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 blasius_h 12bb8a0c61SJames Wright #define blasius_h 13bb8a0c61SJames Wright 14bb8a0c61SJames Wright #include <ceed.h> 152b916ea7SJeremy L Thompson 16e0d1a4dfSLeila Ghaffari #include "newtonian_state.h" 1715a3537eSJed Brown #include "newtonian_types.h" 18704b8bbeSJames Wright #include "utils.h" 19bb8a0c61SJames Wright 200d850f2eSLeila Ghaffari #define BLASIUS_MAX_N_CHEBYSHEV 50 210d850f2eSLeila Ghaffari 22bb8a0c61SJames Wright typedef struct BlasiusContext_ *BlasiusContext; 23bb8a0c61SJames Wright struct BlasiusContext_ { 24bb8a0c61SJames Wright bool implicit; // !< Using implicit timesteping or not 252acc7cbcSKenneth E. Jansen bool weakT; // !< flag to set Temperature weakly at inflow 26bb8a0c61SJames Wright CeedScalar delta0; // !< Boundary layer height at inflow 27aef1eb53SLeila Ghaffari CeedScalar U_inf; // !< Velocity at boundary layer edge 28aef1eb53SLeila Ghaffari CeedScalar T_inf; // !< Temperature at boundary layer edge 29e0d1a4dfSLeila Ghaffari CeedScalar T_wall; // !< Temperature at the wall 30bb8a0c61SJames Wright CeedScalar P0; // !< Pressure at outflow 31ef2c71fdSJames Wright CeedScalar x_inflow; // !< Location of inflow in x 32e0d1a4dfSLeila Ghaffari CeedScalar n_cheb; // !< Number of Chebyshev terms 330d850f2eSLeila Ghaffari CeedScalar *X; // !< Chebyshev polynomial coordinate vector (CPU only) 34e0d1a4dfSLeila Ghaffari CeedScalar eta_max; // !< Maximum eta in the domain 350d850f2eSLeila Ghaffari CeedScalar Tf_cheb[BLASIUS_MAX_N_CHEBYSHEV]; // !< Chebyshev coefficient for f 360d850f2eSLeila Ghaffari CeedScalar Th_cheb[BLASIUS_MAX_N_CHEBYSHEV - 1]; // !< Chebyshev coefficient for h 37bb8a0c61SJames Wright struct NewtonianIdealGasContext_ newtonian_ctx; 38bb8a0c61SJames Wright }; 39bb8a0c61SJames Wright 40e0d1a4dfSLeila Ghaffari // ***************************************************************************** 4104e40bb6SJeremy L Thompson // This helper function evaluates Chebyshev polynomials with a set of coefficients with all their derivatives represented as a recurrence table. 42e0d1a4dfSLeila Ghaffari // ***************************************************************************** 432b916ea7SJeremy L Thompson CEED_QFUNCTION_HELPER void ChebyshevEval(int N, const double *Tf, double x, double eta_max, double *f) { 44e0d1a4dfSLeila Ghaffari double dX_deta = 2 / eta_max; 45e0d1a4dfSLeila Ghaffari double table[4][3] = { 46e0d1a4dfSLeila Ghaffari // Chebyshev polynomials T_0, T_1, T_2 of the first kind in (-1,1) 472b916ea7SJeremy L Thompson {1, x, 2 * x * x - 1}, 482b916ea7SJeremy L Thompson {0, 1, 4 * x }, 492b916ea7SJeremy L Thompson {0, 0, 4 }, 502b916ea7SJeremy L Thompson {0, 0, 0 } 51e0d1a4dfSLeila Ghaffari }; 52e0d1a4dfSLeila Ghaffari for (int i = 0; i < 4; i++) { 53e0d1a4dfSLeila Ghaffari // i-th derivative of f 54e0d1a4dfSLeila Ghaffari f[i] = table[i][0] * Tf[0] + table[i][1] * Tf[1] + table[i][2] * Tf[2]; 55e0d1a4dfSLeila