1bb8a0c61SJames Wright // Copyright (c) 2017-2022, Lawrence Livermore National Security, LLC and other CEED contributors. 2bb8a0c61SJames Wright // All Rights Reserved. See the top-level LICENSE and NOTICE files for details. 3bb8a0c61SJames Wright // 4bb8a0c61SJames Wright // SPDX-License-Identifier: BSD-2-Clause 5bb8a0c61SJames Wright // 6bb8a0c61SJames Wright // This file is part of CEED: http://github.com/ceed 7bb8a0c61SJames Wright 8bb8a0c61SJames Wright /// @file 9bb8a0c61SJames Wright /// Operator for Navier-Stokes example using PETSc 10bb8a0c61SJames Wright 11bb8a0c61SJames Wright #ifndef channel_h 12bb8a0c61SJames Wright #define channel_h 13bb8a0c61SJames Wright 14d0cce58aSJeremy L Thompson #include <ceed.h> 15bb8a0c61SJames Wright #include <math.h> 162b916ea7SJeremy L Thompson 17cbe60e31SLeila Ghaffari #include "newtonian_state.h" 18d0cce58aSJeremy L Thompson #include "newtonian_types.h" 19704b8bbeSJames Wright #include "utils.h" 20bb8a0c61SJames Wright 21bb8a0c61SJames Wright typedef struct ChannelContext_ *ChannelContext; 22bb8a0c61SJames Wright struct ChannelContext_ { 23bb8a0c61SJames Wright bool implicit; // !< Using implicit timesteping or not 24bb8a0c61SJames Wright CeedScalar theta0; // !< Reference temperature 25bb8a0c61SJames Wright CeedScalar P0; // !< Reference Pressure 26bb8a0c61SJames Wright CeedScalar umax; // !< Centerline velocity 27bb8a0c61SJames Wright CeedScalar center; // !< Y Coordinate for center of channel 28bb8a0c61SJames Wright CeedScalar H; // !< Channel half-height 29bb8a0c61SJames Wright CeedScalar B; // !< Body-force driving the flow 30bb8a0c61SJames Wright struct NewtonianIdealGasContext_ newtonian_ctx; 31bb8a0c61SJames Wright }; 32bb8a0c61SJames Wright 332b916ea7SJeremy L Thompson CEED_QFUNCTION_HELPER State Exact_Channel(CeedInt dim, CeedScalar time, const CeedScalar X[], CeedInt Nf, void *ctx) { 34bb8a0c61SJames Wright const ChannelContext context = (ChannelContext)ctx; 35bb8a0c61SJames Wright const CeedScalar theta0 = context->theta0; 36bb8a0c61SJames Wright const CeedScalar P0 = context->P0; 37bb8a0c61SJames Wright const CeedScalar umax = context->umax; 38bb8a0c61SJames Wright const CeedScalar center = context->center; 39bb8a0c61SJames Wright const CeedScalar H = context->H; 40cbe60e31SLeila Ghaffari NewtonianIdealGasContext gas = &context->newtonian_ctx; 41cbe60e31SLeila Ghaffari const CeedScalar cp = gas->cp; 42cbe60e31SLeila Ghaffari const CeedScalar mu = gas->mu; 43cbe60e31SLeila Ghaffari const CeedScalar k = gas->k; 44cbe60e31SLeila Ghaffari // There is a gravity body force but it is excluded from 45cbe60e31SLeila Ghaffari // the potential energy due to periodicity. 46d1b9ef12SLeila Ghaffari // g = (g, 0, 0) 47d1b9ef12SLeila Ghaffari // x = (0, x_2, x_3) 48d1b9ef12SLeila Ghaffari // e_potential = dot(g, x) = 0 49d1b9ef12SLeila Ghaffari const CeedScalar x[3] = {0, X[1], X[2]}; 50bb8a0c61SJames Wright 51bb8a0c61SJames Wright const CeedScalar Pr = mu / (cp * k); 52bb8a0c61SJames Wright const CeedScalar Ec = (umax * umax) / (cp * theta0); 532b916ea7SJeremy L Thompson const CeedScalar theta = theta0 * (1 + (Pr * Ec / 3) * (1 - Square(Square((x[1] - center) / H)))); 54cbe60e31SLeila Ghaffari CeedScalar Y[5] = {0.