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. 4ccaff030SJeremy L Thompson 5ccaff030SJeremy L ThompsonThe Navier-Stokes problem solves the compressible Navier-Stokes equations in three dimensions using an 6ccaff030SJeremy L Thompsonexplicit time integration. The state variables are mass density, momentum density, and energy density. 7ccaff030SJeremy L Thompson 8ccaff030SJeremy L ThompsonThe main Navier-Stokes solver for libCEED is defined in [`navierstokes.c`](navierstokes.c) 9ccaff030SJeremy L Thompsonwith different problem definitions according to the application of interest. 10ccaff030SJeremy L Thompson 11ccaff030SJeremy L ThompsonBuild by using 12ccaff030SJeremy L Thompson 13ccaff030SJeremy L Thompson`make` 14ccaff030SJeremy L Thompson 15ccaff030SJeremy L Thompsonand run with 16ccaff030SJeremy L Thompson 17ff6701fcSJed Brown`./navierstokes` 18ccaff030SJeremy L Thompson 19ccaff030SJeremy L ThompsonAvailable runtime options are: 20ccaff030SJeremy L Thompson 21ccaff030SJeremy L Thompson| Option | Meaning | 22ccaff030SJeremy L Thompson| :----------------------- | :-----------------------------------------------------------------------------------------------| 23ccaff030SJeremy L Thompson| `-ceed` | CEED resource specifier | 24ccaff030SJeremy L Thompson| `-test` | Run in test mode | 25ccaff030SJeremy L Thompson| `-problem` | Problem to solve (`advection`, `advection2d`, or `density_current`) | 26ccaff030SJeremy L Thompson| `-stab` | Stabilization method | 27ccaff030SJeremy L Thompson| `-implicit` | Use implicit time integartor formulation | 28ccaff030SJeremy L Thompson| `-bc_wall` | Use wall boundary conditions on this list of faces | 29ccaff030SJeremy L Thompson| `-bc_slip_x` | Use slip boundary conditions, for the x component, on this list of faces | 30ccaff030SJeremy L Thompson| `-bc_slip_y` | Use slip boundary conditions, for the y component, on this list of faces | 31ccaff030SJeremy L Thompson| `-bc_slip_z` | Use slip boundary conditions, for the z component, on this list of faces | 32ccaff030SJeremy L Thompson| `-viz_refine` | Use regular refinement for visualization | 33ff6701fcSJed Brown| `-degree` | Polynomial degree of tensor product basis (must be >= 1) | 34ccaff030SJeremy L Thompson| `-units_meter` | 1 meter in scaled length units | 35ccaff030SJeremy L Thompson| `-units_second` | 1 second in scaled time units | 36ccaff030SJeremy L Thompson| `-units_kilogram` | 1 kilogram in scaled mass units | 37ccaff030SJeremy L Thompson| `-units_Kelvin` | 1 Kelvin in scaled temperature units | 38ccaff030SJeremy L Thompson| `-theta0` | Reference potential temperature | 39ccaff030SJeremy L Thompson| `-thetaC` | Perturbation of potential temperature | 40ccaff030SJeremy L Thompson| `-P0` | Atmospheric pressure | 41ccaff030SJeremy L Thompson| `-N` | Brunt-Vaisala frequency | 42ccaff030SJeremy L Thompson| `-cv` | Heat capacity at constant volume | 43ccaff030SJeremy L Thompson| `-cp` | Heat capacity at constant pressure | 44ccaff030SJeremy L Thompson| `-g` | Gravitational acceleration | 45ccaff030SJeremy L Thompson| `-lambda` | Stokes hypothesis second viscosity coefficient | 46ccaff030SJeremy L Thompson| `-mu` | Shear dynamic viscosity coefficient | 47ccaff030SJeremy L Thompson| `-k` | Thermal conductivity | 48ccaff030SJeremy L Thompson| `-CtauS` | Scale coefficient for stabilization tau (nondimensional) | 49ccaff030SJeremy L Thompson| `-strong_form` | Strong (1) or weak/integrated by parts (0) advection residual | 50ccaff030SJeremy L Thompson| `-lx` | Length scale in x direction | 51ccaff030SJeremy L Thompson| `-ly` | Length scale in y direction | 52ccaff030SJeremy L Thompson| `-lz` | Length scale in z direction | 53ccaff030SJeremy L