188626eedSJames Wright // Copyright (c) 2017-2022, Lawrence Livermore National Security, LLC and other CEED contributors. 288626eedSJames Wright // All Rights Reserved. See the top-level LICENSE and NOTICE files for details. 388626eedSJames Wright // 488626eedSJames Wright // SPDX-License-Identifier: BSD-2-Clause 588626eedSJames Wright // 688626eedSJames Wright // This file is part of CEED: http://github.com/ceed 788626eedSJames Wright 888626eedSJames Wright /// @file 988626eedSJames Wright /// Operator for Navier-Stokes example using PETSc 1088626eedSJames Wright 1188626eedSJames Wright #ifndef blasius_h 1288626eedSJames Wright #define blasius_h 1388626eedSJames Wright 1488626eedSJames Wright #include <ceed.h> 152b730f8bSJeremy L Thompson 162518f336SLeila Ghaffari #include "newtonian_state.h" 17841e4c73SJed Brown #include "newtonian_types.h" 1813fa47b2SJames Wright #include "utils.h" 1988626eedSJames Wright 2007d14e58SLeila Ghaffari #define BLASIUS_MAX_N_CHEBYSHEV 50 2107d14e58SLeila Ghaffari 2288626eedSJames Wright typedef struct BlasiusContext_ *BlasiusContext; 2388626eedSJames Wright struct BlasiusContext_ { 2488626eedSJames Wright bool implicit; // !< Using implicit timesteping or not 25871db79fSKenneth E. Jansen bool weakT; // !< flag to set Temperature weakly at inflow 2688626eedSJames Wright CeedScalar delta0; // !< Boundary layer height at inflow 27fb455ff0SLeila Ghaffari CeedScalar U_inf; // !< Velocity at boundary layer edge 28fb455ff0SLeila Ghaffari CeedScalar T_inf; // !< Temperature at boundary layer edge 292518f336SLeila Ghaffari CeedScalar T_wall; // !< Temperature at the wall 3088626eedSJames Wright CeedScalar P0; // !< Pressure at outflow 31f1122ed0SJames Wright CeedScalar x_inflow; // !< Location of inflow in x 322518f336SLeila Ghaffari CeedScalar n_cheb; // !< Number of Chebyshev terms 3307d14e58SLeila Ghaffari CeedScalar *X; // !< Chebyshev polynomial coordinate vector (CPU only) 342518f336SLeila Ghaffari CeedScalar eta_max; // !< Maximum eta in the domain 3507d14e58SLeila Ghaffari CeedScalar Tf_cheb[BLASIUS_MAX_N_CHEBYSHEV]; // !< Chebyshev coefficient for f 3607d14e58SLeila Ghaffari CeedScalar Th_cheb[BLASIUS_MAX_N_CHEBYSHEV - 1]; // !< Chebyshev coefficient for h 3788626eedSJames Wright struct NewtonianIdealGasContext_ newtonian_ctx; 3888626eedSJames Wright }; 3988626eedSJames Wright 402518f336SLeila Ghaffari // ***************************************************************************** 41*ea61e9acSJeremy L Thompson // This helper function evaluates Chebyshev polynomials with a set of coefficients with all their derivatives represented as a recurrence table. 422518f336SLeila Ghaffari // ***************************************************************************** 432b730f8bSJeremy L Thompson CEED_QFUNCTION_HELPER void ChebyshevEval(int N, const double *Tf, double x, double eta_max, double *f) { 442518f336SLeila Ghaffari double dX_deta = 2 / eta_max; 452518f336SLeila Ghaffari double table[4][3] = { 462518f336SLeila Ghaffari // Chebyshev polynomials T_0, T_1, T_2 of the first kind in (-1,1) 472b730f8bSJeremy L Thompson {1, x, 2 * x * x - 1}, 482b730f8bSJeremy L Thompson {0, 1, 4 * x }, 492b730f8bSJeremy L Thompson {0, 0, 4 }, 502b730f8bSJeremy L Thompson {0, 0, 0 } 512518f336SLeila Ghaffari }; 522518f336SLeila Ghaffari for (int i = 0; i < 4; i++) { 532518f336SLeila Ghaffari // i-th derivative of f 542518f336SLeila Ghaffari f[i] = table[i][0] * Tf[0] + table[i][1] * Tf[1] + table[i][2] * Tf[2]; 