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 1288626eedSJames Wright #ifndef blasius_h 1388626eedSJames Wright #define blasius_h 1488626eedSJames Wright 1588626eedSJames Wright #include <ceed.h> 162518f336SLeila Ghaffari #include "newtonian_state.h" 17841e4c73SJed Brown #include "newtonian_types.h" 1813fa47b2SJames Wright #include "utils.h" 1988626eedSJames Wright 2088626eedSJames Wright typedef struct BlasiusContext_ *BlasiusContext; 2188626eedSJames Wright struct BlasiusContext_ { 2288626eedSJames Wright bool implicit; // !< Using implicit timesteping or not 23871db79fSKenneth E. Jansen bool weakT; // !< flag to set Temperature weakly at inflow 2488626eedSJames Wright CeedScalar delta0; // !< Boundary layer height at inflow 25*fb455ff0SLeila Ghaffari CeedScalar U_inf; // !< Velocity at boundary layer edge 26*fb455ff0SLeila Ghaffari CeedScalar T_inf; // !< Temperature at boundary layer edge 272518f336SLeila Ghaffari CeedScalar T_wall; // !< Temperature at the wall 2888626eedSJames Wright CeedScalar P0; // !< Pressure at outflow 29f1122ed0SJames Wright CeedScalar x_inflow; // !< Location of inflow in x 302518f336SLeila Ghaffari CeedScalar n_cheb; // !< Number of Chebyshev terms 312518f336SLeila Ghaffari CeedScalar *X; // !< Chebyshev polynomial coordinate vector 322518f336SLeila Ghaffari CeedScalar eta_max; // !< Maximum eta in the domain 332518f336SLeila Ghaffari CeedScalar *Tf_cheb; // !< Chebyshev coefficient for f 342518f336SLeila Ghaffari CeedScalar *Th_cheb; // !< Chebyshev coefficient for h 3588626eedSJames Wright struct NewtonianIdealGasContext_ newtonian_ctx; 3688626eedSJames Wright }; 3788626eedSJames Wright 382518f336SLeila Ghaffari // ***************************************************************************** 392518f336SLeila Ghaffari // This helper function evaluates Chebyshev polynomials with a set of 402518f336SLeila Ghaffari // coefficients with all their derivatives represented as a recurrence table. 412518f336SLeila Ghaffari // ***************************************************************************** 422518f336SLeila Ghaffari CEED_QFUNCTION_HELPER void ChebyshevEval(int N, const double *Tf, double x, 432518f336SLeila Ghaffari 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) 472518f336SLeila Ghaffari {1, x, 2*x *x - 1}, {0, 1, 4*x}, {0, 0, 4}, {0, 0, 0} 482518f336SLeila Ghaffari }; 492518f336SLeila Ghaffari for (int i=0; i<4; i++) { 502518f336SLeila Ghaffari // i-th derivative of f 512518f336SLeila Ghaffari f[i] = table[i][0] * Tf[0] + table[i][1] * Tf[1] + table[i][2] * Tf[2]; 522518f336SLeila Ghaffari } 532518f336SLeila Ghaffari for (int i=3; i<N; i++) { 542518f336SLeila Ghaffari // T_n(x) = 2xT_{n-1}(x) - T_{n-2}(x) 552518f336SLeila Ghaffari table[0][i%3] = 2 * x * table[0][(i-1) % 3] - table[0][(i-2)%3]; 562518f336SLeila Ghaffari // Differentiate Chebyshev polynomials with the recurrence relation 572518f336SLeila Ghaffari for (int j=1; j<4; j++) { 582518f336SLeila Ghaffari // T'_{n}(x)/n = 2T_{n-1}(x) + T'_{n-2}(x)/n-2 592518f336SLeila Ghaffari table[j][i%3] = i * (2 * table[j-1][(i-1) % 3] + table[j][(i-2)%3] / (i-2)); 602518f336SLeila Ghaffari } 612518f336SLeila Ghaffari for (int j=0; j<4; j++) { 622518f336SLeila Ghaffari f[j] += table[j][i%3] * Tf[i]; 6388626eedSJames Wright } 6488626eedSJames Wright } 652518f336SLeila Ghaffari for (int i=1; i<4; i++) { 662518f336SLeila Ghaffari // Transform derivatives from Chebyshev [-1, 1] to [0, eta_max]. 