1ea10196cSJeremy L Thompson## libCEED: Navier-Stokes Example 2ea10196cSJeremy L Thompson 3ea10196cSJeremy L ThompsonThis page provides a description of the Navier-Stokes example for the libCEED library, based on PETSc. 4ea10196cSJeremy L Thompson 5ea10196cSJeremy L ThompsonThe Navier-Stokes problem solves the compressible Navier-Stokes equations in three dimensions using an 6ea10196cSJeremy L Thompsonexplicit time integration. The state variables are mass density, momentum density, and energy density. 7ea10196cSJeremy L Thompson 8ea10196cSJeremy L ThompsonThe main Navier-Stokes solver for libCEED is defined in [`navierstokes.c`](navierstokes.c) 9ea10196cSJeremy L Thompsonwith different problem definitions according to the application of interest. 10ea10196cSJeremy L Thompson 11ea10196cSJeremy L ThompsonBuild by using 12ea10196cSJeremy L Thompson 13ea10196cSJeremy L Thompson`make` 14ea10196cSJeremy L Thompson 15ea10196cSJeremy L Thompsonand run with 16ea10196cSJeremy L Thompson 1740f3b208SJed Brown`./navierstokes` 18ea10196cSJeremy L Thompson 19ea10196cSJeremy L ThompsonAvailable runtime options are: 20ea10196cSJeremy L Thompson 21ea10196cSJeremy L Thompson| Option | Meaning | 22ea10196cSJeremy L Thompson| :----------------------- | :-----------------------------------------------------------------------------------------------| 23ea10196cSJeremy L Thompson| `-ceed` | CEED resource specifier | 24ea10196cSJeremy L Thompson| `-test` | Run in test mode | 25ea10196cSJeremy L Thompson| `-problem` | Problem to solve (`advection`, `advection2d`, or `density_current`) | 26ea10196cSJeremy L Thompson| `-stab` | Stabilization method | 27ea10196cSJeremy L Thompson| `-implicit` | Use implicit time integartor formulation | 28ea10196cSJeremy L Thompson| `-bc_wall` | Use wall boundary conditions on this list of faces | 29ea10196cSJeremy L Thompson| `-bc_slip_x` | Use slip boundary conditions, for the x component, on this list of faces | 30ea10196cSJeremy L Thompson| `-bc_slip_y` | Use slip boundary conditions, for the y component, on this list of faces | 31ea10196cSJeremy L Thompson| `-bc_slip_z` | Use slip boundary conditions, for the z component, on this list of faces | 32ea10196cSJeremy L Thompson| `-viz_refine` | Use regular refinement for visualization | 3340f3b208SJed Brown| `-degree` | Polynomial degree of tensor product basis (must be >= 1) | 34ea10196cSJeremy L Thompson| `-units_meter` | 1 meter in scaled length units | 35ea10196cSJeremy L Thompson| `-units_second` | 1 second in scaled time units | 36ea10196cSJeremy L Thompson| `-units_kilogram` | 1 kilogram in scaled mass units | 37ea10196cSJeremy L Thompson| `-units_Kelvin` | 1 Kelvin in scaled temperature units | 38ea10196cSJeremy L Thompson| `-theta0` | Reference potential temperature | 39ea10196cSJeremy L Thompson| `-thetaC` | Perturbation of potential temperature | 40ea10196cSJeremy L Thompson| `-P0` | Atmospheric pressure | 41ea10196cSJeremy L Thompson| `-N` | Brunt-Vaisala frequency | 