552518f336SLeila Ghaffari } 562518f336SLeila Ghaffari for (int i = 3; i < N; i++) { 572518f336SLeila Ghaffari // T_n(x) = 2xT_{n-1}(x) - T_{n-2}(x) 582518f336SLeila Ghaffari table[0][i % 3] = 2 * x * table[0][(i - 1) % 3] - table[0][(i - 2) % 3]; 592518f336SLeila Ghaffari // Differentiate Chebyshev polynomials with the recurrence relation 602518f336SLeila Ghaffari for (int j = 1; j < 4; j++) { 612518f336SLeila Ghaffari // T'_{n}(x)/n = 2T_{n-1}(x) + T'_{n-2}(x)/n-2 622518f336SLeila Ghaffari table[j][i % 3] = i * (2 * table[j - 1][(i - 1) % 3] + table[j][(i - 2) % 3] / (i - 2)); 632518f336SLeila Ghaffari } 642518f336SLeila Ghaffari for (int j = 0; j < 4; j++) { 652518f336SLeila Ghaffari f[j] += table[j][i % 3] * Tf[i]; 6688626eedSJames Wright } 6788626eedSJames Wright } 682518f336SLeila Ghaffari for (int i = 1; i < 4; i++) { 692518f336SLeila Ghaffari // Transform derivatives from Chebyshev [-1, 1] to [0, eta_max]. 702518f336SLeila Ghaffari for (int j = 0; j < i; j++) f[i] *= dX_deta; 712518f336SLeila Ghaffari } 7288626eedSJames Wright } 7388626eedSJames Wright 742518f336SLeila Ghaffari // ***************************************************************************** 752518f336SLeila Ghaffari // This helper function computes the Blasius boundary layer solution. 762518f336SLeila Ghaffari // ***************************************************************************** 772b730f8bSJeremy L Thompson State CEED_QFUNCTION_HELPER(BlasiusSolution)(const BlasiusContext blasius, const CeedScalar x[3], const CeedScalar x0, const CeedScalar x_inflow, 7807d14e58SLeila Ghaffari const CeedScalar rho_infty, CeedScalar *t12) { 792518f336SLeila Ghaffari CeedInt N = blasius->n_cheb; 8007d14e58SLeila Ghaffari CeedScalar mu = blasius->newtonian_ctx.mu; 8107d14e58SLeila Ghaffari CeedScalar nu = mu / rho_infty; 82fb455ff0SLeila Ghaffari CeedScalar eta = x[1] * sqrt(blasius->U_inf / (nu * (x0 + x[0] - x_inflow))); 832518f336SLeila Ghaffari CeedScalar X = 2 * (eta / blasius->eta_max) - 1.; 84fb455ff0SLeila Ghaffari CeedScalar U_inf = blasius->U_inf; 852518f336SLeila Ghaffari CeedScalar Rd = GasConstant(&blasius->newtonian_ctx); 862518f336SLeila Ghaffari 872518f336SLeila Ghaffari CeedScalar f[4], h[4]; 882518f336SLeila Ghaffari ChebyshevEval(N, blasius->Tf_cheb, X, blasius->eta_max, f); 892518f336SLeila Ghaffari ChebyshevEval(N - 1, blasius->Th_cheb, X, blasius->eta_max, h); 902518f336SLeila Ghaffari 9107d14e58SLeila Ghaffari *t12 = mu * U_inf * f[2] * sqrt(U_inf / (nu * (x0 + x[0] - x_inflow))); 922518f336SLeila Ghaffari 932518f336SLeila Ghaffari CeedScalar Y[5]; 94fb455ff0SLeila Ghaffari Y[1] = U_inf * f[1]; 95fb455ff0SLeila Ghaffari Y[2] = 0.5 * sqrt(nu * U_inf / (x0 + x[0] - x_inflow)) * (eta * f[1] - f[0]); 962518f336SLeila Ghaffari Y[3] = 0.; 97fb455ff0SLeila Ghaffari Y[4] = blasius->T_inf * h[0]; 9807d14e58SLeila Ghaffari Y[0] = rho_infty / h[0] * Rd * Y[4]; 992518f336SLeila Ghaffari return StateFromY(&blasius->newtonian_ctx, Y, x); 10088626eedSJames Wright } 10188626eedSJames Wright 10288626eedSJames Wright // ***************************************************************************** 10388626eedSJames Wright // This QFunction sets a Blasius boundary layer for the initial condition 10488626eedSJames Wright // ***************************************************************************** 1052b730f8bSJeremy L Thompson CEED_QFUNCTION(ICsBlasius)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 