Thompson| `-rc` | Characteristic radius of thermal bubble | 54ccaff030SJeremy L Thompson| `-resx` | Resolution in x | 55ccaff030SJeremy L Thompson| `-resy` | Resolution in y | 56ccaff030SJeremy L Thompson| `-resz` | Resolution in z | 57ccaff030SJeremy L Thompson| `-center` | Location of bubble center | 58ccaff030SJeremy L Thompson| `-dc_axis` | Axis of density current cylindrical anomaly, or {0,0,0} for spherically symmetric | 59ccaff030SJeremy L Thompson| `-output_freq` | Frequency of output, in number of steps | 60ccaff030SJeremy L Thompson| `-continue` | Continue from previous solution | 61ccaff030SJeremy L Thompson| `-degree` | Polynomial degree of tensor product basis | 62ccaff030SJeremy L Thompson| `-qextra` | Number of extra quadrature points | 63ccaff030SJeremy L Thompson| `-of` | Output folder | 64ccaff030SJeremy L Thompson 65*c063f476SvaleriabarraFor the case of a square/cubic mesh, the list of face indices to be used with `-bc_wall` and/or `-bc_slip_x`, 66*c063f476Svaleriabarra`-bc_slip_y`, and `-bc_slip_z` are: 67*c063f476Svaleriabarra 68*c063f476Svaleriabarra* 2D: 69*c063f476Svaleriabarra - faceMarkerBottom = 1; 70*c063f476Svaleriabarra - faceMarkerRight = 2; 71*c063f476Svaleriabarra - faceMarkerTop = 3; 72*c063f476Svaleriabarra - faceMarkerLeft = 4; 73*c063f476Svaleriabarra* 3D: 74*c063f476Svaleriabarra - faceMarkerBottom = 1; 75*c063f476Svaleriabarra - faceMarkerTop = 2; 76*c063f476Svaleriabarra - faceMarkerFront = 3; 77*c063f476Svaleriabarra - faceMarkerBack = 4; 78*c063f476Svaleriabarra - faceMarkerRight = 5; 79*c063f476Svaleriabarra - faceMarkerLeft = 6; 80ccaff030SJeremy L Thompson 81ccaff030SJeremy L Thompson### Advection 82ccaff030SJeremy L Thompson 83ccaff030SJeremy L ThompsonThis problem solves the convection (advection) equation for the total (scalar) energy density, 84ccaff030SJeremy L Thompsontransported by the (vector) velocity field. 85ccaff030SJeremy L Thompson 86ccaff030SJeremy L ThompsonThis is 3D advection given in two formulations based upon the weak form. 87ccaff030SJeremy L Thompson 88ccaff030SJeremy L ThompsonState Variables: 89ccaff030SJeremy L Thompson 90ccaff030SJeremy L Thompson *q = ( rho, U<sub>1</sub>, U<sub>2</sub>, U<sub>3</sub>, E )* 91ccaff030SJeremy L Thompson 92ccaff030SJeremy L Thompson *rho* - Mass Density 93ccaff030SJeremy L Thompson 94ccaff030SJeremy L Thompson *U<sub>i</sub>* - Momentum Density , *U<sub>i</sub> = rho ui* 95ccaff030SJeremy L Thompson 96ccaff030SJeremy L Thompson *E* - Total Energy Density, *E = rho Cv T + rho (u u) / 2 + rho g z* 97ccaff030SJeremy L Thompson 98ccaff030SJeremy L ThompsonAdvection Equation: 99ccaff030SJeremy L Thompson 100ccaff030SJeremy L Thompson *dE/dt + div( E _u_ ) = 0* 101ccaff030SJeremy L Thompson 102ccaff030SJeremy L Thompson#### Initial Conditions 103ccaff030SJeremy L Thompson 104ccaff030SJeremy L ThompsonMass Density: 105ccaff030SJeremy L Thompson Constant mass density of 1.0 106ccaff030SJeremy L Thompson 107ccaff030SJeremy L ThompsonMomentum Density: 108ccaff030SJeremy L Thompson Rotational field in x,y with no momentum in z 109ccaff030SJeremy L Thompson 110ccaff030SJeremy L ThompsonEnergy Density: 111ccaff030SJeremy L Thompson Maximum of 1. x0 decreasing linearly to 0. as radial distance increases 112ccaff030SJeremy L Thompson to 1/8, then 0. everywhere else 113ccaff030SJeremy L Thompson 114ccaff030SJeremy L Thompson#### Boundary Conditions 115ccaff030SJeremy L Thompson 116ccaff030SJeremy L ThompsonMass Density: 117ccaff030SJeremy L Thompson 0.0 flux 118ccaff030SJeremy L Thompson 119ccaff030SJeremy L ThompsonMomentum Density: 120ccaff030SJeremy L Thompson 0.0 121ccaff030SJeremy L Thompson 122ccaff030SJeremy L ThompsonEnergy Density: 123ccaff030SJeremy