672518f336SLeila Ghaffari for (int j=0; j<i; j++) f[i] *= dX_deta; 682518f336SLeila Ghaffari } 6988626eedSJames Wright } 7088626eedSJames Wright 712518f336SLeila Ghaffari // ***************************************************************************** 722518f336SLeila Ghaffari // This helper function computes the Blasius boundary layer solution. 732518f336SLeila Ghaffari // ***************************************************************************** 742518f336SLeila Ghaffari State CEED_QFUNCTION_HELPER(BlasiusSolution)(const BlasiusContext blasius, 752518f336SLeila Ghaffari const CeedScalar x[3], const CeedScalar x0, const CeedScalar x_inflow, 762518f336SLeila Ghaffari const CeedScalar rho, CeedScalar *t12) { 772518f336SLeila Ghaffari CeedInt N = blasius->n_cheb; 782518f336SLeila Ghaffari CeedScalar nu = blasius->newtonian_ctx.mu / rho; 79*fb455ff0SLeila Ghaffari CeedScalar eta = x[1]*sqrt(blasius->U_inf/(nu*(x0+x[0]-x_inflow))); 802518f336SLeila Ghaffari CeedScalar X = 2 * (eta / blasius->eta_max) - 1.; 81*fb455ff0SLeila Ghaffari CeedScalar U_inf = blasius->U_inf; 822518f336SLeila Ghaffari CeedScalar Rd = GasConstant(&blasius->newtonian_ctx); 832518f336SLeila Ghaffari 842518f336SLeila Ghaffari CeedScalar f[4], h[4]; 852518f336SLeila Ghaffari ChebyshevEval(N, blasius->Tf_cheb, X, blasius->eta_max, f); 862518f336SLeila Ghaffari ChebyshevEval(N-1, blasius->Th_cheb, X, blasius->eta_max, h); 872518f336SLeila Ghaffari 88*fb455ff0SLeila Ghaffari *t12 = rho*nu*U_inf*f[2]*sqrt(U_inf/(nu*(x0+x[0]-x_inflow))); 892518f336SLeila Ghaffari 902518f336SLeila Ghaffari CeedScalar Y[5]; 91*fb455ff0SLeila Ghaffari Y[1] = U_inf * f[1]; 92*fb455ff0SLeila Ghaffari Y[2] = 0.5*sqrt(nu*U_inf/(x0+x[0]-x_inflow))*(eta*f[1] - f[0]); 932518f336SLeila Ghaffari Y[3] = 0.; 94*fb455ff0SLeila Ghaffari Y[4] = blasius->T_inf * h[0]; 952518f336SLeila Ghaffari Y[0] = rho * Rd * Y[4]; 962518f336SLeila Ghaffari return StateFromY(&blasius->newtonian_ctx, Y, x); 9788626eedSJames Wright } 9888626eedSJames Wright 9988626eedSJames Wright // ***************************************************************************** 10088626eedSJames Wright // This QFunction sets a Blasius boundary layer for the initial condition 10188626eedSJames Wright // ***************************************************************************** 10288626eedSJames Wright CEED_QFUNCTION(ICsBlasius)(void *ctx, CeedInt Q, 10388626eedSJames Wright const CeedScalar *const *in, CeedScalar *const *out) { 10488626eedSJames Wright // Inputs 10588626eedSJames Wright const CeedScalar (*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 10688626eedSJames Wright 10788626eedSJames Wright // Outputs 10888626eedSJames Wright CeedScalar (*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 10988626eedSJames Wright 11088626eedSJames Wright const BlasiusContext context = (BlasiusContext)ctx; 11188626eedSJames Wright const CeedScalar cv = context->newtonian_ctx.cv; 11288626eedSJames Wright const CeedScalar mu = context->newtonian_ctx.mu; 113*fb455ff0SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 11488626eedSJames Wright const CeedScalar P0 = context->P0; 11588626eedSJames Wright const CeedScalar delta0 = context->delta0; 116*fb455ff0SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 117f1122ed0SJames Wright const CeedScalar x_inflow = context->x_inflow; 1182518f336SLeila Ghaffari const CeedScalar gamma = HeatCapacityRatio(&context->newtonian_ctx); 119*fb455ff0SLeila Ghaffari const CeedScalar e_internal = cv * T_inf; 12088626eedSJames Wright const CeedScalar rho = P0 / ((gamma - 1) * e_internal); 121*fb455ff0SLeila Ghaffari const CeedScalar x0 = U_inf*rho / (mu*25/(delta0*delta0)); 1222518f336SLeila Ghaffari CeedScalar t12; 12388626eedSJames Wright 12488626eedSJames Wright // Quadrature Point Loop 12588626eedSJames Wright CeedPragmaSIMD 12688626eedSJames Wright for (CeedInt i=0; i<Q; i++) { 1272518f336SLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], 0.