10688626eedSJames Wright // Inputs 10788626eedSJames Wright const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 10888626eedSJames Wright 10988626eedSJames Wright // Outputs 11088626eedSJames Wright CeedScalar(*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 11188626eedSJames Wright 11288626eedSJames Wright const BlasiusContext context = (BlasiusContext)ctx; 11388626eedSJames Wright const CeedScalar cv = context->newtonian_ctx.cv; 11488626eedSJames Wright const CeedScalar mu = context->newtonian_ctx.mu; 115fb455ff0SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 11688626eedSJames Wright const CeedScalar P0 = context->P0; 11788626eedSJames Wright const CeedScalar delta0 = context->delta0; 118fb455ff0SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 119f1122ed0SJames Wright const CeedScalar x_inflow = context->x_inflow; 1202518f336SLeila Ghaffari const CeedScalar gamma = HeatCapacityRatio(&context->newtonian_ctx); 121fb455ff0SLeila Ghaffari const CeedScalar e_internal = cv * T_inf; 12288626eedSJames Wright const CeedScalar rho = P0 / ((gamma - 1) * e_internal); 123fb455ff0SLeila Ghaffari const CeedScalar x0 = U_inf * rho / (mu * 25 / (delta0 * delta0)); 1242518f336SLeila Ghaffari CeedScalar t12; 12588626eedSJames Wright 12688626eedSJames Wright // Quadrature Point Loop 1272b730f8bSJeremy L Thompson CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 1282518f336SLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], 0.}; 1292518f336SLeila Ghaffari State s = BlasiusSolution(context, x, x0, x_inflow, rho, &t12); 1302518f336SLeila Ghaffari CeedScalar q[5] = {0}; 1312518f336SLeila Ghaffari UnpackState_U(s.U, q); 1322518f336SLeila Ghaffari for (CeedInt j = 0; j < 5; j++) q0[j][i] = q[j]; 13388626eedSJames Wright 13488626eedSJames Wright } // End of Quadrature Point Loop 13588626eedSJames Wright return 0; 13688626eedSJames Wright } 13788626eedSJames Wright 13888626eedSJames Wright // ***************************************************************************** 1392b730f8bSJeremy L Thompson CEED_QFUNCTION(Blasius_Inflow)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 14088626eedSJames Wright // Inputs 14146603fc5SJames Wright const CeedScalar(*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 14246603fc5SJames Wright const CeedScalar(*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2]; 14346603fc5SJames Wright const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 14488626eedSJames Wright 14588626eedSJames Wright // Outputs 14688626eedSJames Wright CeedScalar(*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 14746603fc5SJames Wright 14888626eedSJames Wright const BlasiusContext context = (BlasiusContext)ctx; 14988626eedSJames Wright const bool implicit = context->implicit; 15007d14e58SLeila Ghaffari NewtonianIdealGasContext gas = &context->newtonian_ctx; 15188626eedSJames Wright const CeedScalar mu = context->newtonian_ctx.mu; 1522518f336SLeila Ghaffari const CeedScalar Rd = GasConstant(&context->newtonian_ctx); 153fb455ff0SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 15488626eedSJames Wright const CeedScalar P0 = context->P0; 15588626eedSJames Wright const CeedScalar delta0 = context->delta0; 156fb455ff0SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 157f1122ed0SJames Wright const CeedScalar x_inflow = context->x_inflow; 158871db79fSKenneth E. Jansen const bool weakT = context->weakT; 159fb455ff0SLeila Ghaffari const CeedScalar rho_0 = P0 / (Rd * T_inf); 160fb455ff0SLeila Ghaffari const CeedScalar x0 = U_inf * rho_0 / (mu * 25 / Square(delta0)); 16188626eedSJames Wright 16288626eedSJames Wright // Quadrature Point Loop 16346603fc5SJames Wright CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 16488626eedSJames Wright // Setup 16588626eedSJames Wright // -- Interp-to-Interp q_data 16688626eedSJames Wright // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q). 