xref: /libCEED/examples/fluids/README.md (revision 44e8f77db7594e84476b92f66f596c47c9eec762)
1ccaff030SJeremy L Thompson## libCEED: Navier-Stokes Example
2ccaff030SJeremy L Thompson
3ccaff030SJeremy L ThompsonThis page provides a description of the Navier-Stokes example for the libCEED library, based on PETSc.
4b8962995SJeremy L ThompsonPETSc v3.17 or a development version of PETSc at commit 0e95d842 or later is required.
5ccaff030SJeremy L Thompson
677841947SLeila GhaffariThe Navier-Stokes problem solves the compressible Navier-Stokes equations in three dimensions using an explicit time integration.
777841947SLeila GhaffariThe state variables are mass density, momentum density, and energy density.
8ccaff030SJeremy L Thompson
977841947SLeila GhaffariThe main Navier-Stokes solver for libCEED is defined in [`navierstokes.c`](navierstokes.c) with different problem definitions according to the application of interest.
10ccaff030SJeremy L Thompson
113b219b86SJames Wright## Build instructions
123b219b86SJames Wright
13bc7bbd5dSLeila GhaffariBuild by using:
14ccaff030SJeremy L Thompson
15ccaff030SJeremy L Thompson`make`
16ccaff030SJeremy L Thompson
17bc7bbd5dSLeila Ghaffariand run with:
18ccaff030SJeremy L Thompson
19bc7bbd5dSLeila Ghaffari```
20bc7bbd5dSLeila Ghaffari./navierstokes -ceed [ceed] -problem [problem type] -degree [degree]
21bc7bbd5dSLeila Ghaffari```
22ccaff030SJeremy L Thompson
233b219b86SJames WrightIf you want to do *in situ* machine-learning training, specify `SMARTREDIS_DIR` in the make command like:
243b219b86SJames Wright
253b219b86SJames Wright```
263b219b86SJames Wrightmake SMARTREDIS_DIR=~/software/smartredis/install
273b219b86SJames Wright```
283b219b86SJames Wright
29bc7bbd5dSLeila Ghaffari## Runtime options
30ccaff030SJeremy L Thompson
31bc7bbd5dSLeila Ghaffari% inclusion-fluids-marker
32ccaff030SJeremy L Thompson
33bc7bbd5dSLeila GhaffariThe Navier-Stokes mini-app is controlled via command-line options.
34bc7bbd5dSLeila GhaffariThe following options are common among all problem types:
35ccaff030SJeremy L Thompson
36bc7bbd5dSLeila Ghaffari:::{list-table} Common Runtime Options
37bc7bbd5dSLeila Ghaffari:header-rows: 1
38ccaff030SJeremy L Thompson
39bc7bbd5dSLeila Ghaffari* - Option
40bc7bbd5dSLeila Ghaffari  - Description
41bc7bbd5dSLeila Ghaffari  - Default value
42ccaff030SJeremy L Thompson
43bc7bbd5dSLeila Ghaffari* - `-ceed`
44bc7bbd5dSLeila Ghaffari  - CEED resource specifier
45bc7bbd5dSLeila Ghaffari  - `/cpu/self/opt/blocked`
46ccaff030SJeremy L Thompson
473866774cSJames Wright* - `-test_type`
483866774cSJames Wright  - Run in test mode and specify whether solution (`solver`) or turbulent statistics (`turb_spanstats`) output should be verified
493866774cSJames Wright  - `none`
50ccaff030SJeremy L Thompson
51bc7bbd5dSLeila Ghaffari* - `-compare_final_state_atol`
52bc7bbd5dSLeila Ghaffari  - Test absolute tolerance
53bc7bbd5dSLeila Ghaffari  - `1E-11`
54ccaff030SJeremy L Thompson
55bc7bbd5dSLeila Ghaffari* - `-compare_final_state_filename`
56bc7bbd5dSLeila Ghaffari  - Test filename
57bc7bbd5dSLeila Ghaffari  -
58ccaff030SJeremy L Thompson
59bc7bbd5dSLeila Ghaffari* - `-problem`
609e529eadSJames Wright  - Problem to solve (`advection`, `density_current`, `euler_vortex`, `shocktube`, `blasius`, `channel`, `gaussian_wave`, and `taylor_green`)
61bc7bbd5dSLeila Ghaffari  - `density_current`
62ccaff030SJeremy L Thompson
63bc7bbd5dSLeila Ghaffari* - `-implicit`
649e576805SJames Wright  - Use implicit time integrator formulation
65bc7bbd5dSLeila Ghaffari  -
66ccaff030SJeremy L Thompson
67bc7bbd5dSLeila Ghaffari* - `-degree`
68bc7bbd5dSLeila Ghaffari  - Polynomial degree of tensor product basis (must be >= 1)
69bc7bbd5dSLeila Ghaffari  - `1`
70ccaff030SJeremy L Thompson
712288fb52SJeremy L Thompson* - `-q_extra`
72bc7bbd5dSLeila Ghaffari  - Number of extra quadrature points
73fc14f3f6SLeila Ghaffari  - `0`
74ccaff030SJeremy L Thompson
7537cbb16aSJed Brown* - `-ts_monitor_solution`
7637cbb16aSJed Brown  - PETSc output format, such as `cgns:output-%d.cgns` (requires PETSc `--download-cgns`)
7737cbb16aSJed Brown  -
78ccaff030SJeremy L Thompson
7937cbb16aSJed Brown* - `-ts_monitor_solution_interval`
8037cbb16aSJed Brown  - Number of time steps between visualization output frames.
8137cbb16aSJed Brown  - `1`
8237cbb16aSJed Brown
8337cbb16aSJed Brown* - `-viewer_cgns_batch_size`
8437cbb16aSJed Brown  - Number of frames written per CGNS file if the CGNS file name includes a format specifier (`%d`).
8537cbb16aSJed Brown  - `20`
8637cbb16aSJed Brown
8737cbb16aSJed Brown* - `-checkpoint_interval`
8837cbb16aSJed Brown  - Number of steps between writing binary checkpoints. `0` has no output, `-1` outputs final state only
89bc7bbd5dSLeila Ghaffari  - `10`
90ccaff030SJeremy L Thompson
9137cbb16aSJed Brown* - `-checkpoint_vtk`
9237cbb16aSJed Brown  - Checkpoints include VTK (`*.vtu`) files for visualization. Consider `-ts_monitor_solution`instead.
9337cbb16aSJed Brown  - `false`
9437cbb16aSJed Brown
9537cbb16aSJed Brown* - `-viz_refine`
9637cbb16aSJed Brown  - Use regular refinement for VTK visualization
9737cbb16aSJed Brown  - `0`
9837cbb16aSJed Brown
99bc7bbd5dSLeila Ghaffari* - `-output_dir`
10037cbb16aSJed Brown  - Output directory for binary checkpoints and VTK files (if enabled).
