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Home › WOMBAT - Astrophysical Fluid Code › Code Tests ›

Rayleigh-Taylor Instability

Submitted by peter on Fri, 09/25/2009 - 12:20

Introduction
The Rayleigh-Taylor instability shown here is caused when a heavy fluid sits on top of a lighter fluid in the presence of gravity. A small perturbation to the interface of these two fluids will start the growth of the instability.

ρ top = 2
ρ bottom = 1
Pgas = 2.5
Gravity = 0.1

2-d Tests

Hydro

The movie below shows a single mode perturbation.

MHD

β = 2 * Pgas/ B 2

The simulation below shows the single mode MHD case with β = 500. In this case Kelvin-Helmholtz instabilities present in the hydro version are smoothed out by the magnetic field.

The simulation below shows the single mode MHD case with β = 125. In this case the magnetic field is strong enough to prevent the instability from developing.

3-d Tests

‹ Orszag-Tang Vortex up Relativistic MHD Tests ›

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University of Minnesota :: Minnesota Institute of Astrophysics
Contact :: Tom Jones :: twj@msi.umn.edu