}; 1282518f336SLeila Ghaffari State s = BlasiusSolution(context, x, x0, x_inflow, rho, &t12); 1292518f336SLeila Ghaffari CeedScalar q[5] = {0}; 1302518f336SLeila Ghaffari UnpackState_U(s.U, q); 1312518f336SLeila Ghaffari for (CeedInt j=0; j<5; j++) q0[j][i] = q[j]; 13288626eedSJames Wright 13388626eedSJames Wright } // End of Quadrature Point Loop 13488626eedSJames Wright return 0; 13588626eedSJames Wright } 13688626eedSJames Wright 13788626eedSJames Wright // ***************************************************************************** 13888626eedSJames Wright CEED_QFUNCTION(Blasius_Inflow)(void *ctx, CeedInt Q, 13988626eedSJames Wright const CeedScalar *const *in, 14088626eedSJames Wright CeedScalar *const *out) { 14188626eedSJames Wright // *INDENT-OFF* 14288626eedSJames Wright // Inputs 14388626eedSJames Wright const CeedScalar (*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 144e8b03feeSJames Wright (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 145e8b03feeSJames Wright (*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 14688626eedSJames Wright 14788626eedSJames Wright // Outputs 14888626eedSJames Wright CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 14988626eedSJames Wright // *INDENT-ON* 15088626eedSJames Wright const BlasiusContext context = (BlasiusContext)ctx; 15188626eedSJames Wright const bool implicit = context->implicit; 15288626eedSJames Wright const CeedScalar mu = context->newtonian_ctx.mu; 15388626eedSJames Wright const CeedScalar cv = context->newtonian_ctx.cv; 1542518f336SLeila Ghaffari const CeedScalar Rd = GasConstant(&context->newtonian_ctx); 1552518f336SLeila Ghaffari const CeedScalar gamma = HeatCapacityRatio(&context->newtonian_ctx); 156*fb455ff0SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 15788626eedSJames Wright const CeedScalar P0 = context->P0; 15888626eedSJames Wright const CeedScalar delta0 = context->delta0; 159*fb455ff0SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 160f1122ed0SJames Wright const CeedScalar x_inflow = context->x_inflow; 161871db79fSKenneth E. Jansen const bool weakT = context->weakT; 162*fb455ff0SLeila Ghaffari const CeedScalar rho_0 = P0 / (Rd * T_inf); 163*fb455ff0SLeila Ghaffari const CeedScalar x0 = U_inf*rho_0 / (mu*25/ Square(delta0)); 16488626eedSJames Wright 16588626eedSJames Wright CeedPragmaSIMD 16688626eedSJames Wright // Quadrature Point Loop 16788626eedSJames Wright for (CeedInt i=0; i<Q; i++) { 16888626eedSJames Wright // Setup 16988626eedSJames Wright // -- Interp-to-Interp q_data 17088626eedSJames Wright // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q). 17188626eedSJames Wright // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q). 17288626eedSJames Wright // We can effect this by swapping the sign on this weight 17388626eedSJames Wright const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i]; 17488626eedSJames Wright 175871db79fSKenneth E. Jansen // Calculate inflow values 1762518f336SLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], 0.