Related Experiment Video
Updated: Feb 4, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
Oscillatory instability in a reaction front separating fluids of different densities
Dan Coroian1, Desiderio A Vasquez2,3
1Department of Mathematical Sciences, Purdue University Fort Wayne, Fort Wayne, Indiana 46805, USA.
Abstract:
Reaction fronts described by the Kuramoto-Sivashinsky (KS) equation can exhibit complex behavior as they separate reacted from unreacted fluids. If the fluid of higher density is above a fluid of lower density, then the Rayleigh-Taylor instability can lead to fluid motion. In the reverse situation, where the lighter fluid is on top, gravitationally driven forces can stabilize a convectionless flat front inhibiting the complex front propagation described by the KS equation. In these cases, a critical density difference is required to provide stability to the flat front. A linear stability analysis shows that the transition from stable to unstable flat fronts can be oscillatory for viscous fluid motion. Once the transition takes place, the fronts exhibit oscillatory convection resulting in oscillations of the shape and speed of the front.
Related Concept Videos
Microtubule Instability
Density, Specific Weight, Specific Gravity and Compressibility of Fluid
Specific weight represents the weight per unit volume and is calculated by multiplying...
The Fluid Mosaic Model
Density
Precipitation Reactions
Current Density