101bc7bbd5dSLeila Ghaffari  - `.`
102ccaff030SJeremy L Thompson
10369293791SJames Wright* - `-output_add_stepnum2bin`
10469293791SJames Wright  - Whether to add step numbers to output binary files
10569293791SJames Wright  - `false`
10669293791SJames Wright
10769293791SJames Wright* - `-continue`
10869293791SJames Wright  - Continue from previous solution (input is step number of previous solution)
10969293791SJames Wright  - `0`
11069293791SJames Wright
11169293791SJames Wright* - `-continue_filename`
11269293791SJames Wright  - Path to solution binary file from which to continue from
11369293791SJames Wright  - `[output_dir]/ns-solution.bin`
11469293791SJames Wright
11569293791SJames Wright* - `-continue_time_filename`
1164de8550aSJed Brown  - Path to time stamp binary file (only for legacy checkpoints)
11769293791SJames Wright  - `[output_dir]/ns-time.bin`
11869293791SJames Wright
1194534a52eSLeila Ghaffari* - `-bc_wall`
1204534a52eSLeila Ghaffari  - Use wall boundary conditions on this list of faces
1214534a52eSLeila Ghaffari  -
1224534a52eSLeila Ghaffari
1234534a52eSLeila Ghaffari* - `-wall_comps`
1244534a52eSLeila Ghaffari  - An array of constrained component numbers for wall BCs
1254534a52eSLeila Ghaffari  -
1264534a52eSLeila Ghaffari
1279f844368SJames Wright* - `-bc_slip`
1289f844368SJames Wright  - Use weak slip boundary condition on this list of faces
1299f844368SJames Wright  -
1309f844368SJames Wright
1317c5bba50SJames Wright* - `-bc_symmetry_x`
1327c5bba50SJames Wright  - Use symmetry boundary conditions, for the x component, on this list of faces
1334534a52eSLeila Ghaffari  -
1344534a52eSLeila Ghaffari
1357c5bba50SJames Wright* - `-bc_symmetry_y`
1367c5bba50SJames Wright  - Use symmetry boundary conditions, for the y component, on this list of faces
1374534a52eSLeila Ghaffari  -
1384534a52eSLeila Ghaffari
1397c5bba50SJames Wright* - `-bc_symmetry_z`
1407c5bba50SJames Wright  - Use symmetry boundary conditions, for the z component, on this list of faces
1414534a52eSLeila Ghaffari  -
1424534a52eSLeila Ghaffari
1434534a52eSLeila Ghaffari* - `-bc_inflow`
1444534a52eSLeila Ghaffari  - Use inflow boundary conditions on this list of faces
1454534a52eSLeila Ghaffari  -
1464534a52eSLeila Ghaffari
1474534a52eSLeila Ghaffari* - `-bc_outflow`
1484534a52eSLeila Ghaffari  - Use outflow boundary conditions on this list of faces
1494534a52eSLeila Ghaffari  -
15089d0f5c0SLeila Ghaffari
1517ec884f8SJames Wright* - `-bc_freestream`
1527ec884f8SJames Wright  - Use freestream boundary conditions on this list of faces
1537ec884f8SJames Wright  -
1547ec884f8SJames Wright
155b7d66439SJames Wright* - `-ts_monitor_turbulence_spanstats_collect_interval`
156ee3de563SJames Wright  - Number of timesteps between statistics collection
157ee3de563SJames Wright  - `1`
158ee3de563SJames Wright
159b7d66439SJames Wright* - `-ts_monitor_turbulence_spanstats_viewer`
160b7d66439SJames Wright  - Sets the PetscViewer for the statistics file writing, such as `cgns:output-%d.cgns` (requires PETSc `--download-cgns`). Also turns the statistics collection on.
1618ed52730SJames Wright  -
1628ed52730SJames Wright
163b7d66439SJames Wright* - `-ts_monitor_turbulence_spanstats_viewer_interval`
164ee3de563SJames Wright  - Number of timesteps between statistics file writing (`-1` means only at end of run)
165ee3de563SJames Wright  - `-1`
166ee3de563SJames Wright
167b7d66439SJames Wright* - `-ts_monitor_turbulence_spanstats_viewer_cgns_batch_size`
1688ed52730SJames Wright  - Number of frames written per CGNS file if the CGNS file name includes a format specifier (`%d`).
1698ed52730SJames Wright  - `20`
1708ed52730SJames Wright
171ca69d878SAdeleke O. Bankole* - `-ts_monitor_wall_force`
172ca69d878SAdeleke O. Bankole  - Viewer for the force on each no-slip wall, e.g., `ascii:force.csv:ascii_csv` to write a CSV file.
173ca69d878SAdeleke O. Bankole  -
174ca69d878SAdeleke O. Bankole
1752526956eSJames Wright* - `-mesh_transform`
1762526956eSJames Wright  - Transform the mesh, usually for an initial box mesh.
1772526956eSJames Wright  - `none`
1782526956eSJames Wright
179bc7bbd5dSLeila Ghaffari* - `-snes_view`
180bc7bbd5dSLeila Ghaffari  - View PETSc `SNES` nonlinear solver configuration
181bc7bbd5dSLeila Ghaffari  -
18289d0f5c0SLeila Ghaffari
183bc7bbd5dSLeila Ghaffari* - `-log_view`
184bc7bbd5dSLeila Ghaffari  - View PETSc performance log
185bc7bbd5dSLeila Ghaffari  -
186ccaff030SJeremy L Thompson
187bc7bbd5dSLeila Ghaffari* - `-help`
188bc7bbd5dSLeila Ghaffari  - View comprehensive information about run-time options
189bc7bbd5dSLeila Ghaffari  -
190bc7bbd5dSLeila Ghaffari:::
191ccaff030SJeremy L Thompson
1927c5bba50SJames WrightFor the case of a square/cubic mesh, the list of face indices to be used with `-bc_wall`, `bc_inflow`, `bc_outflow`, `bc_freestream`  and/or `-bc_symmetry_x`, `-bc_symmetry_y`, and `-bc_symmetry_z` are:
1934534a52eSLeila Ghaffari
19488626eedSJames Wright:::{list-table} 2D Face ID Labels
19588626eedSJames Wright:header-rows: 1
19688626eedSJames Wright* - PETSc Face Name
19788626eedSJames Wright  - Cartesian direction
19888626eedSJames Wright  - Face ID
19988626eedSJames Wright
20088626eedSJames Wright* - faceMarkerBottom
20188626eedSJames Wright  - -z
20288626eedSJames Wright  - 1
20388626eedSJames Wright
20488626eedSJames Wright* - faceMarkerRight
20588626eedSJames Wright  - +x
20688626eedSJames Wright  - 2
20788626eedSJames Wright
20888626eedSJames Wright* - faceMarkerTop
20988626eedSJames Wright  - +z
21088626eedSJames Wright  - 3
21188626eedSJames Wright
21288626eedSJames Wright* - faceMarkerLeft
21388626eedSJames Wright  - -x
21488626eedSJames Wright  - 4
21588626eedSJames Wright:::
21688626eedSJames Wright
217b5e826a6SLeila Ghaffari:::{list-table} 3D Face ID Labels
21888626eedSJames Wright:header-rows: 1
21988626eedSJames Wright* - PETSc Face Name
22088626eedSJames Wright  - Cartesian direction
22188626eedSJames Wright  - Face ID
22288626eedSJames Wright
22388626eedSJames Wright* - faceMarkerBottom
22488626eedSJames Wright  - -z
22588626eedSJames Wright  - 1
22688626eedSJames Wright
22788626eedSJames Wright* - faceMarkerTop
22888626eedSJames Wright  - +z
22988626eedSJames Wright  - 2
23088626eedSJames Wright
23188626eedSJames Wright* - faceMarkerFront
23288626eedSJames Wright  - -y
23388626eedSJames Wright  - 3
23488626eedSJames Wright
23588626eedSJames Wright* - faceMarkerBack
23688626eedSJames Wright  - +y
23788626eedSJames Wright  - 4
23888626eedSJames Wright
23988626eedSJames Wright* - faceMarkerRight
24088626eedSJames Wright  - +x
24188626eedSJames Wright  - 5
24288626eedSJames Wright
24388626eedSJames Wright* - faceMarkerLeft
24488626eedSJames Wright  - -x
24588626eedSJames Wright  - 6
24688626eedSJames Wright:::
2474534a52eSLeila Ghaffari
2488a94a473SJed Brown### Boundary conditions
2498a94a473SJed Brown
2503b219b86SJames WrightBoundary conditions for compressible viscous flows are notoriously tricky.
2513b219b86SJames WrightHere we offer some recommendations.
2528a94a473SJed Brown
2538a94a473SJed Brown#### Inflow
2548a94a473SJed Brown
2558a94a473SJed BrownIf in a region where the flow velocity is known (e.g., away from viscous walls), use `bc_freestream`, which solves a Riemann problem and can handle inflow and outflow (simultaneously and dynamically).
2568a94a473SJed BrownIt is stable and the least reflective boundary condition for acoustics.
2578a94a473SJed Brown
2588a94a473SJed BrownIf near a viscous wall, you may want a specified inflow profile.
2598a94a473SJed BrownUse `bc_inflow` and see {ref}`example-blasius` and discussion of synthetic turbulence generation for ways to analytically generate developed inflow profiles.
2608a94a473SJed BrownThese conditions may be either weak or strong, with the latter specifying velocity and temperature as essential boundary conditions and evaluating a boundary integral for the mass flux.
2618a94a473SJed BrownThe strong approach gives sharper resolution of velocity structures.
2628a94a473SJed BrownWe have described the primitive variable formulation here; the conservative variants are similar, but not equivalent.
2638a94a473SJed Brown
264f3f66076SJames Wright#### Outflow
2658a94a473SJed Brown
2668a94a473SJed BrownIf you know the complete exterior state, `bc_freestream` is the least reflective boundary condition, but is disruptive to viscous flow structures.