L Thompson 0.0 flux 124ccaff030SJeremy L Thompson 125ccaff030SJeremy L Thompson### Density Current 126ccaff030SJeremy L Thompson 127ccaff030SJeremy L ThompsonThis problem solves the full compressible Navier-Stokes equations, using 128ccaff030SJeremy L Thompsonoperator composition and design of coupled solvers in the context of atmospheric 129ccaff030SJeremy L Thompsonmodeling. This problem uses the formulation given in Semi-Implicit Formulations 130ccaff030SJeremy L Thompsonof the Navier-Stokes Equations: Application to Nonhydrostatic Atmospheric Modeling, 131ccaff030SJeremy L ThompsonGiraldo, Restelli, and Lauter (2010). 132ccaff030SJeremy L Thompson 133ccaff030SJeremy L ThompsonThe 3D compressible Navier-Stokes equations are formulated in conservation form with state 134ccaff030SJeremy L Thompsonvariables of density, momentum density, and total energy density. 135ccaff030SJeremy L Thompson 136ccaff030SJeremy L ThompsonState Variables: 137ccaff030SJeremy L Thompson 138ccaff030SJeremy L Thompson *q = ( rho, U<sub>1</sub>, U<sub>2</sub>, U<sub>3</sub>, E )* 139ccaff030SJeremy L Thompson 140ccaff030SJeremy L Thompson *rho* - Mass Density 141ccaff030SJeremy L Thompson 142ccaff030SJeremy L Thompson *U<sub>i</sub>* - Momentum Density , *U<sub>i</sub> = rho u<sub>i</sub>* 143ccaff030SJeremy L Thompson 144ccaff030SJeremy L Thompson *E* - Total Energy Density, *E = rho c<sub>v</sub> T + rho (u u) / 2 + rho g z* 145ccaff030SJeremy L Thompson 146ccaff030SJeremy L ThompsonNavier-Stokes Equations: 147ccaff030SJeremy L Thompson 148ccaff030SJeremy L Thompson *drho/dt + div( U ) = 0* 149ccaff030SJeremy L Thompson 150ccaff030SJeremy L Thompson *dU/dt + div( rho (u x u) + P I<sub>3</sub> ) + rho g khat = div( F<sub>u</sub> )* 151ccaff030SJeremy L Thompson 152ccaff030SJeremy L Thompson *dE/dt + div( (E + P) u ) = div( F<sub>e</sub> )* 153ccaff030SJeremy L Thompson 154ccaff030SJeremy L ThompsonViscous Stress: 155ccaff030SJeremy L Thompson 156ccaff030SJeremy L Thompson *F<sub>u</sub> = mu (grad( u ) + grad( u )^T + lambda div ( u ) I<sub>3</sub>)* 157ccaff030SJeremy L Thompson 158ccaff030SJeremy L ThompsonThermal Stress: 159ccaff030SJeremy L Thompson 160ccaff030SJeremy L Thompson *F<sub>e</sub> = u F<sub>u</sub> + k grad( T )* 161ccaff030SJeremy L Thompson 162ccaff030SJeremy L ThompsonEquation of State: 163ccaff030SJeremy L Thompson 164ccaff030SJeremy L Thompson *P = (gamma - 1) (E - rho (u u) / 2 - rho g z)* 165ccaff030SJeremy L Thompson 166ccaff030SJeremy L ThompsonTemperature: 167ccaff030SJeremy L Thompson 168ccaff030SJeremy L Thompson *T = (E / rho - (u u) / 2 - g z) / c<sub>v</sub>* 169ccaff030SJeremy L Thompson 170ccaff030SJeremy L ThompsonConstants: 171ccaff030SJeremy L Thompson 172ccaff030SJeremy L Thompson *lambda = - 2 / 3*, From Stokes hypothesis 173ccaff030SJeremy L Thompson 174ccaff030SJeremy L Thompson *mu* , Dynamic viscosity 175ccaff030SJeremy L Thompson 176ccaff030SJeremy L Thompson *k* , Thermal conductivity 177ccaff030SJeremy L Thompson 178ccaff030SJeremy L Thompson *c<sub>v</sub>* , Specific heat, constant volume 179ccaff030SJeremy L Thompson 180ccaff030SJeremy L Thompson *c<sub>p</sub>* , Specific heat, constant pressure 181ccaff030SJeremy L Thompson 182ccaff030SJeremy L Thompson *g* , Gravity 183ccaff030SJeremy L Thompson 184ccaff030SJeremy L Thompson *gamma = c<sub>p</sub> / c<sub>v</sub>*, Specific heat ratio 185ccaff030SJeremy L Thompson 186ccaff030SJeremy L Thompson#### Initial Conditions 187ccaff030SJeremy L Thompson 188ccaff030SJeremy L ThompsonPotential Temperature: 189ccaff030SJeremy L Thompson 190ccaff030SJeremy L Thompson *theta = thetabar + deltatheta* 191ccaff030SJeremy L Thompson 192ccaff030SJeremy L Thompson *thetabar = theta0 exp( N * * 2 z / g )* 193ccaff030SJeremy L Thompson 194ccaff030SJeremy L Thompson *deltatheta = 195ccaff030SJeremy L Thompson r <= rc : theta0(1 + cos(pi r)) / 2 196ccaff030SJeremy L Thompson r > rc : 0* 197ccaff030SJeremy L Thompson 198ccaff030SJeremy L Thompson *r = sqrt( (x - xc) * * 2 + (y - yc) * * 2 + (z - zc) * * 2 )* 199ccaff030SJeremy L Thompson with *(xc,yc,zc)* center of domain 200ccaff030SJeremy L Thompson 201ccaff030SJeremy L ThompsonExner Pressure: 202ccaff030SJeremy L Thompson 203ccaff030SJeremy L Thompson *Pi = Pibar + deltaPi* 204ccaff030SJeremy L Thompson 205ccaff030SJeremy L Thompson *Pibar = g * * 2 (exp( - N * * 2 z / g ) - 1) / (cp theta0 N * * 2)* 206ccaff030SJeremy L Thompson 207ccaff030SJeremy L Thompson *deltaPi = 0* (hydrostatic balance) 208ccaff030SJeremy L Thompson 209ccaff030SJeremy L ThompsonVelocity/Momentum Density: 210ccaff030SJeremy L Thompson 211ccaff030SJeremy L Thompson *U<sub>i</sub> = u<sub>i</sub> = 0* 212ccaff030SJeremy L Thompson 213ccaff030SJeremy L ThompsonConversion to Conserved Variables: 214ccaff030SJeremy L Thompson 215ccaff030SJeremy L Thompson *rho = P0 Pi**(c<sub>v</sub>/R<sub>d</sub>) / (R<sub>d</sub> theta)* 216ccaff030SJeremy L Thompson 217ccaff030SJeremy L Thompson *E = rho (c<sub>v</sub> theta Pi + (u u)/2 + g z)* 218ccaff030SJeremy L Thompson 219ccaff030SJeremy L ThompsonConstants: 220ccaff030SJeremy L Thompson 221ccaff030SJeremy L Thompson *theta0* , Potential temperature constant 222ccaff030SJeremy L Thompson 223ccaff030SJeremy L Thompson *thetaC* , Potential temperature perturbation 224ccaff030SJeremy L Thompson 225ccaff030SJeremy L Thompson *P0* , Pressure at the surface 226ccaff030SJeremy L Thompson 227ccaff030SJeremy L Thompson *N* , Brunt-Vaisala frequency 228ccaff030SJeremy L Thompson 229ccaff030SJeremy L Thompson *c<sub>v</sub>* , Specific heat, constant volume 230ccaff030SJeremy L Thompson 231ccaff030SJeremy L Thompson *c<sub>p</sub>* , Specific heat, constant pressure 232ccaff030SJeremy L Thompson 233ccaff030SJeremy L Thompson *R<sub>d</sub>* = c<sub>p</sub> - c<sub>v</sub>, Specific heat difference 234ccaff030SJeremy L Thompson 235ccaff030SJeremy L Thompson *g* , Gravity 236ccaff030SJeremy L Thompson 237ccaff030SJeremy L Thompson *r<sub>c</sub>* , Characteristic radius of thermal bubble 238ccaff030SJeremy L Thompson 239ccaff030SJeremy L Thompson *l<sub>x</sub>* , Characteristic length scale of domain in x 240ccaff030SJeremy L Thompson 241ccaff030SJeremy L Thompson *l<sub>y</sub>* , Characteristic length scale of domain in y 242ccaff030SJeremy L Thompson 243ccaff030SJeremy L Thompson *l<sub>z</sub>* , Characteristic length scale of domain in z 244ccaff030SJeremy L Thompson 245ccaff030SJeremy L Thompson 246ccaff030SJeremy L Thompson#### Boundary Conditions 247ccaff030SJeremy L Thompson 248ccaff030SJeremy L ThompsonMass Density: 249ccaff030SJeremy L Thompson 0.0 flux 250ccaff030SJeremy L Thompson 251ccaff030SJeremy L ThompsonMomentum Density: 252ccaff030SJeremy L Thompson 0.0 253ccaff030SJeremy L Thompson 254ccaff030SJeremy L ThompsonEnergy Density: 255ccaff030SJeremy L Thompson 0.0 flux 256ccaff030SJeremy L Thompson 257ccaff030SJeremy L Thompson### Time Discretization 258ccaff030SJeremy L Thompson 259*c063f476SvaleriabarraFor all different problems, the time integration is performed with an explicit 260*c063f476Svaleriabarraor implicit formulation. 261ccaff030SJeremy L Thompson 262ccaff030SJeremy L Thompson### Space Discretization 263ccaff030SJeremy L Thompson 264ccaff030SJeremy L ThompsonThe geometric factors and coordinate transformations required for the integration of the weak form 265ccaff030SJeremy L Thompsonare described in the file [`common.h`](common.h) 266