![]() |
Research School of Astronomy and Astrophysics
Fyris Alpha Simulation Code
|
![]() |
2D Kelvin -Helmholtz TestThis test consists of a dense central layer moving with respect to a lower density layer above and below the dense layer. Using periodiuc boundaries on all sides, a steady state can be established. Noise is added to the dense layer velocity field at the 1% level to seed the Kelvin-Helmholtz instability (KH instability). There is not an analysitcal solution, but the growth of the Y component of the kinetic energy grows in essentially the same fashon as the test performed by the ATHENA code: (http://www.astro.princeton.edu/~jstone/tests/kh/kh.html). There is a brief settling period, followed by exponential growth and finally saturation. The three resolutions excite increasing maximum wavenumber modes, and the higher wavenumebr modes grow more quickly than the lower wavnumber modes, as expected. Initial Conditions:
Grid:
Algorithm Settings:
Ending Condition:
ResultsY-Axis Kinetic energy 0.5*d*v_y^2QuickTime Movies
128 x 128 cells
256 x 256 cells
512 x 512 cells
|
![]() |
Page last updated: Wednesday, 19-May-2010 13:56:28 AEST Please direct all enquiries to: Ralph.Sutherland@anu.edu.au Page authorised by: Ralph Sutherland |
The Australian National University CRICOS Provider Number 00120C — ABN: 522 34063906 |