}; 55cbe60e31SLeila Ghaffari Y[0] = P0; 56d1b9ef12SLeila Ghaffari Y[1] = umax * (1 - Square((x[1] - center) / H)); 57cbe60e31SLeila Ghaffari Y[2] = 0.; 58cbe60e31SLeila Ghaffari Y[3] = 0.; 59cbe60e31SLeila Ghaffari Y[4] = theta; 60bb8a0c61SJames Wright 61d1b9ef12SLeila Ghaffari return StateFromY(gas, Y, x); 62bb8a0c61SJames Wright } 63bb8a0c61SJames Wright 64bb8a0c61SJames Wright // ***************************************************************************** 65cbe60e31SLeila Ghaffari // This QFunction set the initial condition 66bb8a0c61SJames Wright // ***************************************************************************** 672b916ea7SJeremy L Thompson CEED_QFUNCTION(ICsChannel)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 68bb8a0c61SJames Wright // Inputs 69bb8a0c61SJames Wright const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 70bb8a0c61SJames Wright 71bb8a0c61SJames Wright // Outputs 72bb8a0c61SJames Wright CeedScalar(*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 73bb8a0c61SJames Wright 74cbe60e31SLeila Ghaffari // Context 75cbe60e31SLeila Ghaffari const ChannelContext context = (ChannelContext)ctx; 76cbe60e31SLeila Ghaffari 77bb8a0c61SJames Wright // Quadrature Point Loop 782b916ea7SJeremy L Thompson CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 79bb8a0c61SJames Wright const CeedScalar x[] = {X[0][i], X[1][i], X[2][i]}; 80cbe60e31SLeila Ghaffari State s = Exact_Channel(3, 0., x, 5, ctx); 81d1b9ef12SLeila Ghaffari CeedScalar q[5] = {0}; 823636f6a4SJames Wright switch (context->newtonian_ctx.state_var) { 833636f6a4SJames Wright case STATEVAR_CONSERVATIVE: 84d1b9ef12SLeila Ghaffari UnpackState_U(s.U, q); 853636f6a4SJames Wright break; 863636f6a4SJames Wright case STATEVAR_PRIMITIVE: 873636f6a4SJames Wright UnpackState_Y(s.Y, q); 883636f6a4SJames Wright break; 893636f6a4SJames Wright } 90d1b9ef12SLeila Ghaffari 912b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 5; j++) q0[j][i] = q[j]; 92bb8a0c61SJames Wright 93bb8a0c61SJames Wright } // End of Quadrature Point Loop 94bb8a0c61SJames Wright return 0; 95bb8a0c61SJames Wright } 96bb8a0c61SJames Wright 97bb8a0c61SJames Wright // ***************************************************************************** 98d1b9ef12SLeila Ghaffari // This QFunction set the inflow boundary condition for conservative variables 99d1b9ef12SLeila Ghaffari // ***************************************************************************** 1002b916ea7SJeremy L Thompson CEED_QFUNCTION(Channel_Inflow)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 101bb8a0c61SJames Wright // Inputs 102*3d65b166SJames Wright const CeedScalar(*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 103*3d65b166SJames Wright const CeedScalar(*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2]; 104*3d65b166SJames Wright const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 105bb8a0c61SJames Wright 106bb8a0c61SJames Wright // Outputs 107bb8a0c61SJames Wright CeedScalar(*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 108*3d65b166SJames Wright 109bb8a0c61SJames Wright const ChannelContext context = (ChannelContext)ctx; 110bb8a0c61SJames Wright const bool implicit = context->implicit; 111d1b9ef12SLeila Ghaffari NewtonianIdealGasContext gas = &context->newtonian_ctx; 112d1b9ef12SLeila Ghaffari const CeedScalar cv = gas->cv; 113*3d65b166SJames Wright const CeedScalar gamma = HeatCapacityRatio(&context->newtonian_ctx); 114bb8a0c61SJames Wright 115bb8a0c61SJames Wright // Quadrature Point Loop 116*3d65b166SJames Wright CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 117bb8a0c61SJames Wright // Setup 118bb8a0c61SJames Wright // -- Interp-to-Interp q_data 119bb8a0c61SJames Wright // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q). 