Ghaffari } 56e0d1a4dfSLeila Ghaffari for (int i = 3; i < N; i++) { 57e0d1a4dfSLeila Ghaffari // T_n(x) = 2xT_{n-1}(x) - T_{n-2}(x) 58e0d1a4dfSLeila Ghaffari table[0][i % 3] = 2 * x * table[0][(i - 1) % 3] - table[0][(i - 2) % 3]; 59e0d1a4dfSLeila Ghaffari // Differentiate Chebyshev polynomials with the recurrence relation 60e0d1a4dfSLeila Ghaffari for (int j = 1; j < 4; j++) { 61e0d1a4dfSLeila Ghaffari // T'_{n}(x)/n = 2T_{n-1}(x) + T'_{n-2}(x)/n-2 62e0d1a4dfSLeila Ghaffari table[j][i % 3] = i * (2 * table[j - 1][(i - 1) % 3] + table[j][(i - 2) % 3] / (i - 2)); 63e0d1a4dfSLeila Ghaffari } 64e0d1a4dfSLeila Ghaffari for (int j = 0; j < 4; j++) { 65e0d1a4dfSLeila Ghaffari f[j] += table[j][i % 3] * Tf[i]; 66bb8a0c61SJames Wright } 67bb8a0c61SJames Wright } 68e0d1a4dfSLeila Ghaffari for (int i = 1; i < 4; i++) { 69e0d1a4dfSLeila Ghaffari // Transform derivatives from Chebyshev [-1, 1] to [0, eta_max]. 70e0d1a4dfSLeila Ghaffari for (int j = 0; j < i; j++) f[i] *= dX_deta; 71e0d1a4dfSLeila Ghaffari } 72bb8a0c61SJames Wright } 73bb8a0c61SJames Wright 74e0d1a4dfSLeila Ghaffari // ***************************************************************************** 75e0d1a4dfSLeila Ghaffari // This helper function computes the Blasius boundary layer solution. 76e0d1a4dfSLeila Ghaffari // ***************************************************************************** 772b916ea7SJeremy L Thompson State CEED_QFUNCTION_HELPER(BlasiusSolution)(const BlasiusContext blasius, const CeedScalar x[3], const CeedScalar x0, const CeedScalar x_inflow, 780d850f2eSLeila Ghaffari const CeedScalar rho_infty, CeedScalar *t12) { 79e0d1a4dfSLeila Ghaffari CeedInt N = blasius->n_cheb; 800d850f2eSLeila Ghaffari CeedScalar mu = blasius->newtonian_ctx.mu; 810d850f2eSLeila Ghaffari CeedScalar nu = mu / rho_infty; 82aef1eb53SLeila Ghaffari CeedScalar eta = x[1] * sqrt(blasius->U_inf / (nu * (x0 + x[0] - x_inflow))); 83e0d1a4dfSLeila Ghaffari CeedScalar X = 2 * (eta / blasius->eta_max) - 1.; 84aef1eb53SLeila Ghaffari CeedScalar U_inf = blasius->U_inf; 85e0d1a4dfSLeila Ghaffari CeedScalar Rd = GasConstant(&blasius->newtonian_ctx); 86e0d1a4dfSLeila Ghaffari 87e0d1a4dfSLeila Ghaffari CeedScalar f[4], h[4]; 88e0d1a4dfSLeila Ghaffari ChebyshevEval(N, blasius->Tf_cheb, X, blasius->eta_max, f); 89e0d1a4dfSLeila Ghaffari ChebyshevEval(N - 1, blasius->Th_cheb, X, blasius->eta_max, h); 90e0d1a4dfSLeila Ghaffari 910d850f2eSLeila Ghaffari *t12 = mu * U_inf * f[2] * sqrt(U_inf / (nu * (x0 + x[0] - x_inflow))); 92e0d1a4dfSLeila Ghaffari 93e0d1a4dfSLeila Ghaffari CeedScalar Y[5]; 94aef1eb53SLeila Ghaffari Y[1] = U_inf * f[1]; 95aef1eb53SLeila Ghaffari Y[2] = 0.5 * sqrt(nu * U_inf / (x0 + x[0] - x_inflow)) * (eta * f[1] - f[0]); 96e0d1a4dfSLeila Ghaffari Y[3] = 0.; 97aef1eb53SLeila Ghaffari Y[4] = blasius->T_inf * h[0]; 980d850f2eSLeila Ghaffari Y[0] = rho_infty / h[0] * Rd * Y[4]; 99*edcfef1bSKenneth E. Jansen return StateFromY(&blasius->newtonian_ctx, Y); 