Time evolution of density perturbations in accelerating stratified fluids
- 1 September 1983
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review A
- Vol. 28 (3) , 1637-1646
- https://doi.org/10.1103/physreva.28.1637
Abstract
We consider superimposed fluids, having arbitary initial perturbations at their interfaces, undergoing a Rayleigh-Taylor instability with constant acceleration. The time evolution of these perturbations is described by a sum over normal modes and in general is a combination of oscillation and exponential rise. We derive the equation governing their growth, discuss the case analytically, and give two numerical examples where we plot the time evolution of the perturbations at the four interfaces of five superimposed fluids. Our examples illustrate how the evolution depends on the density profile, on the wavelength of the perturbations, and on the initial conditions.
Keywords
This publication has 16 references indexed in Scilit:
- Rayleigh-Taylor and Kelvin-Helmholtz Instabilities in Targets Accelerated by Laser AblationPhysical Review Letters, 1982
- Effect of long internal waves on the evolution of deep-water surface gravity wavesPhysics of Fluids, 1982
- Sunspots and the physics of magnetic flux tubes. X - On the hydrodynamic instability of buoyant fieldsThe Astrophysical Journal, 1980
- Theory of Rayleigh‐Taylor bubbles in the equatorial ionosphereJournal of Geophysical Research, 1978
- Two-Dimensional Simulation of Fluid Instability in Laser-Fusion PelletsPhysical Review Letters, 1975
- On the interaction of internal waves and surface gravity wavesJournal of Fluid Mechanics, 1974
- Laser-driven fusionReviews of Modern Physics, 1974
- Equatorial spreadF: Recent observations and a new interpretationJournal of Geophysical Research, 1972
- Laser Compression of Matter to Super-High Densities: Thermonuclear (CTR) ApplicationsNature, 1972
- The instability of liquid surfaces when accelerated in a direction perpendicular to their planes. IProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1950