120bb8a0c61SJames Wright // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q). 121bb8a0c61SJames Wright // We can effect this by swapping the sign on this weight 122bb8a0c61SJames Wright const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i]; 123bb8a0c61SJames Wright 124d1b9ef12SLeila Ghaffari // There is a gravity body force but it is excluded from 125d1b9ef12SLeila Ghaffari // the potential energy due to periodicity. 126d1b9ef12SLeila Ghaffari // g = (g, 0, 0) 127d1b9ef12SLeila Ghaffari // x = (0, x_2, x_3) 128d1b9ef12SLeila Ghaffari // e_potential = dot(g, x) = 0 129d1b9ef12SLeila Ghaffari const CeedScalar x[3] = {0, X[1][i], X[2][i]}; 130d1b9ef12SLeila Ghaffari 131bb8a0c61SJames Wright // Calcualte prescribed inflow values 132d1b9ef12SLeila Ghaffari State s_exact = Exact_Channel(3, 0., x, 5, ctx); 133bb8a0c61SJames Wright CeedScalar q_exact[5] = {0.}; 134d1b9ef12SLeila Ghaffari UnpackState_U(s_exact.U, q_exact); 135bb8a0c61SJames Wright 136bb8a0c61SJames Wright // Find pressure using state inside the domain 137d1b9ef12SLeila Ghaffari CeedScalar q_inside[5] = {0}; 1382b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 5; j++) q_inside[j] = q[j][i]; 139d1b9ef12SLeila Ghaffari State s_inside = StateFromU(gas, q_inside, x); 140d1b9ef12SLeila Ghaffari const CeedScalar P = s_inside.Y.pressure; 141bb8a0c61SJames Wright 142bb8a0c61SJames Wright // Find inflow state using calculated P and prescribed velocity, theta0 143d1b9ef12SLeila Ghaffari const CeedScalar e_internal = cv * s_exact.Y.temperature; 144bb8a0c61SJames Wright const CeedScalar rho_in = P / ((gamma - 1) * e_internal); 1452b916ea7SJeremy L Thompson const CeedScalar E_kinetic = .5 * rho_in * Dot3(s_exact.Y.velocity, s_exact.Y.velocity); 146bb8a0c61SJames Wright const CeedScalar E = rho_in * e_internal + E_kinetic; 147d1b9ef12SLeila Ghaffari 148bb8a0c61SJames Wright // ---- Normal vect 1492b916ea7SJeremy L Thompson const CeedScalar norm[3] = {q_data_sur[1][i], q_data_sur[2][i], q_data_sur[3][i]}; 150bb8a0c61SJames Wright // The Physics 151bb8a0c61SJames Wright // Zero v so all future terms can safely sum into it 152493642f1SJames Wright for (CeedInt j = 0; j < 5; j++) v[j][i] = 0.; 153bb8a0c61SJames Wright 154d1b9ef12SLeila Ghaffari const CeedScalar u_normal = Dot3(norm, s_exact.Y.velocity); 155bb8a0c61SJames Wright 156bb8a0c61SJames Wright // The Physics 157bb8a0c61SJames Wright // -- Density 158bb8a0c61SJames Wright v[0][i] -= wdetJb * rho_in * u_normal; 159bb8a0c61SJames Wright 160bb8a0c61SJames Wright // -- Momentum 1612b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 3; j++) v[j + 1][i] -= wdetJb * (rho_in * u_normal * s_exact.Y.velocity[j] + norm[j] * P); 162bb8a0c61SJames Wright 163bb8a0c61SJames Wright // -- Total Energy Density 164bb8a0c61SJames Wright v[4][i] -= wdetJb * u_normal * (E + P); 165bb8a0c61SJames Wright 166bb8a0c61SJames Wright } // End Quadrature Point Loop 167bb8a0c61SJames Wright return 0; 168bb8a0c61SJames Wright } 169bb8a0c61SJames