100bb8a0c61SJames Wright } 101bb8a0c61SJames Wright 102bb8a0c61SJames Wright // ***************************************************************************** 103bb8a0c61SJames Wright // This QFunction sets a Blasius boundary layer for the initial condition 104bb8a0c61SJames Wright // ***************************************************************************** 1052b916ea7SJeremy L Thompson CEED_QFUNCTION(ICsBlasius)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 106bb8a0c61SJames Wright const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 107bb8a0c61SJames Wright CeedScalar(*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 108bb8a0c61SJames Wright 109bb8a0c61SJames Wright const BlasiusContext context = (BlasiusContext)ctx; 11033796533SJames Wright const NewtonianIdealGasContext gas = &context->newtonian_ctx; 111bb8a0c61SJames Wright const CeedScalar mu = context->newtonian_ctx.mu; 112bb8a0c61SJames Wright const CeedScalar delta0 = context->delta0; 113ef2c71fdSJames Wright const CeedScalar x_inflow = context->x_inflow; 114e0d1a4dfSLeila Ghaffari CeedScalar t12; 115bb8a0c61SJames Wright 11633796533SJames Wright const CeedScalar Y_inf[5] = {context->P0, context->U_inf, 0, 0, context->T_inf}; 117*edcfef1bSKenneth E. Jansen const State s_inf = StateFromY(gas, Y_inf); 118bb8a0c61SJames Wright 11933796533SJames Wright const CeedScalar x0 = context->U_inf * s_inf.U.density / (mu * 25 / Square(delta0)); 12033796533SJames Wright 12133796533SJames Wright CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 12233796533SJames Wright const CeedScalar x[3] = {X[0][i], X[1][i], X[2][i]}; 12333796533SJames Wright State s = BlasiusSolution(context, x, x0, x_inflow, s_inf.U.density, &t12); 12433796533SJames Wright CeedScalar q[5] = {0}; 12533796533SJames Wright 12633796533SJames Wright switch (gas->state_var) { 12733796533SJames Wright case STATEVAR_CONSERVATIVE: 12833796533SJames Wright UnpackState_U(s.U, q); 12933796533SJames Wright break; 13033796533SJames Wright case STATEVAR_PRIMITIVE: 13133796533SJames Wright UnpackState_Y(s.Y, q); 13233796533SJames Wright break; 13333796533SJames Wright } 13433796533SJames Wright for (CeedInt j = 0; j < 5; j++) q0[j][i] = q[j]; 13533796533SJames Wright } 136bb8a0c61SJames Wright return 0; 137bb8a0c61SJames Wright } 138bb8a0c61SJames Wright 139bb8a0c61SJames Wright // ***************************************************************************** 1402b916ea7SJeremy L Thompson CEED_QFUNCTION(Blasius_Inflow)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 141bb8a0c61SJames Wright // Inputs 1423d65b166SJames Wright const CeedScalar(*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 143ade49511SJames Wright const CeedScalar(*q_data_sur) = in[2]; 1443d65b166SJames Wright const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 145bb8a0c61SJames Wright 146bb8a0c61SJames Wright // Outputs 147bb8a0c61SJames Wright CeedScalar(*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 