}; 17788626eedSJames Wright CeedScalar t12; 1782518f336SLeila Ghaffari State s = BlasiusSolution(context, x, x0, x_inflow, rho_0, &t12); 17988626eedSJames Wright 180871db79fSKenneth E. Jansen // enabling user to choose between weak T and weak rho inflow 181871db79fSKenneth E. Jansen CeedScalar rho,E_internal, P, E_kinetic; 182871db79fSKenneth E. Jansen if (weakT) { 183871db79fSKenneth E. Jansen // rho should be from the current solution 184871db79fSKenneth E. Jansen rho = q[0][i]; 185*fb455ff0SLeila Ghaffari // Temperature is being set weakly (T_inf) and for constant cv this sets E_internal 186*fb455ff0SLeila Ghaffari E_internal = rho * cv * T_inf; 187871db79fSKenneth E. Jansen // Find pressure using 188*fb455ff0SLeila Ghaffari P = rho*Rd*T_inf; // interior rho with exterior T 1892518f336SLeila Ghaffari E_kinetic = .5 * rho * Dot3(s.Y.velocity, s.Y.velocity); 190871db79fSKenneth E. Jansen } else { 191*fb455ff0SLeila Ghaffari // Fixing rho weakly on the inflow to a value consistent with T_inf and P0 192871db79fSKenneth E. Jansen rho = rho_0; 1932518f336SLeila Ghaffari E_kinetic = .5 * rho * Dot3(s.Y.velocity, s.Y.velocity); 194871db79fSKenneth E. Jansen E_internal = q[4][i] - E_kinetic; // uses set rho and u but E from solution 195871db79fSKenneth E. Jansen P = E_internal * (gamma - 1.); 196871db79fSKenneth E. Jansen } 197871db79fSKenneth E. Jansen const CeedScalar E = E_internal + E_kinetic; 19888626eedSJames Wright // ---- Normal vect 19988626eedSJames Wright const CeedScalar norm[3] = {q_data_sur[1][i], 20088626eedSJames Wright q_data_sur[2][i], 20188626eedSJames Wright q_data_sur[3][i] 20288626eedSJames Wright }; 20388626eedSJames Wright 20488626eedSJames Wright // The Physics 20588626eedSJames Wright // Zero v so all future terms can safely sum into it 206ba6664aeSJames Wright for (CeedInt j=0; j<5; j++) v[j][i] = 0.; 20788626eedSJames Wright 2082518f336SLeila Ghaffari const CeedScalar u_normal = Dot3(norm, s.Y.velocity); 20930ccfdeaSJed Brown const CeedScalar viscous_flux[3] = {-t12 *norm[1], -t12 *norm[0], 0}; 21088626eedSJames Wright 21188626eedSJames Wright // The Physics 21288626eedSJames Wright // -- Density 21388626eedSJames Wright v[0][i] -= wdetJb * rho * u_normal; // interior rho 21488626eedSJames Wright 21588626eedSJames Wright // -- Momentum 216ba6664aeSJames Wright for (CeedInt j=0; j<3; j++) 2172518f336SLeila Ghaffari v[j+1][i] -= wdetJb * (rho * u_normal * s.Y.velocity[j] // interior rho 21830ccfdeaSJed Brown + norm[j] * P // mixed P 21930ccfdeaSJed Brown + viscous_flux[j]); 22088626eedSJames Wright 22188626eedSJames Wright // -- Total Energy Density 2222518f336SLeila Ghaffari v[4][i] -= wdetJb * (u_normal * (E + P) + Dot3(viscous_flux, s.Y.velocity)); 22388626eedSJames Wright 22488626eedSJames Wright } // End Quadrature Point Loop 22588626eedSJames Wright return 0; 22688626eedSJames Wright } 22788626eedSJames Wright 2282518f336SLeila Ghaffari // ***************************************************************************** 229e334ad8fSJed Brown CEED_QFUNCTION(Blasius_Inflow_Jacobian)(void *ctx, CeedInt Q, 230e334ad8fSJed Brown const CeedScalar *const *in, 231e334ad8fSJed Brown CeedScalar *const *out) { 232e334ad8fSJed Brown // *INDENT-OFF* 233e334ad8fSJed Brown // Inputs 234e334ad8fSJed Brown const CeedScalar (*dq)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 235b55ac660SJames Wright (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 236b55ac660SJames Wright (*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 237e334ad8fSJed