Author(s)

Bing Wang¹, Jing-Song Bai^1,2, Tao Wang¹

¹Institute of Fluid Physics, China Academy of Engineering Physics, Mianyang, China.
²National Key Laboratory of Shock Wave and Detonation Physics, Institute of Fluid Physics, China Academy of Engineering Physics, Mianyang, China.

A detailed numerical simulation of a shock accelerated heavy gas (SF₆) cylinder surrounded by air gas is presented. It is a simplified configuration of the more general shock-accelerated inhomogeneous flows which occur in a wide variety of astrophysical systems. From the snapshots of the time evolution of the gas cylinder, we find that the evolution of the shock accelerated gas cylinder is in some ways similar to the roll-ups of a vortex sheet for both roll up into a spiral and fall into a self-similar behavior. The systemic and meaningful analyses of the negative circulation, the center of vorticity and the vortex spacing are in a good agreement with results obtained from the prediction of vorticity dynamics. Unlike the mixing zone width in single-mode or multi-mode Richtmyer-Meshkov instability which doesn’t exist, a single power law of time owing to the bubble and spike fronts follow a power law of t^θ with different power exponents, the normalized length of the shock accelerated gas cylinder follows a single power law with θ = 0.43 in its self-similar regime obtained from the numerical results.

Interficial Instabilities, Vortex Dynamics, Power Laws

Wang, B. , Bai, J. and Wang, T. (2015) Numerical Investigation of a Shock Accelerated Heavy Gas Cylinder in the Self-Similar Regime. International Journal of Astronomy and Astrophysics, 5, 38-46. doi: 10.4236/ijaa.2015.51006.