The Richtmyer-Meshkov instabilityoccurs when two fluids of differing density are hit by ashock wave. The animation above shows a cylinder of denser gas (white) in still air (black) before being hit with a Mach 1.2 shock wave. The cylinder is quickly accelerated and flattened, with either end spinning up to form the counter-rotatingvorticesthat dominate the instability. As the vortices spin, the fluids along the interface shear against one another, and new, secondary instabilities, like the wave-likeKelvin-Helmholtz instability, form along the edges. The two gases mix quickly. This instability is of especial interest for the application ofinertial confinement fusion. During implosion, the shell material surrounding the fuel layer is shock-accelerated; since mixing of the shell and fuel is undesirable, researchers are interested in understanding how to control and prevent the instability. (Image credit:S. Shankar et al.)
The APS Division of Fluid Dynamics conference begins this Sunday in Pittsburgh. I’ll be giving a talk about FYFDSunday evening at 5:37pm in Rm 306/307. I hope to see some of you there!