16788626eedSJames Wright // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q). 16888626eedSJames Wright // We can effect this by swapping the sign on this weight 16988626eedSJames Wright const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i]; 17088626eedSJames Wright 171871db79fSKenneth E. Jansen // Calculate inflow values 1722518f336SLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], 0.}; 17388626eedSJames Wright CeedScalar t12; 1742518f336SLeila Ghaffari State s = BlasiusSolution(context, x, x0, x_inflow, rho_0, &t12); 17507d14e58SLeila Ghaffari CeedScalar qi[5]; 17607d14e58SLeila Ghaffari for (CeedInt j = 0; j < 5; j++) qi[j] = q[j][i]; 17707d14e58SLeila Ghaffari State s_int = StateFromU(gas, qi, x); 17888626eedSJames Wright 179871db79fSKenneth E. Jansen // enabling user to choose between weak T and weak rho inflow 18007d14e58SLeila Ghaffari if (weakT) { // density from the current solution 18107d14e58SLeila Ghaffari s.U.density = s_int.U.density; 18207d14e58SLeila Ghaffari s.Y = StatePrimitiveFromConservative(gas, s.U, x); 18307d14e58SLeila Ghaffari } else { // Total energy from current solution 18407d14e58SLeila Ghaffari s.U.E_total = s_int.U.E_total; 18507d14e58SLeila Ghaffari s.Y = StatePrimitiveFromConservative(gas, s.U, x); 186871db79fSKenneth E. Jansen } 18707d14e58SLeila Ghaffari 18888626eedSJames Wright // ---- Normal vect 1892b730f8bSJeremy L Thompson const CeedScalar norm[3] = {q_data_sur[1][i], q_data_sur[2][i], q_data_sur[3][i]}; 19088626eedSJames Wright 19107d14e58SLeila Ghaffari StateConservative Flux_inviscid[3]; 19207d14e58SLeila Ghaffari FluxInviscid(&context->newtonian_ctx, s, Flux_inviscid); 19388626eedSJames Wright 1942b730f8bSJeremy L Thompson const CeedScalar stress[3][3] = { 1952b730f8bSJeremy L Thompson {0, t12, 0}, 1962b730f8bSJeremy L Thompson {t12, 0, 0}, 1972b730f8bSJeremy L Thompson {0, 0, 0} 1982b730f8bSJeremy L Thompson }; 19907d14e58SLeila Ghaffari const CeedScalar Fe[3] = {0}; // TODO: viscous energy flux needs grad temperature 20007d14e58SLeila Ghaffari CeedScalar Flux[5]; 20107d14e58SLeila Ghaffari FluxTotal_Boundary(Flux_inviscid, stress, Fe, norm, Flux); 2022b730f8bSJeremy L Thompson for (CeedInt j = 0; j < 5; j++) v[j][i] = -wdetJb * Flux[j]; 20388626eedSJames Wright } // End Quadrature Point Loop 20488626eedSJames Wright return 0; 20588626eedSJames Wright } 20688626eedSJames Wright 2072518f336SLeila Ghaffari // ***************************************************************************** 2082b730f8bSJeremy L Thompson CEED_QFUNCTION(Blasius_Inflow_Jacobian)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 209e334ad8fSJed Brown // Inputs 21046603fc5SJames Wright const CeedScalar(*dq)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 21146603fc5SJames Wright const CeedScalar(*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2]; 21246603fc5SJames Wright const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 213e334ad8fSJed Brown 214e334ad8fSJed