Brown 238e334ad8fSJed Brown // Outputs 239e334ad8fSJed Brown CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 240e334ad8fSJed Brown // *INDENT-ON* 241e334ad8fSJed Brown const BlasiusContext context = (BlasiusContext)ctx; 242e334ad8fSJed Brown const bool implicit = context->implicit; 243e334ad8fSJed Brown const CeedScalar mu = context->newtonian_ctx.mu; 244e334ad8fSJed Brown const CeedScalar cv = context->newtonian_ctx.cv; 2452518f336SLeila Ghaffari const CeedScalar Rd = GasConstant(&context->newtonian_ctx); 2462518f336SLeila Ghaffari const CeedScalar gamma = HeatCapacityRatio(&context->newtonian_ctx); 247*fb455ff0SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 248e334ad8fSJed Brown const CeedScalar P0 = context->P0; 249e334ad8fSJed Brown const CeedScalar delta0 = context->delta0; 250*fb455ff0SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 251e334ad8fSJed Brown const bool weakT = context->weakT; 252*fb455ff0SLeila Ghaffari const CeedScalar rho_0 = P0 / (Rd * T_inf); 253*fb455ff0SLeila Ghaffari const CeedScalar x0 = U_inf*rho_0 / (mu*25/ (delta0*delta0)); 254e334ad8fSJed Brown 255e334ad8fSJed Brown CeedPragmaSIMD 256e334ad8fSJed Brown // Quadrature Point Loop 257e334ad8fSJed Brown for (CeedInt i=0; i<Q; i++) { 258e334ad8fSJed Brown // Setup 259e334ad8fSJed Brown // -- Interp-to-Interp q_data 260e334ad8fSJed Brown // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q). 261e334ad8fSJed Brown // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q). 262e334ad8fSJed Brown // We can effect this by swapping the sign on this weight 263e334ad8fSJed Brown const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i]; 264e334ad8fSJed Brown 265e334ad8fSJed Brown // Calculate inflow values 2662518f336SLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], 0.}; 267e334ad8fSJed Brown CeedScalar t12; 2682518f336SLeila Ghaffari State s = BlasiusSolution(context, x, x0, 0, rho_0, &t12); 269e334ad8fSJed Brown 270e334ad8fSJed Brown // enabling user to choose between weak T and weak rho inflow 271e334ad8fSJed Brown CeedScalar drho, dE, dP; 272e334ad8fSJed Brown if (weakT) { 273e334ad8fSJed Brown // rho should be from the current solution 274e334ad8fSJed Brown drho = dq[0][i]; 275*fb455ff0SLeila Ghaffari CeedScalar dE_internal = drho * cv * T_inf; 2762518f336SLeila Ghaffari CeedScalar dE_kinetic = .5 * drho * Dot3(s.Y.velocity, s.Y.velocity); 277e334ad8fSJed Brown dE = dE_internal + dE_kinetic; 278*fb455ff0SLeila Ghaffari dP = drho * Rd * T_inf; // interior rho with exterior T 279e334ad8fSJed Brown } else { // rho specified, E_internal from solution 280e334ad8fSJed Brown drho = 0; 281e334ad8fSJed Brown dE = dq[4][i]; 282e334ad8fSJed Brown dP = dE * (gamma - 1.); 283e334ad8fSJed Brown } 284e334ad8fSJed Brown const CeedScalar norm[3] = {q_data_sur[1][i], 285e334ad8fSJed Brown q_data_sur[2][i], 286e334ad8fSJed Brown q_data_sur[3][i] 287e334ad8fSJed Brown }; 288e334ad8fSJed Brown 2892518f336SLeila Ghaffari const CeedScalar u_normal = Dot3(norm, s.Y.velocity); 290e334ad8fSJed Brown 291e334ad8fSJed Brown v[0][i] = - wdetJb * drho * u_normal; 292e334ad8fSJed Brown for (int j=0; j<3; j++) 2932518f336SLeila Ghaffari v[j+1][i] = -wdetJb * (drho * u_normal * s.Y.velocity[j] + norm[j] * dP); 294e334ad8fSJed Brown v[4][i] = - wdetJb * u_normal * (dE + dP); 295e334ad8fSJed Brown } // End Quadrature Point Loop 296e334ad8fSJed Brown return 0; 297e334ad8fSJed Brown } 298e334ad8fSJed Brown 29988626eedSJames Wright #endif // blasius_h 300