As an illustration of the model's capability we show a sample calculation of a gravity
current in a straight-channel. The channel is occupied by two fluids whose density interface
is initially vertical. As the heavy fluid slumps under the lighter one, Kelvin-Helmholtz rolls
develop at the density and lead to vigorous mixing of the two fluids. For more details on the
equations and expected behavior see for example Ã
Tamay M. Ozgokmen, and Eric P. Chassignet,
Dynamics of Two-Dimensional Turbulent Bottom Gravity Currents
Journal of Physical Oceanography 2002 32 No 5: 1460-1478. The parameters for this
simulation include a Prandtl number of 7 and Reynolds number of 10,0000 based on the aforementioned
reference's definitions. There are 128x25 elements in the x-z directions using 14-th degree polynomials for the streamfunction and vorticity and 13-th degree
polynomials for the density field. The two images below show high resolution snapshot of the density distribution before and after hitting the side-wall.
Click
here to see a cool low resolution (but nevertheless 87 MB) movie of the gravity current.
Hi resolution image of density front prior to hitting the side-walls.
Hi resolution image of density front after hitting the side-walls.