2678a94a473SJed BrownIf thermal anomalies must exit the domain, the Riemann solver must resolve the contact wave to avoid reflections.
2688a94a473SJed BrownThe default Riemann solver, HLLC, is sufficient in this regard while the simpler HLL converts thermal structures exiting the domain into grid-scale reflecting acoustics.
2698a94a473SJed Brown
2708a94a473SJed BrownIf acoustic reflections are not a concern and/or the flow is impacted by walls or interior structures that you wish to resolve to near the boundary, choose `bc_outflow`. This condition (with default `outflow_type: riemann`) is stable for both inflow and outflow, so can be used in areas that have recirculation and lateral boundaries in which the flow fluctuates.
2718a94a473SJed Brown
2728a94a473SJed BrownThe simpler `bc_outflow` variant, `outflow_type: pressure`, requires that the flow be a strict outflow (or the problem becomes ill-posed and the solver will diverge).
2738a94a473SJed BrownIn our experience, `riemann` is slightly less reflective but produces similar flows in cases of strict outflow.
2748a94a473SJed BrownThe `pressure` variant is retained to facilitate comparison with other codes, such as PHASTA-C, but we recommend `riemann` for general use.
2758a94a473SJed Brown
276f3f66076SJames Wright#### Periodicity
2778a94a473SJed Brown
2788a94a473SJed BrownPETSc provides two ways to specify periodicity:
2798a94a473SJed Brown
2808a94a473SJed Brown1. Topological periodicity, in which the donor and receiver dofs are the same, obtained using:
2818a94a473SJed Brown
2828a94a473SJed Brown```yaml
2838a94a473SJed Browndm_plex:
2848a94a473SJed Brown  shape: box
2858a94a473SJed Brown  box_faces: 10,12,4
2868a94a473SJed Brown  box_bd: none,none,periodic
2878a94a473SJed Brown```
2888a94a473SJed Brown
289ca69d878SAdeleke O. BankoleThe coordinates for such cases are stored as a new field with special cell-based indexing to enable wrapping through the boundary.
290ca69d878SAdeleke O. BankoleThis choice of coordinates prevents evaluating boundary integrals that cross the periodicity, such as for the outflow Riemann problem in the presence of spanwise periodicity.
291ca69d878SAdeleke O. Bankole
292ca69d878SAdeleke O. Bankole2. Isoperiodicity, in which the donor and receiver dofs are distinct in local vectors. This is obtained using `zbox`, as in:
293ca69d878SAdeleke O. Bankole
294ca69d878SAdeleke O. Bankole```yaml
295ca69d878SAdeleke O. Bankoledm_plex:
296ca69d878SAdeleke O. Bankole  shape: zbox
297ca69d878SAdeleke O. Bankole  box_faces: 10,12,4
298ca69d878SAdeleke O. Bankole  box_bd: none,none,periodic
299ca69d878SAdeleke O. Bankole```
300ca69d878SAdeleke O. Bankole
301ca69d878SAdeleke O. BankoleIsoperiodicity enables standard boundary integrals, and is recommended for general use.
302ca69d878SAdeleke O. BankoleAt the time of this writing, it only supports one direction of periodicity.
303ca69d878SAdeleke O. BankoleThe `zbox` method uses [Z-ordering](https://en.wikipedia.org/wiki/Z-order_curve) to construct the mesh in parallel and provide an adequate initial partition, which makes it higher performance and avoids needing a partitioning package.
3048a94a473SJed Brown
305019b7682STimothy Aiken### Advection
306019b7682STimothy Aiken
30717be3a41SJeremy L ThompsonFor testing purposes, there is a reduced mode for pure advection, which holds density $\rho$ and momentum density $\rho \bm u$ constant while advecting "total energy density" $E$.
3089e529eadSJames WrightThe advection problems can be run in both 2D and 3D, based on the DM defined for the problem.
30994a05c6fSJames WrightThe following additional command-line options are available:
310019b7682STimothy Aiken
31194a05c6fSJames Wright:::{list-table} Advection Runtime Options
312bc7bbd5dSLeila Ghaffari:header-rows: 1
313e43605a5SLeila Ghaffari
314bc7bbd5dSLeila Ghaffari* - Option
315bc7bbd5dSLeila Ghaffari  - Description
316bc7bbd5dSLeila Ghaffari  - Default value
317bc7bbd5dSLeila Ghaffari  - Unit
318e43605a5SLeila Ghaffari
319bc7bbd5dSLeila Ghaffari* - `-rc`
320bc7bbd5dSLeila Ghaffari  - Characteristic radius of thermal bubble
321bc7bbd5dSLeila Ghaffari  - `1000`
322bc7bbd5dSLeila Ghaffari  - `m`
323e43605a5SLeila Ghaffari
324bc7bbd5dSLeila Ghaffari* - `-units_meter`
325bc7bbd5dSLeila Ghaffari  - 1 meter in scaled length units
326bc7bbd5dSLeila Ghaffari  - `1E-2`
327bc7bbd5dSLeila Ghaffari  -
328e43605a5SLeila Ghaffari
329bc7bbd5dSLeila Ghaffari* - `-units_second`
330bc7bbd5dSLeila Ghaffari  - 1 second in scaled time units
331bc7bbd5dSLeila Ghaffari  - `1E-2`
332bc7bbd5dSLeila Ghaffari  -
333e43605a5SLeila Ghaffari
334bc7bbd5dSLeila Ghaffari* - `-units_kilogram`
335bc7bbd5dSLeila Ghaffari  - 1 kilogram in scaled mass units
336bc7bbd5dSLeila Ghaffari  - `1E-6`
337bc7bbd5dSLeila Ghaffari  -
338e43605a5SLeila Ghaffari
339bc7bbd5dSLeila Ghaffari* - `-strong_form`
340bc7bbd5dSLeila Ghaffari  - Strong (1) or weak/integrated by parts (0) residual
341bc7bbd5dSLeila Ghaffari  - `0`
342bc7bbd5dSLeila Ghaffari  -
343e43605a5SLeila Ghaffari
344bc7bbd5dSLeila Ghaffari* - `-stab`
345bc7bbd5dSLeila Ghaffari  - Stabilization method (`none`, `su`, or `supg`)
346bc7bbd5dSLeila Ghaffari  - `none`
347bc7bbd5dSLeila Ghaffari  -
348e43605a5SLeila Ghaffari
349*44e8f77dSJames Wright* - `-stab_tau`
350*44e8f77dSJames Wright  - Formulation for $\tau$ in stabilization (`ctau`, `advdiff_shakib`)
351*44e8f77dSJames Wright  - `ctau`
352*44e8f77dSJames Wright  -
353*44e8f77dSJames Wright
354*44e8f77dSJames Wright* - `-Ctau_t`
355*44e8f77dSJames Wright  - Scaling factor on the temporal portion of the $\tau$ formulation
356*44e8f77dSJames Wright  - 0.