42ea10196cSJeremy L Thompson| `-cv` | Heat capacity at constant volume | 43ea10196cSJeremy L Thompson| `-cp` | Heat capacity at constant pressure | 44ea10196cSJeremy L Thompson| `-g` | Gravitational acceleration | 45ea10196cSJeremy L Thompson| `-lambda` | Stokes hypothesis second viscosity coefficient | 46ea10196cSJeremy L Thompson| `-mu` | Shear dynamic viscosity coefficient | 47ea10196cSJeremy L Thompson| `-k` | Thermal conductivity | 48ea10196cSJeremy L Thompson| `-CtauS` | Scale coefficient for stabilization tau (nondimensional) | 49ea10196cSJeremy L Thompson| `-strong_form` | Strong (1) or weak/integrated by parts (0) advection residual | 50ea10196cSJeremy L Thompson| `-lx` | Length scale in x direction | 51ea10196cSJeremy L Thompson| `-ly` | Length scale in y direction | 52ea10196cSJeremy L Thompson| `-lz` | Length scale in z direction | 53ea10196cSJeremy L Thompson| `-rc` | Characteristic radius of thermal bubble | 54ea10196cSJeremy L Thompson| `-resx` | Resolution in x | 55ea10196cSJeremy L Thompson| `-resy` | Resolution in y | 56ea10196cSJeremy L Thompson| `-resz` | Resolution in z | 57ea10196cSJeremy L Thompson| `-center` | Location of bubble center | 58ea10196cSJeremy L Thompson| `-dc_axis` | Axis of density current cylindrical anomaly, or {0,0,0} for spherically symmetric | 59ea10196cSJeremy L Thompson| `-output_freq` | Frequency of output, in number of steps | 60ea10196cSJeremy L Thompson| `-continue` | Continue from previous solution | 61ea10196cSJeremy L Thompson| `-degree` | Polynomial degree of tensor product basis | 62ea10196cSJeremy L Thompson| `-qextra` | Number of extra quadrature points | 63ea10196cSJeremy L Thompson| `-of` | Output folder | 64ea10196cSJeremy L Thompson 65682b106eSvaleriabarraFor the case of a square/cubic mesh, the list of face indices to be used with `-bc_wall` and/or `-bc_slip_x`, 66*a240d89fSLeila Ghaffari`-bc_slip_y`, and `-bc_slip_z` are: 67682b106eSvaleriabarra 68682b106eSvaleriabarra* 2D: 69682b106eSvaleriabarra - faceMarkerBottom = 1; 70682b106eSvaleriabarra - faceMarkerRight = 2; 71682b106eSvaleriabarra - faceMarkerTop = 3; 72682b106eSvaleriabarra - faceMarkerLeft = 4; 73682b106eSvaleriabarra* 3D: 74682b106eSvaleriabarra - faceMarkerBottom = 1; 75682b106eSvaleriabarra - faceMarkerTop = 2; 76682b106eSvaleriabarra - faceMarkerFront = 3; 77682b106eSvaleriabarra - faceMarkerBack = 4; 78682b106eSvaleriabarra - faceMarkerRight = 5; 79682b106eSvaleriabarra - faceMarkerLeft = 6; 80ea10196cSJeremy L Thompson 81ea10196cSJeremy L Thompson### Advection 82ea10196cSJeremy L Thompson 83ea10196cSJeremy L ThompsonThis problem solves the convection (advection) equation for the total (scalar) energy density, 84ea10196cSJeremy L Thompsontransported by the (vector) velocity field. 