Brown // Outputs 215e334ad8fSJed Brown CeedScalar(*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 21646603fc5SJames Wright 217e334ad8fSJed Brown const BlasiusContext context = (BlasiusContext)ctx; 218e334ad8fSJed Brown const bool implicit = context->implicit; 219e334ad8fSJed Brown const CeedScalar mu = context->newtonian_ctx.mu; 220e334ad8fSJed Brown const CeedScalar cv = context->newtonian_ctx.cv; 2212518f336SLeila Ghaffari const CeedScalar Rd = GasConstant(&context->newtonian_ctx); 2222518f336SLeila Ghaffari const CeedScalar gamma = HeatCapacityRatio(&context->newtonian_ctx); 223fb455ff0SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 224e334ad8fSJed Brown const CeedScalar P0 = context->P0; 225e334ad8fSJed Brown const CeedScalar delta0 = context->delta0; 226fb455ff0SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 227e334ad8fSJed Brown const bool weakT = context->weakT; 228fb455ff0SLeila Ghaffari const CeedScalar rho_0 = P0 / (Rd * T_inf); 229fb455ff0SLeila Ghaffari const CeedScalar x0 = U_inf * rho_0 / (mu * 25 / (delta0 * delta0)); 230e334ad8fSJed Brown 231e334ad8fSJed Brown // Quadrature Point Loop 23246603fc5SJames Wright CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 233e334ad8fSJed Brown // Setup 234e334ad8fSJed Brown // -- Interp-to-Interp q_data 235e334ad8fSJed Brown // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q). 236e334ad8fSJed Brown // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q). 237e334ad8fSJed Brown // We can effect this by swapping the sign on this weight 238e334ad8fSJed Brown const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i]; 239e334ad8fSJed Brown 240e334ad8fSJed Brown // Calculate inflow values 24107d14e58SLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], X[2][i]}; 242e334ad8fSJed Brown CeedScalar t12; 2432518f336SLeila Ghaffari State s = BlasiusSolution(context, x, x0, 0, rho_0, &t12); 244e334ad8fSJed Brown 245e334ad8fSJed Brown // enabling user to choose between weak T and weak rho inflow 246e334ad8fSJed Brown CeedScalar drho, dE, dP; 247e334ad8fSJed Brown if (weakT) { 248e334ad8fSJed Brown // rho should be from the current solution 249e334ad8fSJed Brown drho = dq[0][i]; 250fb455ff0SLeila Ghaffari CeedScalar dE_internal = drho * cv * T_inf; 2512518f336SLeila Ghaffari CeedScalar dE_kinetic = .5 * drho * Dot3(s.Y.velocity, s.Y.velocity); 252e334ad8fSJed Brown dE = dE_internal + dE_kinetic; 253fb455ff0SLeila Ghaffari dP = drho * Rd * T_inf; // interior rho with exterior T 254e334ad8fSJed Brown } else { // rho specified, E_internal from solution 255e334ad8fSJed Brown drho = 0; 256e334ad8fSJed Brown dE = dq[4][i]; 257e334ad8fSJed Brown dP = dE * (gamma - 1.); 258e334ad8fSJed Brown } 2592b730f8bSJeremy L Thompson const CeedScalar norm[3] = {q_data_sur[1][i], q_data_sur[2][i], q_data_sur[3][i]}; 260e334ad8fSJed Brown 2612518f336SLeila Ghaffari const CeedScalar u_normal = Dot3(norm, s.Y.velocity); 262e334ad8fSJed Brown 263e334ad8fSJed Brown v[0][i] = -wdetJb * drho * u_normal; 2642b730f8bSJeremy L Thompson for (int j = 0; j < 3; j++) { 2652518f336SLeila Ghaffari v[j + 1][i] = -wdetJb * (drho * u_normal * s.Y.velocity[j] + norm[j] * dP); 2662b730f8bSJeremy L Thompson } 267e334ad8fSJed Brown v[4][i] = -wdetJb * u_normal * (dE + dP); 268e334ad8fSJed Brown } // End Quadrature Point Loop 269e334ad8fSJed Brown return 0; 270e334ad8fSJed Brown } 271e334ad8fSJed Brown 27288626eedSJames Wright #endif // blasius_h 273