357*44e8f77dSJames Wright  -
358*44e8f77dSJames Wright
359*44e8f77dSJames Wright* - `-Ctau_a`
360*44e8f77dSJames Wright  - Scaling factor on the advection portion of the $\tau$ formulation
361*44e8f77dSJames Wright  - $P^2$
362*44e8f77dSJames Wright  -
363*44e8f77dSJames Wright
364bc7bbd5dSLeila Ghaffari* - `-CtauS`
365bc7bbd5dSLeila Ghaffari  - Scale coefficient for stabilization tau (nondimensional)
366bc7bbd5dSLeila Ghaffari  - `0`
367bc7bbd5dSLeila Ghaffari  -
368e43605a5SLeila Ghaffari
369bc7bbd5dSLeila Ghaffari* - `-wind_type`
370bc7bbd5dSLeila Ghaffari  - Wind type in Advection (`rotation` or `translation`)
371bc7bbd5dSLeila Ghaffari  - `rotation`
372bc7bbd5dSLeila Ghaffari  -
373e43605a5SLeila Ghaffari
374bc7bbd5dSLeila Ghaffari* - `-wind_translation`
375bc7bbd5dSLeila Ghaffari  - Constant wind vector when `-wind_type translation`
376bc7bbd5dSLeila Ghaffari  - `1,0,0`
377bc7bbd5dSLeila Ghaffari  -
378e43605a5SLeila Ghaffari
379bc7bbd5dSLeila Ghaffari* - `-E_wind`
380bc7bbd5dSLeila Ghaffari  - Total energy of inflow wind when `-wind_type translation`
381bc7bbd5dSLeila Ghaffari  - `1E6`
382bc7bbd5dSLeila Ghaffari  - `J`
383e43605a5SLeila Ghaffari
3847b77ddfdSJames Wright* - `-advection_ic_type`
3857b77ddfdSJames Wright  - Initial condition type, from `sphere`, `cylinder`, `cosine_hill`, and `skew`
386f3f66076SJames Wright  - `sphere`
387bc7bbd5dSLeila Ghaffari  -
388e43605a5SLeila Ghaffari
389bc7bbd5dSLeila Ghaffari* - `-bubble_continuity`
3909e529eadSJames Wright  - Different shapes for `sphere` and `cylinder` initial conditions, from `smooth`, `back_sharp`, `thick`, or `cosine`
391bc7bbd5dSLeila Ghaffari  - `smooth`
392bc7bbd5dSLeila Ghaffari  -
393bc7bbd5dSLeila Ghaffari:::
394ccaff030SJeremy L Thompson
39594a05c6fSJames WrightFor 3D advection, an example of the `rotation` mode can be run with:
396ccaff030SJeremy L Thompson
397bc7bbd5dSLeila Ghaffari```
3984534a52eSLeila Ghaffari./navierstokes -problem advection -dm_plex_box_faces 10,10,10 -dm_plex_dim 3 -dm_plex_box_lower 0,0,0 -dm_plex_box_upper 8000,8000,8000 -bc_wall 1,2,3,4,5,6 -wall_comps 4 -wind_type rotation -implicit -stab su
399bc7bbd5dSLeila Ghaffari```
400ccaff030SJeremy L Thompson
401bc7bbd5dSLeila Ghaffariand the `translation` mode with:
402ccaff030SJeremy L Thompson
403bc7bbd5dSLeila Ghaffari```
4044534a52eSLeila Ghaffari./navierstokes -problem advection -dm_plex_box_faces 10,10,10 -dm_plex_dim 3 -dm_plex_box_lower 0,0,0 -dm_plex_box_upper 8000,8000,8000 -wind_type translation -wind_translation .5,-1,0 -bc_inflow 1,2,3,4,5,6
405bc7bbd5dSLeila Ghaffari```
406ccaff030SJeremy L Thompson
40794a05c6fSJames WrightFor 2D advection, an example of the `rotation` mode can be run with:
40894a05c6fSJames Wright
40994a05c6fSJames Wright```
4109e529eadSJames Wright./navierstokes -problem advection -dm_plex_box_faces 20,20 -dm_plex_box_lower 0,0 -dm_plex_box_upper 1000,1000 -bc_wall 1,2,3,4 -wall_comps 4 -wind_type rotation -implicit -stab supg
41194a05c6fSJames Wright```
41294a05c6fSJames Wright
41394a05c6fSJames Wrightand the `translation` mode with:
41494a05c6fSJames Wright
41594a05c6fSJames Wright```
4169e529eadSJames Wright./navierstokes -problem advection -dm_plex_box_faces 20,20 -dm_plex_box_lower 0,0 -dm_plex_box_upper 1000,1000 -units_meter 1e-4 -wind_type translation -wind_translation 1,-.5 -bc_inflow 1,2,3,4
41794a05c6fSJames Wright```
41894a05c6fSJames WrightNote the lengths in `-dm_plex_box_upper` are given in meters, and will be nondimensionalized according to `-units_meter`.
41994a05c6fSJames Wright
420019b7682STimothy Aiken### Inviscid Ideal Gas
421019b7682STimothy Aiken
422019b7682STimothy Aiken#### Isentropic Euler vortex
423019b7682STimothy Aiken
424bc7bbd5dSLeila GhaffariFor the Isentropic Vortex problem, the following additional command-line options are available:
425ccaff030SJeremy L Thompson
426bc7bbd5dSLeila Ghaffari:::{list-table} Isentropic Vortex Runtime Options
427bc7bbd5dSLeila Ghaffari:header-rows: 1
428ccaff030SJeremy L Thompson
429bc7bbd5dSLeila Ghaffari* - Option
430bc7bbd5dSLeila Ghaffari  - Description
431bc7bbd5dSLeila Ghaffari  - Default value
432bc7bbd5dSLeila Ghaffari  - Unit
433ccaff030SJeremy L Thompson
434bc7bbd5dSLeila Ghaffari* - `-center`
435bc7bbd5dSLeila Ghaffari  - Location of vortex center
436bc7bbd5dSLeila Ghaffari  - `(lx,ly,lz)/2`
437bc7bbd5dSLeila Ghaffari  - `(m,m,m)`
438ccaff030SJeremy L Thompson
439bc7bbd5dSLeila Ghaffari* - `-units_meter`
440bc7bbd5dSLeila Ghaffari  - 1 meter in scaled length units
441bc7bbd5dSLeila Ghaffari  - `1E-2`
442bc7bbd5dSLeila Ghaffari  -
443ccaff030SJeremy L Thompson
444bc7bbd5dSLeila Ghaffari* - `-units_second`
445bc7bbd5dSLeila Ghaffari  - 1 second in scaled time units
446bc7bbd5dSLeila Ghaffari  - `1E-2`
447bc7bbd5dSLeila Ghaffari  -
448ccaff030SJeremy L Thompson
449bc7bbd5dSLeila Ghaffari* - `-mean_velocity`
450bc7bbd5dSLeila Ghaffari  - Background velocity vector
451bc7bbd5dSLeila Ghaffari  - `(1,1,0)`
452bc7bbd5dSLeila Ghaffari  -
453ccaff030SJeremy L Thompson
454bc7bbd5dSLeila Ghaffari* - `-vortex_strength`
455bc7bbd5dSLeila Ghaffari  - Strength of vortex < 10
456bc7bbd5dSLeila Ghaffari  - `5`
457bc7bbd5dSLeila Ghaffari  -
458932417b3SJed Brown
459932417b3SJed Brown* - `-c_tau`
460932417b3SJed Brown  - Stabilization constant
461504dc8e0SLeila Ghaffari  - `0.5`
462932417b3SJed Brown  -
463bc7bbd5dSLeila Ghaffari:::
464ccaff030SJeremy L Thompson
465bc7bbd5dSLeila GhaffariThis problem can be run with:
466ccaff030SJeremy L Thompson
467bc7bbd5dSLeila Ghaffari```
4687c5bba50SJames Wright./navierstokes -problem euler_vortex -dm_plex_box_faces 20,20,1 -dm_plex_box_lower 0,0,0 -dm_plex_box_upper 1000,1000,50 -dm_plex_dim 3 -bc_inflow 4,6 -bc_outflow 3,5 -bc_symmetry_z 1,2 -mean_velocity .5,-.8,0.
