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Cylinder Flow

 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
$\Delta t$ 0.005
N-Range 10
KTri 460
Method Galerkin


\begin{figure}
\centerline{
\psfig {file=/crunch/crunch7/tcew/Thesis/Figures1/Ep...
 ...runch7/tcew/Thesis/Figures1/Eps/mhd1.yvel.inc.bw.eps,width=4.50in}
}\end{figure}

  
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
\begin{figure}
\centerline{
\psfig {file=/crunch/crunch7/tcew/Thesis/Figures1/Ep...
 .../crunch7/tcew/Thesis/Figures1/Eps/mhd1.By.inc.bw.eps,width=4.50in}
}\end{figure}

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.


\begin{figure}
\centerline{
\psfig {file=/crunch/crunch7/tcew/Thesis/Figures1/Ep...
 ...runch7/tcew/Thesis/Figures1/Eps/mhd1.vort.inc.bw.eps,width=4.50in}
}\end{figure}

  
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
\begin{figure}
\centerline{
\psfig {file=/crunch/crunch7/tcew/Thesis/Figures1/Eps/mhd1.magstream.inc.bw.eps,width=4.5in}
}\end{figure}


next up previous contents
Next: Compressible Flow Simulations Up: Incompressible Viscous Magnetohydrodynamics Previous: Orszag-Tang Vortex
T. Warburton
10/24/1998