Version 38 (modified by 10 years ago) ( diff ) | ,
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Stampede Statistics Page, for keeping track of production runs.
Scales:
!================================================================================ ! Description of various scaling parameters ! Define lScale and one of [nScale, rScale], and one of [TimeScale, TempScale, or pScale]. Other combinations are possible - as long as the \ scales are consistent with each other. !================================================================================ nScale = 0d0, ! number density scale parameter [particles/cc] rScale = 1d0, ! density scale [g/cc] TimeScale = 0d0, ! time scale [s] (day=8.64d4, yr=3.1556926d7 TempScale = 0d0, ! temperature scale parameter [Kelvin] pScale = 1d0, ! pressure scale [dynes/cm^2] lScale = 1d0, ! length scale parameter [cm] (AU=1.49598e13, pc=3.08568025e18, R_sun=6.955e10
2D Simulations
Summary
Summary
List of simulations
Thickness | MinDensity or | Completed as of 04-20 | ||
10 | 20 | 0.01 | 1d-10 | Frame 184 |
0.03 | 0.01, after frame 90 | Frame 101 | ||
0.06 | 0.01, after frame 110 | Frame 110 | ||
3 | 0.01 | 0.01 | X | |
0.03 | 0.01 | X | ||
0.06 | 0.01 | X | ||
0.1 | 20 | 0.01 | 1d-10 | Yes |
0.03 | 0.01, after frame 45 | Frame 58 | ||
Hydro | 20 | 0.01 | 1d-10 | Yes |
0.03 | 1d-10 | Yes | ||
0.06 | 1d-10 | Yes | ||
Total No. | 11 |
Parameters in .data files
- In physics.data the MinDensity has been changed for some of the slower runs. I have denoted above where I change the minimum density during the time of the simulation.
- Three of the simulations are hydro, so we simply turn off the MHD in physics.data.
- Three of the simulations have a Mach No. = 3. So we multiply the final_time = .02d0 of the Mach No. = 20 simulations by the ratio of the mach numbers, (20/3), to get a new final_time = 1.33d0 for these Mach No. = 3 simulations.
Here is the problem.data for these simulations:
&ProblemData spacing=.2 ! Lattice constant thickness=0.01 ! Radius of wire: 0.01, 0.03, 0.06 beta=10 ! magnetic beta: 0.1, 10 mach=20 ! mach number: 3, 20 screen_x=.25 ! location of screen in x rho_wire=1000d0 ! peak density of screen rho_wind=1d0 ! density of wind rho_amb=.01 ! ambient density /
Note that the values of thickness, beta, and mach, are listed in the comment.
Here is a copy of the space parameters in the global.data:
&GlobalData !============================================================================================= ! Parameters Related to Space !============================================================================================= nDim = 2 ! number of dimensions for this problem (1-3) GmX = 3200,160,160 ! Base grid resolution [x,y,z] MaxLevel = 1 ! Maximum level for this simulation (0 is fixed grid) LastStaticLevel = -1 ! Use static AMR for levels through LastStaticLevel [-1] GxBounds = 0d0,0d0,0d0,4d0,.2d0,.2d0 ! Problem boundaries in computational units,format: ! (xlower, ylower, zlower, xupper, yupper, zupper) ! For 2D problems, set zlower and zupper to 0.d0. Gmthbc = 1,2,2,1,2,2 ! Sets the physical boundary conditions at the edge of the problem domain ! format: (x1, y1, z1, x2, y2, z2) ! 1-Extrapolated, ! 2-Periodic, ! 3-ReflectingWall (Field lines do not penetrate) ! 4-Reflect_BParallel (Field lines held normal ! 5-Reflect_Cylindrical (Like reflect wall, but also changes sign of phi ! components of velocity and magnetic fields) ! [1,1,1,1,1,1]
In summary we have 11 2D simulations with 1 level of AMR with periodic boundary conditions. Thus we can visualize the simulations used the replicate operator in Visit. We expect the simulation box to be very long and thin given the GxBounds. There is a high level for the base grid resolution — given approximately half a million cells in the base grid. So these jobs, despite being 2D, are high resolution.