469bc7bbd5dSLeila Ghaffari```
470ccaff030SJeremy L Thompson
471019b7682STimothy Aiken#### Sod shock tube
472019b7682STimothy Aiken
473019b7682STimothy AikenFor the Shock Tube problem, the following additional command-line options are available:
474019b7682STimothy Aiken
475019b7682STimothy Aiken:::{list-table} Shock Tube Runtime Options
476019b7682STimothy Aiken:header-rows: 1
477019b7682STimothy Aiken
478019b7682STimothy Aiken* - Option
479019b7682STimothy Aiken  - Description
480019b7682STimothy Aiken  - Default value
481019b7682STimothy Aiken  - Unit
482019b7682STimothy Aiken
483019b7682STimothy Aiken* - `-units_meter`
484019b7682STimothy Aiken  - 1 meter in scaled length units
485019b7682STimothy Aiken  - `1E-2`
486019b7682STimothy Aiken  -
487019b7682STimothy Aiken
488019b7682STimothy Aiken* - `-units_second`
489019b7682STimothy Aiken  - 1 second in scaled time units
490019b7682STimothy Aiken  - `1E-2`
491019b7682STimothy Aiken  -
492019b7682STimothy Aiken
493019b7682STimothy Aiken* - `-yzb`
494019b7682STimothy Aiken  - Use YZB discontinuity capturing
495019b7682STimothy Aiken  - `none`
496019b7682STimothy Aiken  -
497019b7682STimothy Aiken
498019b7682STimothy Aiken* - `-stab`
499019b7682STimothy Aiken  - Stabilization method (`none`, `su`, or `supg`)
500019b7682STimothy Aiken  - `none`
501019b7682STimothy Aiken  -
502019b7682STimothy Aiken:::
503019b7682STimothy Aiken
504019b7682STimothy AikenThis problem can be run with:
505019b7682STimothy Aiken
506019b7682STimothy Aiken```
5077c5bba50SJames Wright./navierstokes -problem shocktube -yzb -stab su -bc_symmetry_z 3,4 -bc_symmetry_y 1,2 -bc_wall 5,6 -dm_plex_dim 3 -dm_plex_box_lower 0,0,0 -dm_plex_box_upper 1000,100,100 -dm_plex_box_faces 200,1,1 -units_second 0.1
508019b7682STimothy Aiken```
509019b7682STimothy Aiken
510019b7682STimothy Aiken### Newtonian viscosity, Ideal Gas
511019b7682STimothy Aiken
51288626eedSJames WrightFor the Density Current, Channel, and Blasius problems, the following common command-line options are available:
513ccaff030SJeremy L Thompson
51488626eedSJames Wright:::{list-table} Newtonian Ideal Gas problems Runtime Options
515bc7bbd5dSLeila Ghaffari:header-rows: 1
516ccaff030SJeremy L Thompson
517bc7bbd5dSLeila Ghaffari* - Option
518bc7bbd5dSLeila Ghaffari  - Description
519bc7bbd5dSLeila Ghaffari  - Default value
520bc7bbd5dSLeila Ghaffari  - Unit
521ccaff030SJeremy L Thompson
522bc7bbd5dSLeila Ghaffari* - `-units_meter`
523bc7bbd5dSLeila Ghaffari  - 1 meter in scaled length units
52488626eedSJames Wright  - `1`
525bc7bbd5dSLeila Ghaffari  -
526ccaff030SJeremy L Thompson
527bc7bbd5dSLeila Ghaffari* - `-units_second`
528bc7bbd5dSLeila Ghaffari  - 1 second in scaled time units
52988626eedSJames Wright  - `1`
530bc7bbd5dSLeila Ghaffari  -
531ccaff030SJeremy L Thompson
532bc7bbd5dSLeila Ghaffari* - `-units_kilogram`
533bc7bbd5dSLeila Ghaffari  - 1 kilogram in scaled mass units
53488626eedSJames Wright  - `1`
535bc7bbd5dSLeila Ghaffari  -
536ccaff030SJeremy L Thompson
537bc7bbd5dSLeila Ghaffari* - `-units_Kelvin`
538bc7bbd5dSLeila Ghaffari  - 1 Kelvin in scaled temperature units
539bc7bbd5dSLeila Ghaffari  - `1`
540bc7bbd5dSLeila Ghaffari  -
541ccaff030SJeremy L Thompson
542bc7bbd5dSLeila Ghaffari* - `-stab`
543bc7bbd5dSLeila Ghaffari  - Stabilization method (`none`, `su`, or `supg`)
544bc7bbd5dSLeila Ghaffari  - `none`
545bc7bbd5dSLeila Ghaffari  -
546ccaff030SJeremy L Thompson
547932417b3SJed Brown* - `-c_tau`
54888626eedSJames Wright  - Stabilization constant, $c_\tau$
549504dc8e0SLeila Ghaffari  - `0.5`
550932417b3SJed Brown  -
551932417b3SJed Brown
55288626eedSJames Wright* - `-Ctau_t`
55388626eedSJames Wright  - Stabilization time constant, $C_t$
55488626eedSJames Wright  - `1.0`
55588626eedSJames Wright  -
556ccaff030SJeremy L Thompson
55788626eedSJames Wright* - `-Ctau_v`
55888626eedSJames Wright  - Stabilization viscous constant, $C_v$
55994c01735SLeila Ghaffari  - `36, 60, 128 for degree = 1, 2, 3`
56088626eedSJames Wright  -
561ccaff030SJeremy L Thompson
56288626eedSJames Wright* - `-Ctau_C`
56388626eedSJames Wright  - Stabilization continuity constant, $C_c$
56488626eedSJames Wright  - `1.0`
56588626eedSJames Wright  -
566ccaff030SJeremy L Thompson
56788626eedSJames Wright* - `-Ctau_M`
56888626eedSJames Wright  - Stabilization momentum constant, $C_m$
56988626eedSJames Wright  - `1.0`
57088626eedSJames Wright  -
57188626eedSJames Wright
57288626eedSJames Wright* - `-Ctau_E`
57388626eedSJames Wright  - Stabilization energy constant, $C_E$
57488626eedSJames Wright  - `1.0`
57588626eedSJames Wright  -
576ccaff030SJeremy L Thompson
577bc7bbd5dSLeila Ghaffari* - `-cv`
578bc7bbd5dSLeila Ghaffari  - Heat capacity at constant volume
579bc7bbd5dSLeila Ghaffari  - `717`
580bc7bbd5dSLeila Ghaffari  - `J/(kg K)`
581ccaff030SJeremy L Thompson
582bc7bbd5dSLeila Ghaffari* - `-cp`
583bc7bbd5dSLeila Ghaffari  - Heat capacity at constant pressure
584bc7bbd5dSLeila Ghaffari  - `1004`
585bc7bbd5dSLeila Ghaffari  - `J/(kg K)`
586ccaff030SJeremy L Thompson
587a2726bdbSJames Wright* - `-gravity`
588a2726bdbSJames Wright  - Gravitational acceleration vector
589a2726bdbSJames Wright  - `0,0,0`
590bc7bbd5dSLeila Ghaffari  - `m/s^2`
591ccaff030SJeremy L Thompson
592bc7bbd5dSLeila Ghaffari* - `-lambda`
593bc7bbd5dSLeila Ghaffari  - Stokes hypothesis second viscosity coefficient
594bc7bbd5dSLeila Ghaffari  - `-2/3`
595bc7bbd5dSLeila Ghaffari  -
596ccaff030SJeremy L Thompson
597bc7bbd5dSLeila Ghaffari* - `-mu`
598bc7bbd5dSLeila Ghaffari  - Shear dynamic viscosity coefficient
599a2726bdbSJames Wright  - `1.8e-5`
600bc7bbd5dSLeila Ghaffari  -  `Pa s`
60177841947SLeila Ghaffari
602bc7bbd5dSLeila Ghaffari* - `-k`
603bc7bbd5dSLeila Ghaffari  - Thermal conductivity
604bc7bbd5dSLeila Ghaffari  - `0.02638`
605bc7bbd5dSLeila Ghaffari  - `W/(m K)`
606a1df05f8SJed Brown
607a1df05f8SJed Brown* - `-newtonian_unit_tests`
608a1df05f8SJed Brown  - Developer option to test properties
609a1df05f8SJed Brown  - `false`
610a1df05f8SJed Brown  - boolean
611de2fdd78SJames Wright
6125c0afad3SJames Wright* - `-state_var`
6135c0afad3SJames Wright  - State variables to solve solution with. `conservative` ($\rho, \rho \bm{u}, \rho e$) or `primitive` ($P, \bm{u}, T$)
6145c0afad3SJames Wright  - `conservative`
6155c0afad3SJames Wright  - string
616530ad8c4SKenneth E. Jansen
617530ad8c4SKenneth E. Jansen* - `-idl_decay_time`
618530ad8c4SKenneth E. Jansen  - Characteristic timescale of the pressure deviance decay. The timestep is good starting point
619530ad8c4SKenneth E. Jansen  - `-1` (disabled)
620530ad8c4SKenneth E. Jansen  - `s`
621530ad8c4SKenneth E. Jansen
622530ad8c4SKenneth E. Jansen* - `-idl_start`
623530ad8c4SKenneth E. Jansen  - Start of IDL in the x direction
624530ad8c4SKenneth E. Jansen  - `0`
625530ad8c4SKenneth E. Jansen  - `m`
626530ad8c4SKenneth E. Jansen
627530ad8c4SKenneth E. Jansen* - `-idl_length`
628530ad8c4SKenneth E. Jansen  - Length of IDL in the positive x direction
629530ad8c4SKenneth E. Jansen  - `0`
630530ad8c4SKenneth E. Jansen  - `m`
631530ad8c4SKenneth E. Jansen
632c79d6dc9SJames Wright* - `-sgs_model_type`
633c79d6dc9SJames Wright  - Type of subgrid stress model to use. Currently only `data_driven` is available
634c79d6dc9SJames Wright  - `none`
635c79d6dc9SJames Wright  - string
636c79d6dc9SJames Wright
637c79d6dc9SJames Wright* - `-sgs_model_dd_leakyrelu_alpha`
638c79d6dc9SJames Wright  - Slope parameter for Leaky ReLU activation function. `0` corresponds to normal ReLU
639c79d6dc9SJames Wright  - 0
640c79d6dc9SJames Wright  -
641c79d6dc9SJames Wright
642c79d6dc9SJames Wright* - `-sgs_model_dd_parameter_dir`
643c79d6dc9SJames Wright  - Path to directory with data-driven model parameters (weights, biases, etc.)
