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We now consider the effect of a uniform magnetic field that is aligned
with the velocity field at the inflow to flow past a cylinder. We have
already verified that the incompressible code obtains the correct
answer for the case without magnetic field. This provides us with a
baseline for comparison. The farfield boundary conditions are
straightforward to provide for the magnetic streamfunction. The
condition at the wall was chosen (somewhat arbitrarily) so that the
magnetic streamfunction is set to zero there. This condition sets the
normal component of the magnetic field to zero at the cylinder. A
summary of the simulation parameters is given in table
6.4.
Table 6.4:
Simulation parameters for incompressible MHD flow past a cylinder.
| Parameter |
Value |
| Dimension |
2d |
| Sv |
100 |
| Sr |
100 |
| VA |
0.1 |
 |
0.005 |
| N-Range |
10 |
| KTri |
460 |
| Method |
Galerkin |
Figure 6.6:
Incompressible flow past a cylinder with inflow magnetic fields. From the top: (1) x component of the velocity field, (2) y component of the velocity field, (3) x component of the magnetic field, (4) y component of the magnetic field
 |
The instantaneous primitive variable fields are shown in figures
6.6 and 6.7. We see
from figure 6.7 that the shedding pattern at
the cylinder is only slightly perturbed but that the vortex street has
been destabilized downstream from the cylinder. The wake has also
become more complicated with more small scale structures appearing
than before.
Figure 6.7:
Incompressible flow past a cylinder with inflow magnetic fields aligned with inflow velocity. Top: Pressure field, Middle: Vorticity, Lower: Stream function of the magnetic field
 |
Next: Compressible Flow Simulations
Up: Incompressible Viscous Magnetohydrodynamics
Previous: Orszag-Tang Vortex
T. Warburton
10/24/1998