Visualizations (Table)
Visualizations (Table)
- Replicate vectors: X = {1, 0, 0}, Y = {0, 0.2, 0}, Z = {0, 0, 1}.
- Replications in X = Replications in Z = 1, Replications in Y = 13.
- Merged into one block when possible.
- Using Log scale, with minimum = 0.01, maximum = 1000.
- Color table used is hot_desaturated.
MHD
Beta | Ma | Last Frame Completed | Picture at Final Frame | GIF | Notes, Questions, Observations |
0.1 | 20 | 200 | GIF | - Strong magnetic pressure - "Clumps" seem to grow in density over the evolution of the simulation. Starting with a wire radius of 0.01, it clearly grows to a larger radius (~0.03 cm). This seems to start once the clump moves past x = 0.6 cm. - The clumps get pushed back incredibly far. Starting at , ending at . Perhaps this is due to the high magnetic pressure. - A low density region forms behind the clump at around x = 0.7 cm. - Unclear when the clump stops accreting. | , wire radius, i.e. thickness = 0.01, Ma = 20
10 | 20 | 200 | GIF | - Weak magnetic pressure | , thickness = 0.01, Ma = 20
10 | 20 | 110 | GIF | - Weak magnetic pressure | , thickness = 0.06, Ma = 20
Note: Mach 3 runs to be posted soon (04-22-2014)
Hydro
Ma | Last Frame Completed | Picture at Final Frame (200) | GIF | Notes, Questions, Observations |
20 | 200 | GIF | - Hydro (MHD off), thickness = 0.01, Ma = 20 - Clump seems to end at position | |
20 | 200 | GIF | - Hydro (MHD off), thickness = 0.03, Ma = 20 - Clump seems to end at position | |
20 | 200 | GIF | - Hydro (MHD off), thickness = 0.06, Ma = 20 - Clump seems to end at position - At - x = 0.3cm, the clump seems to "flatten" — not sure if this is physical, to be expected, or a problem with the code. |
3D Simulations — Production Runs
Summary
&ProblemData spacing=1 ! Lattice constant thickness=.125 ! Radius of wire beta=10 ! magnetic beta mach=20 ! mach number screen_x=1.25 ! location of screen in x rho_wire=1000d0 ! peak density of screen rho_wind=1d0 ! density of wind rho_amb=.01 ! ambient density omega = 1 ! cycles per wind crossing time per lattice spacing amplitude=.00 ! fraction of wind velocity offset = 0,.5,.5 thickness2=.0625 /
MinDensity = 1d-3 ! Minimum computational density before protection is triggered [1d-10]
For hydro run we have no magnetic fields, so lMHD is set to false:
lMHD = .false. ! Magnetic Fields present? [.false.]
nDim = 3 ! number of dimensions for this problem (1-3) GmX = 1600,160,160 ! Base grid resolution [x,y,z] MaxLevel = 2 ! Maximum level for this simulation (0 is fixed grid) LastStaticLevel = -1 ! Use static AMR for levels through LastStaticLevel [-1] GxBounds = 0d0,0d0,0d0,10d0,1d0,1d0 ! Problem boundaries in computational units,format: ! (xlower, ylower, zlower, xupper, yupper, zupper) ! For 2D problems, set zlower and zupper to 0.d0. Gmthbc = 1,2,2,1,2,2 ! Sets the physical boundary conditions at the edge of the problem domain ! format: (x1, y1, z1, x2, y2, z2) ! 1-Extrapolated, ! 2-Periodic, ! 3-ReflectingWall (Field lines do not penetrate) ! 4-Reflect_BParallel (Field lines held normal ! 5-Reflect_Cylindrical (Like reflect wall, but also changes sign of phi ! components of velocity and magnetic fields) ! [1,1,1,1,1,1]
final_time = 1d0 ! The final time in computational units. final_frame = 200 ! The final frame [10]
Attachments (44)
- b10_thickp01_mach3long0200.png (30.8 KB ) - added by 10 years ago.
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