644c79d6dc9SJames Wright  - `./dd_sgs_parameters`
645c79d6dc9SJames Wright  - string
646c79d6dc9SJames Wright
647cf90ec9bSJames Wright* - `-sgs_model_dd_use_fused`
648cf90ec9bSJames Wright  - Whether to use "fused" mode for data-driven model evaluation
649cf90ec9bSJames Wright  - `true`
650cf90ec9bSJames Wright  - boolean
651cf90ec9bSJames Wright
6523f89fbfdSJames Wright* - `-diff_filter_monitor`
6533f89fbfdSJames Wright  - Enable differential filter TSMonitor
6543f89fbfdSJames Wright  - `false`
6553f89fbfdSJames Wright  - boolean
6563f89fbfdSJames Wright
6573f89fbfdSJames Wright* - `-diff_filter_grid_based_width`
6583f89fbfdSJames Wright  - Use filter width based on the grid size
6593f89fbfdSJames Wright  - `false`
6603f89fbfdSJames Wright  - boolean
6613f89fbfdSJames Wright
6623f89fbfdSJames Wright* - `-diff_filter_width_scaling`
6633f89fbfdSJames Wright  - Anisotropic scaling for filter width in wall-aligned coordinates (snz)
6643f89fbfdSJames Wright  - `1,1,1`
6653f89fbfdSJames Wright  - `m`
6663f89fbfdSJames Wright
6673f89fbfdSJames Wright* - `-diff_filter_kernel_scaling`
6683f89fbfdSJames Wright  - Scaling to make differential kernel size equivalent to other filter kernels
6693f89fbfdSJames Wright  - `0.1`
6703f89fbfdSJames Wright  - `m^2`
6713f89fbfdSJames Wright
6723f89fbfdSJames Wright* - `-diff_filter_wall_damping_function`
6733f89fbfdSJames Wright  - Damping function to use at the wall for anisotropic filtering (`none`, `van_driest`)
6743f89fbfdSJames Wright  - `none`
6753f89fbfdSJames Wright  - string
6763f89fbfdSJames Wright
6773f89fbfdSJames Wright* - `-diff_filter_wall_damping_constant`
6789d9c52bbSJed Brown  - Constant for the wall-damping function. $A^+$ for `van_driest` damping function.
6793f89fbfdSJames Wright  - 25
6803f89fbfdSJames Wright  -
6813f89fbfdSJames Wright
6823f89fbfdSJames Wright* - `-diff_filter_friction_length`
6833f89fbfdSJames Wright  - Friction length associated with the flow, $\delta_\nu$. Used in wall-damping functions
6843f89fbfdSJames Wright  - 0
6853f89fbfdSJames Wright  - `m`
6863f89fbfdSJames Wright
6873b219b86SJames Wright* - `-sgs_train_enable`
6883b219b86SJames Wright  - Whether to enable *in situ* training of data-driven SGS model. Require building with SmartRedis.
6893b219b86SJames Wright  - `false`
6903b219b86SJames Wright  - boolean
6913b219b86SJames Wright
6923b219b86SJames Wright* - `-sgs_train_write_data_interval`
6933b219b86SJames Wright  - Number of timesteps between writing training data into SmartRedis database
6943b219b86SJames Wright  - `1`
6953b219b86SJames Wright  -
6963b219b86SJames Wright
6973b219b86SJames Wright* - `-sgs_train_overwrite_data`
6983b219b86SJames Wright  - Whether new training data should overwrite old data on database
6993b219b86SJames Wright  - `true`
7003b219b86SJames Wright  - boolean
7013b219b86SJames Wright
7023b219b86SJames Wright* - `-smartsim_collocated_num_ranks`
7033b219b86SJames Wright  - Number of MPI ranks associated with each collocated database (i.e. ranks per node)
7043b219b86SJames Wright  - `1`
7053b219b86SJames Wright  -
706bc7bbd5dSLeila Ghaffari:::
70777841947SLeila Ghaffari
708530ad8c4SKenneth E. Jansen#### Gaussian Wave
7097ec884f8SJames Wright
710530ad8c4SKenneth E. JansenThe Gaussian wave problem has the following command-line options in addition to the Newtonian Ideal Gas options:
7117ec884f8SJames Wright
712530ad8c4SKenneth E. Jansen:::{list-table} Gaussian Wave Runtime Options
7137ec884f8SJames Wright:header-rows: 1
7147ec884f8SJames Wright
7157ec884f8SJames Wright* - Option
7167ec884f8SJames Wright  - Description
7177ec884f8SJames Wright  - Default value
7187ec884f8SJames Wright  - Unit
7197ec884f8SJames Wright
720f1e435c9SJed Brown* - `-freestream_riemann`
721f1e435c9SJed Brown  - Riemann solver for boundaries (HLL or HLLC)
722f1e435c9SJed Brown  - `hllc`
723f1e435c9SJed Brown  -
724f1e435c9SJed Brown
725f1e435c9SJed Brown* - `-freestream_velocity`
7267ec884f8SJames Wright  - Freestream velocity vector
7277ec884f8SJames Wright  - `0,0,0`
7287ec884f8SJames Wright  - `m/s`
7297ec884f8SJames Wright
730f1e435c9SJed Brown* - `-freestream_temperature`
7317ec884f8SJames Wright  - Freestream temperature
7327ec884f8SJames Wright  - `288`
7337ec884f8SJames Wright  - `K`
7347ec884f8SJames Wright
735f1e435c9SJed Brown* - `-freestream_pressure`
73689e3cb53SJames Wright  - Freestream pressure
7377ec884f8SJames Wright  - `1.01e5`
7387ec884f8SJames Wright  - `Pa`
7397ec884f8SJames Wright
7407ec884f8SJames Wright* - `-epicenter`
7417ec884f8SJames Wright  - Coordinates of center of perturbation
7427ec884f8SJames Wright  - `0,0,0`
7437ec884f8SJames Wright  - `m`
7447ec884f8SJames Wright
7457ec884f8SJames Wright* - `-amplitude`
7467ec884f8SJames Wright  - Amplitude of the perturbation
7477ec884f8SJames Wright  - `0.1`
7487ec884f8SJames Wright  -
7497ec884f8SJames Wright
7507ec884f8SJames Wright* - `-width`
7517ec884f8SJames Wright  - Width parameter of the perturbation
7527ec884f8SJames Wright  - `0.002`
7537ec884f8SJames Wright  - `m`
7547ec884f8SJames Wright
7557ec884f8SJames Wright:::
7567ec884f8SJames Wright
757530ad8c4SKenneth E. JansenThis problem can be run with the `gaussianwave.yaml` file via:
7587ec884f8SJames Wright
7597ec884f8SJames Wright```
760530ad8c4SKenneth E. Jansen./navierstokes -options_file gaussianwave.yaml
7617ec884f8SJames Wright```
7627ec884f8SJames Wright
763530ad8c4SKenneth E. Jansen```{literalinclude} ../../../../../examples/fluids/gaussianwave.yaml
7647ec884f8SJames Wright:language: yaml
7657ec884f8SJames Wright```
766a1df05f8SJed Brown
767d310b3d3SAdeleke O. Bankole#### Vortex Shedding - Flow past Cylinder
768d310b3d3SAdeleke O. Bankole
769d310b3d3SAdeleke O. BankoleThe vortex shedding, flow past cylinder problem has the following command-line options in addition to the Newtonian Ideal Gas options:
770d310b3d3SAdeleke O. Bankole
771d310b3d3SAdeleke O. Bankole:::{list-table} Vortex Shedding Runtime Options
772d310b3d3SAdeleke O. Bankole:header-rows: 1
773d310b3d3SAdeleke O. Bankole
774d310b3d3SAdeleke O. Bankole* - Option
775d310b3d3SAdeleke O. Bankole  - Description
776d310b3d3SAdeleke O. Bankole  - Default value
777d310b3d3SAdeleke O. Bankole  - Unit
778d310b3d3SAdeleke O. Bankole
779d310b3d3SAdeleke O. Bankole* - `-freestream_velocity`
780d310b3d3SAdeleke O. Bankole  - Freestream velocity vector
781d310b3d3SAdeleke O. Bankole  - `0,0,0`
782d310b3d3SAdeleke O. Bankole  - `m/s`
783d310b3d3SAdeleke O. Bankole
784d310b3d3SAdeleke O. Bankole* - `-freestream_temperature`
785d310b3d3SAdeleke O. Bankole  - Freestream temperature
786d310b3d3SAdeleke O. Bankole  - `288`
787d310b3d3SAdeleke O. Bankole  - `K`
788d310b3d3SAdeleke O. Bankole
789d310b3d3SAdeleke O. Bankole* - `-freestream_pressure`
790d310b3d3SAdeleke O. Bankole  - Freestream pressure
791d310b3d3SAdeleke O. Bankole  - `1.01e5`
792d310b3d3SAdeleke O. Bankole  - `Pa`
793d310b3d3SAdeleke O. Bankole
794d310b3d3SAdeleke O. Bankole:::
795d310b3d3SAdeleke O. Bankole
796d310b3d3SAdeleke O. BankoleThe initial condition is taken from `-reference_temperature` and `-reference_pressure`.
