurs due to the gravitational instability of a heavy
fluid overlying a lighter fluid, 1, 2 is of fundamental importance in a multitude of applications …

We present a tentative review of compressibility effects in Rayleigh–Taylor instability-
induced flows. The linear, nonlinear and turbulent regimes are considered. We first make the …

Solar prominences are formed by partially ionized plasma with inter-particle collision
frequencies generally warranting magnetohydrodynamic treatment. In this work we explore …

Solar prominences are formed by partially ionized plasma with inter-particle collision
frequencies, which generally warrant magnetohydrodynamic treatment. In this work, we …