85ea10196cSJeremy L Thompson 86ea10196cSJeremy L ThompsonThis is 3D advection given in two formulations based upon the weak form. 87ea10196cSJeremy L Thompson 88ea10196cSJeremy L ThompsonState Variables: 89ea10196cSJeremy L Thompson 90ea10196cSJeremy L Thompson *q = ( rho, U<sub>1</sub>, U<sub>2</sub>, U<sub>3</sub>, E )* 91ea10196cSJeremy L Thompson 92ea10196cSJeremy L Thompson *rho* - Mass Density 93ea10196cSJeremy L Thompson 94ea10196cSJeremy L Thompson *U<sub>i</sub>* - Momentum Density , *U<sub>i</sub> = rho ui* 95ea10196cSJeremy L Thompson 96ea10196cSJeremy L Thompson *E* - Total Energy Density, *E = rho Cv T + rho (u u) / 2 + rho g z* 97ea10196cSJeremy L Thompson 98ea10196cSJeremy L ThompsonAdvection Equation: 99ea10196cSJeremy L Thompson 100ea10196cSJeremy L Thompson *dE/dt + div( E _u_ ) = 0* 101ea10196cSJeremy L Thompson 102ea10196cSJeremy L Thompson#### Initial Conditions 103ea10196cSJeremy L Thompson 104ea10196cSJeremy L ThompsonMass Density: 105ea10196cSJeremy L Thompson Constant mass density of 1.0 106ea10196cSJeremy L Thompson 107ea10196cSJeremy L ThompsonMomentum Density: 108ea10196cSJeremy L Thompson Rotational field in x,y with no momentum in z 109ea10196cSJeremy L Thompson 110ea10196cSJeremy L ThompsonEnergy Density: 111ea10196cSJeremy L Thompson Maximum of 1. x0 decreasing linearly to 0. as radial distance increases 112ea10196cSJeremy L Thompson to 1/8, then 0. everywhere else 113ea10196cSJeremy L Thompson 114ea10196cSJeremy L Thompson#### Boundary Conditions 115ea10196cSJeremy L Thompson 116ea10196cSJeremy L ThompsonMass Density: 117ea10196cSJeremy L Thompson 0.0 flux 118ea10196cSJeremy L Thompson 119ea10196cSJeremy L ThompsonMomentum Density: 120ea10196cSJeremy L Thompson 0.0 121ea10196cSJeremy L Thompson 122ea10196cSJeremy L ThompsonEnergy Density: 123ea10196cSJeremy L Thompson 0.0 flux 124ea10196cSJeremy L Thompson 125ea10196cSJeremy L Thompson### Density Current 126ea10196cSJeremy L Thompson 127ea10196cSJeremy L ThompsonThis problem solves the full compressible Navier-Stokes equations, using 128ea10196cSJeremy L Thompsonoperator composition and design of coupled solvers in the context of atmospheric 129ea10196cSJeremy L Thompsonmodeling. This problem uses the formulation given in Semi-Implicit Formulations 130ea10196cSJeremy L Thompsonof the Navier-Stokes Equations: Application to Nonhydrostatic Atmospheric Modeling, 131ea10196cSJeremy L ThompsonGiraldo, Restelli, and Lauter (2010). 132ea10196cSJeremy L Thompson 133ea10196cSJeremy L ThompsonThe 3D compressible Navier-Stokes equations are formulated in conservation form with state 134ea10196cSJeremy L Thompsonvariables of density, momentum density, and total energy density. 135ea10196cSJeremy L Thompson 136ea10196cSJeremy L ThompsonState Variables: 137ea10196cSJeremy L Thompson 138ea10196cSJeremy L Thompson *q = ( rho, U<sub>1</sub>, U<sub>2</sub>, U<sub>3</sub>, E )* 139ea10196cSJeremy L Thompson 140ea10196cSJeremy L Thompson *rho* - Mass Density 141ea10196cSJeremy L Thompson 142ea10196cSJeremy L Thompson *U<sub>i</sub>* - Momentum Density , *U<sub>i</sub> = rho u<sub>i</sub>* 143ea10196cSJeremy L Thompson 144ea10196cSJeremy L Thompson *E* - Total Energy Density, *E = rho c<sub>v</sub> T + rho (u u) / 2 + rho g z* 145ea10196cSJeremy L Thompson 146ea10196cSJeremy L ThompsonNavier-Stokes Equations: 147ea10196cSJeremy L Thompson 148ea10196cSJeremy L Thompson *drho/dt + div( U ) = 0* 149ea10196cSJeremy L Thompson 150ea10196cSJeremy L Thompson *dU/dt + div( rho (u x u) + P I<sub>3</sub> ) + rho g khat = div( F<sub>u</sub> )* 151ea10196cSJeremy L Thompson 152ea10196cSJeremy L Thompson *dE/dt + div( (E + P) u ) = div( F<sub>e</sub> )* 153ea10196cSJeremy L Thompson 154ea10196cSJeremy L ThompsonViscous Stress: 155ea10196cSJeremy L Thompson 156ea10196cSJeremy L Thompson *F<sub>u</sub> = mu (grad( u ) + grad( u )^T + lambda div ( u ) I<sub>3</sub>)* 157ea10196cSJeremy L Thompson 158ea10196cSJeremy L ThompsonThermal Stress: 159ea10196cSJeremy L Thompson 160ea10196cSJeremy L Thompson *F<sub>e</sub> = u F<sub>u</sub> + k grad( T )* 161ea10196cSJeremy L Thompson 162ea10196cSJeremy L ThompsonEquation of State: 163ea10196cSJeremy L Thompson 164ea10196cSJeremy L Thompson *P = (gamma - 1) (E - rho (u u) / 2 - rho g z)* 165ea10196cSJeremy L Thompson 166ea10196cSJeremy L ThompsonTemperature: 167ea10196cSJeremy L Thompson 168ea10196cSJeremy L Thompson *T = (E / rho - (u u) / 2 - g z) / c<sub>v</sub>* 169ea10196cSJeremy L Thompson 170ea10196cSJeremy L ThompsonConstants: 171ea10196cSJeremy L Thompson 172ea10196cSJeremy L Thompson *lambda = - 2 / 3*, From Stokes hypothesis 173ea10196cSJeremy L Thompson 174ea10196cSJeremy L Thompson *mu* , Dynamic viscosity 175ea10196cSJeremy L Thompson 176ea10196cSJeremy L Thompson *k* , Thermal conductivity 177ea10196cSJeremy L Thompson 178ea10196cSJeremy L Thompson *c<sub>v</sub>* , Specific heat, constant volume 179ea10196cSJeremy L Thompson 180ea10196cSJeremy L Thompson *c<sub>p</sub>* , Specific heat, constant pressure 181ea10196cSJeremy L Thompson 182ea10196cSJeremy L Thompson *g* , Gravity 183ea10196cSJeremy L Thompson 184ea10196cSJeremy L Thompson *gamma = c<sub>p</sub> / c<sub>v</sub>*, Specific heat ratio 185ea10196cSJeremy L Thompson 186ea10196cSJeremy L Thompson#### Initial Conditions 187ea10196cSJeremy L Thompson 188ea10196cSJeremy L ThompsonPotential Temperature: 189ea10196cSJeremy L Thompson 190ea10196cSJeremy L Thompson *theta = thetabar + deltatheta* 191ea10196cSJeremy L Thompson 192ea10196cSJeremy L Thompson *thetabar = theta0 exp( N * * 2 z / g )* 193ea10196cSJeremy L Thompson 194ea10196cSJeremy L Thompson *deltatheta = 195ea10196cSJeremy L Thompson r <= rc : theta0(1 + cos(pi r)) / 2 196ea10196cSJeremy L Thompson r > rc : 0* 197ea10196cSJeremy L Thompson 198ea10196cSJeremy L Thompson *r = sqrt( (x - xc) * * 2 + (y - yc) * * 2 + (z - zc) * * 2 )* 199ea10196cSJeremy L Thompson with *(xc,yc,zc)* center of domain 200ea10196cSJeremy L Thompson 201ea10196cSJeremy L ThompsonExner Pressure: 202ea10196cSJeremy L Thompson 203ea10196cSJeremy L Thompson *Pi = Pibar + deltaPi* 204ea10196cSJeremy L Thompson 205ea10196cSJeremy L Thompson *Pibar = g * * 2 (exp( - N * * 2 z / g ) - 1) / (cp theta0 N * * 2)* 206ea10196cSJeremy L