797d310b3d3SAdeleke O. BankoleTo run this problem, first generate a mesh:
798d310b3d3SAdeleke O. Bankole
799d310b3d3SAdeleke O. Bankole```console
800d310b3d3SAdeleke O. Bankole$ make -C examples/fluids/meshes
801d310b3d3SAdeleke O. Bankole```
802d310b3d3SAdeleke O. Bankole
803d310b3d3SAdeleke O. BankoleThen run by building the executable and running:
804d310b3d3SAdeleke O. Bankole
805d310b3d3SAdeleke O. Bankole```console
806d310b3d3SAdeleke O. Bankole$ make build/fluids-navierstokes
807ca69d878SAdeleke O. Bankole$ mpiexec -n 6 build/fluids-navierstokes -options_file examples/fluids/vortexshedding.yaml -{ts,snes}_monitor_
808d310b3d3SAdeleke O. Bankole```
809d310b3d3SAdeleke O. Bankole
810ca69d878SAdeleke O. BankoleThe vortex shedding period is roughly 5.6 and this problem runs until time 100 (2000 time steps).
811ca69d878SAdeleke O. BankoleThe above run writes a file named `force.csv` (see `ts_monitor_wall_force` in `vortexshedding.yaml`), which can be postprocessed by running to create a figure showing lift and drag coefficients over time.
812ca69d878SAdeleke O. Bankole
813ca69d878SAdeleke O. Bankole```console
814d6734f85SAdeleke O. Bankole$ python examples/fluids/postprocess/vortexshedding.py
815ca69d878SAdeleke O. Bankole```
816d310b3d3SAdeleke O. Bankole
817d310b3d3SAdeleke O. Bankole```{literalinclude} ../../../../../examples/fluids/vortexshedding.yaml
818d310b3d3SAdeleke O. Bankole:language: yaml
819d310b3d3SAdeleke O. Bankole```
820d310b3d3SAdeleke O. Bankole
821019b7682STimothy Aiken#### Density current
822019b7682STimothy Aiken
823061ff11eSJames WrightThe Density Current problem has the following command-line options in addition to the Newtonian Ideal Gas options:
82488626eedSJames Wright
82588626eedSJames Wright:::{list-table} Density Current Runtime Options
82688626eedSJames Wright:header-rows: 1
82788626eedSJames Wright
82888626eedSJames Wright* - Option
82988626eedSJames Wright  - Description
83088626eedSJames Wright  - Default value
83188626eedSJames Wright  - Unit
83288626eedSJames Wright
83388626eedSJames Wright* - `-center`
83488626eedSJames Wright  - Location of bubble center
83588626eedSJames Wright  - `(lx,ly,lz)/2`
83688626eedSJames Wright  - `(m,m,m)`
83788626eedSJames Wright
83888626eedSJames Wright* - `-dc_axis`
83988626eedSJames Wright  - Axis of density current cylindrical anomaly, or `(0,0,0)` for spherically symmetric
84088626eedSJames Wright  - `(0,0,0)`
84188626eedSJames Wright  -
84288626eedSJames Wright
84388626eedSJames Wright* - `-rc`
84488626eedSJames Wright  - Characteristic radius of thermal bubble
84588626eedSJames Wright  - `1000`
84688626eedSJames Wright  - `m`
84788626eedSJames Wright
84888626eedSJames Wright* - `-theta0`
84988626eedSJames Wright  - Reference potential temperature
85088626eedSJames Wright  - `300`
85188626eedSJames Wright  - `K`
85288626eedSJames Wright
85388626eedSJames Wright* - `-thetaC`
85488626eedSJames Wright  - Perturbation of potential temperature
85588626eedSJames Wright  - `-15`
85688626eedSJames Wright  - `K`
85788626eedSJames Wright
85888626eedSJames Wright* - `-P0`
85988626eedSJames Wright  - Atmospheric pressure
86088626eedSJames Wright  - `1E5`
86188626eedSJames Wright  - `Pa`
86288626eedSJames Wright
86388626eedSJames Wright* - `-N`
86488626eedSJames Wright  - Brunt-Vaisala frequency
86588626eedSJames Wright  - `0.01`
86688626eedSJames Wright  - `1/s`
86788626eedSJames Wright:::
86888626eedSJames Wright
869bc7bbd5dSLeila GhaffariThis problem can be run with:
870ccaff030SJeremy L Thompson
871bc7bbd5dSLeila Ghaffari```
8727c5bba50SJames Wright./navierstokes -problem density_current -dm_plex_box_faces 16,1,8 -degree 1 -dm_plex_box_lower 0,0,0 -dm_plex_box_upper 2000,125,1000 -dm_plex_dim 3 -rc 400. -bc_wall 1,2,5,6 -wall_comps 1,2,3 -bc_symmetry_y 3,4 -mu 75
87388626eedSJames Wright```
87488626eedSJames Wright
875019b7682STimothy Aiken#### Channel flow
876019b7682STimothy Aiken
877061ff11eSJames WrightThe Channel problem has the following command-line options in addition to the Newtonian Ideal Gas options:
87888626eedSJames Wright
87988626eedSJames Wright:::{list-table} Channel Runtime Options
88088626eedSJames Wright:header-rows: 1
88188626eedSJames Wright
88288626eedSJames Wright* - Option
88388626eedSJames Wright  - Description
88488626eedSJames Wright  - Default value
88588626eedSJames Wright  - Unit
88688626eedSJames Wright
88788626eedSJames Wright* - `-umax`
88888626eedSJames Wright  - Maximum/centerline velocity of the flow
88988626eedSJames Wright  - `10`
89088626eedSJames Wright  - `m/s`
89188626eedSJames Wright
89288626eedSJames Wright* - `-theta0`
89388626eedSJames Wright  - Reference potential temperature
89488626eedSJames Wright  - `300`
89588626eedSJames Wright  - `K`
89688626eedSJames Wright
89788626eedSJames Wright* - `-P0`
89888626eedSJames Wright  - Atmospheric pressure
89988626eedSJames Wright  - `1E5`
90088626eedSJames Wright  - `Pa`
901a1df05f8SJed Brown
902a1df05f8SJed Brown* - `-body_force_scale`
903a1df05f8SJed Brown  - Multiplier for body force (`-1` for flow reversal)
904a1df05f8SJed Brown  - 1
905a1df05f8SJed Brown  -
90688626eedSJames Wright:::
90788626eedSJames Wright
90888626eedSJames WrightThis problem can be run with the `channel.yaml` file via:
90988626eedSJames Wright
91088626eedSJames Wright```
91188626eedSJames Wright./navierstokes -options_file channel.yaml
91288626eedSJames Wright```
91388626eedSJames Wright```{literalinclude} ../../../../../examples/fluids/channel.yaml
91488626eedSJames Wright:language: yaml
91588626eedSJames Wright```
91688626eedSJames Wright
9178a94a473SJed Brown(example-blasius)=
9188a94a473SJed Brown
919019b7682STimothy Aiken#### Blasius boundary layer
920019b7682STimothy Aiken
921061ff11eSJames WrightThe Blasius problem has the following command-line options in addition to the Newtonian Ideal Gas options:
92288626eedSJames Wright
92388626eedSJames Wright:::{list-table} Blasius Runtime Options
92488626eedSJames Wright:header-rows: 1
92588626eedSJames Wright
92688626eedSJames Wright* - Option
92788626eedSJames Wright  - Description
92888626eedSJames Wright  - Default value
92988626eedSJames Wright  - Unit
93088626eedSJames Wright
931fb455ff0SLeila Ghaffari* - `-velocity_infinity`
93288626eedSJames Wright  - Freestream velocity
93388626eedSJames Wright  - `40`
93488626eedSJames Wright  - `m/s`
93588626eedSJames Wright
936fb455ff0SLeila Ghaffari* - `-temperature_infinity`
937fb455ff0SLeila Ghaffari  - Freestream temperature
93888626eedSJames Wright  - `288`
93988626eedSJames Wright  - `K`
94088626eedSJames Wright
941fb455ff0SLeila Ghaffari* - `-temperature_wall`
942fb455ff0SLeila Ghaffari  - Wall temperature
94307d14e58SLeila Ghaffari  - `288`
944fb455ff0SLeila Ghaffari  - `K`
945fb455ff0SLeila Ghaffari
946fb455ff0SLeila Ghaffari* - `-delta0`
947fb455ff0SLeila Ghaffari  - Boundary layer height at the inflow
948fb455ff0SLeila Ghaffari  - `4.2e-3`
949fb455ff0SLeila Ghaffari  - `m`
950fb455ff0SLeila Ghaffari
95188626eedSJames Wright* - `-P0`
95288626eedSJames Wright  - Atmospheric pressure
95388626eedSJames Wright  - `1.01E5`
95488626eedSJames Wright  - `Pa`
95588626eedSJames Wright
9569309e21cSJames Wright* - `-platemesh_modify_mesh`
9579309e21cSJames Wright  - Whether to modify the mesh using the given options below.
