2D AD Magnetohydrodynamic Blast Wave - SFG-CUHK/scorpio-test-cases GitHub Wiki
Two-fluid MHD was introduced by Tilley & Balsara (2008) with isothermal two-fluid MHD, and the adiabatic version in Tilley, Balsara & Meyer (2012). It studied the behavior of the spherical blast wave triggered by the high uniform density region within a radius and propagate radially outward. Below are the initial conditions of the simulation setting.
| Parameter | Setting | Parameter | Setting |
|---|---|---|---|
|
|
[0.1 x 0.1] |
|
400 |
| 5/3 | 1.4 | ||
| 0.0126 | 0.00126 | ||
| 10 | 0.1 | ||
| 4347.8 | 4.3478 | ||
| 0.43478 | 4.3478 x 10-4 | ||
| 29.0 | 2.3 | ||
| 0.1 | 3.5468 x 10 -2 | ||
|
|
0 | ||
| CFL |
0.2 | CFL |
0.2 |
| Solver |
HLLMHD | Solver |
HLLCHD |
| 0.006 |
Below is the output of the code. Figure 1 shows the density of ions (left) and neutrals (right). Figure 2 shows the cross-section along the x-direction of density (left) and velocity (right) of the two types of fluids. Similar result compares with Figure 5 & Figure 6 (c, f) of Tilley, Balsara & Meyer (2012).
Figure 1. Result of the 2D AD MHD blast wave, simulated with Scorpio.
Figure 2. Result of the 2D AD MHD blast wave, simulated with Scorpio.