Wright 170bb8a0c61SJames Wright // ***************************************************************************** 171d1b9ef12SLeila Ghaffari // This QFunction set the outflow boundary condition for conservative variables 172d1b9ef12SLeila Ghaffari // ***************************************************************************** 1732b916ea7SJeremy L Thompson CEED_QFUNCTION(Channel_Outflow)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 174bb8a0c61SJames Wright // Inputs 175*3d65b166SJames Wright const CeedScalar(*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 176*3d65b166SJames Wright const CeedScalar(*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2]; 177dd64951cSJames Wright 178bb8a0c61SJames Wright // Outputs 179bb8a0c61SJames Wright CeedScalar(*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 180bb8a0c61SJames Wright 181bb8a0c61SJames Wright const ChannelContext context = (ChannelContext)ctx; 182bb8a0c61SJames Wright const bool implicit = context->implicit; 183bb8a0c61SJames Wright const CeedScalar P0 = context->P0; 184bb8a0c61SJames Wright 185bb8a0c61SJames Wright // Quadrature Point Loop 186*3d65b166SJames Wright CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 187bb8a0c61SJames Wright // Setup 188bb8a0c61SJames Wright // -- Interp in 189bb8a0c61SJames Wright const CeedScalar rho = q[0][i]; 1902b916ea7SJeremy L Thompson const CeedScalar u[3] = {q[1][i] / rho, q[2][i] / rho, q[3][i] / rho}; 191bb8a0c61SJames Wright const CeedScalar E = q[4][i]; 192bb8a0c61SJames Wright 193bb8a0c61SJames Wright // -- Interp-to-Interp q_data 194bb8a0c61SJames Wright // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q). 195bb8a0c61SJames Wright // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q). 196bb8a0c61SJames Wright // We can effect this by swapping the sign on this weight 197bb8a0c61SJames Wright const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i]; 198bb8a0c61SJames Wright 199bb8a0c61SJames Wright // ---- Normal vect 2002b916ea7SJeremy L Thompson const CeedScalar norm[3] = {q_data_sur[1][i], q_data_sur[2][i], q_data_sur[3][i]}; 201bb8a0c61SJames Wright // The Physics 202bb8a0c61SJames Wright // Zero v so all future terms can safely sum into it 203493642f1SJames Wright for (CeedInt j = 0; j < 5; j++) v[j][i] = 0.; 204bb8a0c61SJames Wright 205bb8a0c61SJames Wright // Implementing outflow condition 206bb8a0c61SJames Wright const CeedScalar P = P0; // pressure 207704b8bbeSJames Wright const CeedScalar u_normal = Dot3(norm, u); // Normal velocity 208bb8a0c61SJames Wright // The Physics 209bb8a0c61SJames Wright // -- Density 210bb8a0c61SJames Wright v[0][i] -= wdetJb * rho * u_normal; 211bb8a0c61SJames Wright 212bb8a0c61SJames Wright // -- Momentum 2132b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 3; j++) v[j + 1][i] -= wdetJb * (rho * u_normal * u[j] + norm[j] * P); 214bb8a0c61SJames Wright 215bb8a0c61SJames Wright // -- Total Energy Density 216bb8a0c61SJames Wright v[4][i] -= wdetJb * u_normal * (E + P); 217bb8a0c61SJames Wright 218bb8a0c61SJames Wright } // End Quadrature Point Loop 219bb8a0c61SJames Wright return 0; 220bb8a0c61SJames Wright } 221cbe60e31SLeila Ghaffari 222cbe60e31SLeila Ghaffari // ***************************************************************************** 223bb8a0c61SJames Wright #endif // channel_h 224