9589309e21cSJames Wright  - `false`
9599309e21cSJames Wright  -
9609309e21cSJames Wright
96191eaef80SJames Wright* - `-platemesh_refine_height`
96291eaef80SJames Wright  - Height at which `-platemesh_Ndelta` number of elements should refined into
96388626eedSJames Wright  - `5.9E-4`
96488626eedSJames Wright  - `m`
96588626eedSJames Wright
96691eaef80SJames Wright* - `-platemesh_Ndelta`
96791eaef80SJames Wright  - Number of elements to keep below `-platemesh_refine_height`
96888626eedSJames Wright  - `45`
96988626eedSJames Wright  -
97088626eedSJames Wright
97191eaef80SJames Wright* - `-platemesh_growth`
97288626eedSJames Wright  - Growth rate of the elements in the refinement region
97388626eedSJames Wright  - `1.08`
97488626eedSJames Wright  -
97588626eedSJames Wright
97691eaef80SJames Wright* - `-platemesh_top_angle`
97788626eedSJames Wright  - Downward angle of the top face of the domain. This face serves as an outlet.
97888626eedSJames Wright  - `5`
97988626eedSJames Wright  - `degrees`
980ba6664aeSJames Wright
98191eaef80SJames Wright* - `-platemesh_y_node_locs_path`
98291eaef80SJames Wright  - Path to file with y node locations. If empty, will use mesh warping instead.
98391eaef80SJames Wright  - `""`
98491eaef80SJames Wright  -
985fb455ff0SLeila Ghaffari
9869309e21cSJames Wright* - `-stg_use`
9879309e21cSJames Wright  - Whether to use STG for the inflow conditions
9889309e21cSJames Wright  - `false`
9899309e21cSJames Wright  -
9909309e21cSJames Wright
99107d14e58SLeila Ghaffari* - `-n_chebyshev`
992fb455ff0SLeila Ghaffari  - Number of Chebyshev terms
993fb455ff0SLeila Ghaffari  - `20`
994fb455ff0SLeila Ghaffari  -
995fb455ff0SLeila Ghaffari
99607d14e58SLeila Ghaffari* - `-chebyshev_`
99707d14e58SLeila Ghaffari  - Prefix for Chebyshev snes solve
99807d14e58SLeila Ghaffari  -
99907d14e58SLeila Ghaffari  -
100007d14e58SLeila Ghaffari
100188626eedSJames Wright:::
100288626eedSJames Wright
100388626eedSJames WrightThis problem can be run with the `blasius.yaml` file via:
100488626eedSJames Wright
100588626eedSJames Wright```
100688626eedSJames Wright./navierstokes -options_file blasius.yaml
100788626eedSJames Wright```
100888626eedSJames Wright
100988626eedSJames Wright```{literalinclude} ../../../../../examples/fluids/blasius.yaml
101088626eedSJames Wright:language: yaml
1011bc7bbd5dSLeila Ghaffari```
1012ba6664aeSJames Wright
1013ba6664aeSJames Wright#### STG Inflow for Flat Plate
1014ba6664aeSJames Wright
101517be3a41SJeremy L ThompsonUsing the STG Inflow for the blasius problem adds the following command-line options:
1016ba6664aeSJames Wright
1017ba6664aeSJames Wright:::{list-table} Blasius Runtime Options
1018ba6664aeSJames Wright:header-rows: 1
1019ba6664aeSJames Wright
1020ba6664aeSJames Wright* - Option
1021ba6664aeSJames Wright  - Description
1022ba6664aeSJames Wright  - Default value
1023ba6664aeSJames Wright  - Unit
1024ba6664aeSJames Wright
1025ba6664aeSJames Wright* - `-stg_inflow_path`
1026ba6664aeSJames Wright  - Path to the STGInflow file
1027ba6664aeSJames Wright  - `./STGInflow.dat`
1028ba6664aeSJames Wright  -
1029ba6664aeSJames Wright
1030ba6664aeSJames Wright* - `-stg_rand_path`
1031ba6664aeSJames Wright  - Path to the STGRand file
1032ba6664aeSJames Wright  - `./STGRand.dat`
1033ba6664aeSJames Wright  -
1034ba6664aeSJames Wright
1035ba6664aeSJames Wright* - `-stg_alpha`
1036ba6664aeSJames Wright  - Growth rate of the wavemodes
1037ba6664aeSJames Wright  - `1.01`
1038ba6664aeSJames Wright  -
1039ba6664aeSJames Wright
1040ba6664aeSJames Wright* - `-stg_u0`
1041ba6664aeSJames Wright  - Convective velocity, $U_0$
1042ba6664aeSJames Wright  - `0.0`
1043ba6664aeSJames Wright  - `m/s`
1044ba6664aeSJames Wright
1045ba6664aeSJames Wright* - `-stg_mean_only`
1046ba6664aeSJames Wright  - Only impose the mean velocity (no fluctutations)
1047ba6664aeSJames Wright  - `false`
1048ba6664aeSJames Wright  -
1049ba6664aeSJames Wright
105030af3636SJames Wright* - `-stg_strong`
105130af3636SJames Wright  - Strongly enforce the STG inflow boundary condition
105230af3636SJames Wright  - `false`
105330af3636SJames Wright  -
105430af3636SJames Wright
105589060322SJames Wright* - `-stg_fluctuating_IC`
105689060322SJames Wright  - "Extrude" the fluctuations through the domain as an initial condition
105789060322SJames Wright  - `false`
105889060322SJames Wright  -
105989060322SJames Wright
1060ba6664aeSJames Wright:::
1061ba6664aeSJames Wright
1062ba6664aeSJames WrightThis problem can be run with the `blasius.yaml` file via:
1063ba6664aeSJames Wright
1064ba6664aeSJames Wright```
1065ba6664aeSJames Wright./navierstokes -options_file blasius.yaml -stg_use true
1066ba6664aeSJames Wright```
1067ba6664aeSJames Wright
106817be3a41SJeremy L ThompsonNote the added `-stg_use true` flag
106917be3a41SJeremy L ThompsonThis overrides the `stg: use: false` setting in the `blasius.yaml` file, enabling the use of the STG inflow.
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