Thompson 207ea10196cSJeremy L Thompson *deltaPi = 0* (hydrostatic balance) 208ea10196cSJeremy L Thompson 209ea10196cSJeremy L ThompsonVelocity/Momentum Density: 210ea10196cSJeremy L Thompson 211ea10196cSJeremy L Thompson *U<sub>i</sub> = u<sub>i</sub> = 0* 212ea10196cSJeremy L Thompson 213ea10196cSJeremy L ThompsonConversion to Conserved Variables: 214ea10196cSJeremy L Thompson 215ea10196cSJeremy L Thompson *rho = P0 Pi**(c<sub>v</sub>/R<sub>d</sub>) / (R<sub>d</sub> theta)* 216ea10196cSJeremy L Thompson 217ea10196cSJeremy L Thompson *E = rho (c<sub>v</sub> theta Pi + (u u)/2 + g z)* 218ea10196cSJeremy L Thompson 219ea10196cSJeremy L ThompsonConstants: 220ea10196cSJeremy L Thompson 221ea10196cSJeremy L Thompson *theta0* , Potential temperature constant 222ea10196cSJeremy L Thompson 223ea10196cSJeremy L Thompson *thetaC* , Potential temperature perturbation 224ea10196cSJeremy L Thompson 225ea10196cSJeremy L Thompson *P0* , Pressure at the surface 226ea10196cSJeremy L Thompson 227ea10196cSJeremy L Thompson *N* , Brunt-Vaisala frequency 228ea10196cSJeremy L Thompson 229ea10196cSJeremy L Thompson *c<sub>v</sub>* , Specific heat, constant volume 230ea10196cSJeremy L Thompson 231ea10196cSJeremy L Thompson *c<sub>p</sub>* , Specific heat, constant pressure 232ea10196cSJeremy L Thompson 233ea10196cSJeremy L Thompson *R<sub>d</sub>* = c<sub>p</sub> - c<sub>v</sub>, Specific heat difference 234ea10196cSJeremy L Thompson 235ea10196cSJeremy L Thompson *g* , Gravity 236ea10196cSJeremy L Thompson 237ea10196cSJeremy L Thompson *r<sub>c</sub>* , Characteristic radius of thermal bubble 238ea10196cSJeremy L Thompson 239ea10196cSJeremy L Thompson *l<sub>x</sub>* , Characteristic length scale of domain in x 240ea10196cSJeremy L Thompson 241ea10196cSJeremy L Thompson *l<sub>y</sub>* , Characteristic length scale of domain in y 242ea10196cSJeremy L Thompson 243ea10196cSJeremy L Thompson *l<sub>z</sub>* , Characteristic length scale of domain in z 244ea10196cSJeremy L Thompson 245ea10196cSJeremy L Thompson 246ea10196cSJeremy L Thompson#### Boundary Conditions 247ea10196cSJeremy L Thompson 248ea10196cSJeremy L ThompsonMass Density: 249ea10196cSJeremy L Thompson 0.0 flux 250ea10196cSJeremy L Thompson 251ea10196cSJeremy L ThompsonMomentum Density: 252ea10196cSJeremy L Thompson 0.0 253ea10196cSJeremy L Thompson 254ea10196cSJeremy L ThompsonEnergy Density: 255ea10196cSJeremy L Thompson 0.0 flux 256ea10196cSJeremy L Thompson 257ea10196cSJeremy L Thompson### Time Discretization 258ea10196cSJeremy L Thompson 259682b106eSvaleriabarraFor all different problems, the time integration is performed with an explicit 260682b106eSvaleriabarraor implicit formulation. 261ea10196cSJeremy L Thompson 262ea10196cSJeremy L Thompson### Space Discretization 263ea10196cSJeremy L Thompson 264ea10196cSJeremy L ThompsonThe geometric factors and coordinate transformations required for the integration of the weak form 265ea10196cSJeremy L Thompsonare described in the file [`common.h`](common.h) 266