1483d65b166SJames Wright 149bb8a0c61SJames Wright const BlasiusContext context = (BlasiusContext)ctx; 150ade49511SJames Wright const bool is_implicit = context->implicit; 1510d850f2eSLeila Ghaffari NewtonianIdealGasContext gas = &context->newtonian_ctx; 152bb8a0c61SJames Wright const CeedScalar mu = context->newtonian_ctx.mu; 153e0d1a4dfSLeila Ghaffari const CeedScalar Rd = GasConstant(&context->newtonian_ctx); 154aef1eb53SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 155bb8a0c61SJames Wright const CeedScalar P0 = context->P0; 156bb8a0c61SJames Wright const CeedScalar delta0 = context->delta0; 157aef1eb53SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 158ef2c71fdSJames Wright const CeedScalar x_inflow = context->x_inflow; 1592acc7cbcSKenneth E. Jansen const bool weakT = context->weakT; 160aef1eb53SLeila Ghaffari const CeedScalar rho_0 = P0 / (Rd * T_inf); 161aef1eb53SLeila Ghaffari const CeedScalar x0 = U_inf * rho_0 / (mu * 25 / Square(delta0)); 162bb8a0c61SJames Wright 1633d65b166SJames Wright CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 164ade49511SJames Wright CeedScalar wdetJb, norm[3]; 165ade49511SJames Wright QdataBoundaryUnpack_3D(Q, i, q_data_sur, &wdetJb, NULL, norm); 166ade49511SJames Wright wdetJb *= is_implicit ? -1. : 1.; 167bb8a0c61SJames Wright 1682acc7cbcSKenneth E. Jansen // Calculate inflow values 169e0d1a4dfSLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], 0.}; 170bb8a0c61SJames Wright CeedScalar t12; 171e0d1a4dfSLeila Ghaffari State s = BlasiusSolution(context, x, x0, x_inflow, rho_0, &t12); 1720d850f2eSLeila Ghaffari CeedScalar qi[5]; 1730d850f2eSLeila Ghaffari for (CeedInt j = 0; j < 5; j++) qi[j] = q[j][i]; 174*edcfef1bSKenneth E. Jansen State s_int = StateFromU(gas, qi); 175bb8a0c61SJames Wright 1762acc7cbcSKenneth E. Jansen // enabling user to choose between weak T and weak rho inflow 1770d850f2eSLeila Ghaffari if (weakT) { // density from the current solution 1780d850f2eSLeila Ghaffari s.U.density = s_int.U.density; 179*edcfef1bSKenneth E. Jansen s.Y = StatePrimitiveFromConservative(gas, s.U); 1800d850f2eSLeila Ghaffari } else { // Total energy from current solution 1810d850f2eSLeila Ghaffari s.U.E_total = s_int.U.E_total; 182*edcfef1bSKenneth E. Jansen s.Y = StatePrimitiveFromConservative(gas, s.U); 1832acc7cbcSKenneth E. Jansen } 1840d850f2eSLeila Ghaffari 1850d850f2eSLeila Ghaffari StateConservative Flux_inviscid[3]; 1860d850f2eSLeila Ghaffari FluxInviscid(&context->newtonian_ctx, s, Flux_inviscid); 187bb8a0c61SJames Wright 1882b916ea7SJeremy L Thompson const CeedScalar stress[3][3] = { 1892b916ea7SJeremy L Thompson {0, t12, 0}, 1902b916ea7SJeremy L Thompson {t12, 0, 0}, 1912b916ea7SJeremy L Thompson {0, 0, 0} 1922b916ea7SJeremy L Thompson }; 1930d850f2eSLeila Ghaffari const CeedScalar Fe[3] = {0}; // TODO: viscous energy flux needs grad temperature 1940d850f2eSLeila Ghaffari CeedScalar Flux[5]; 1950d850f2eSLeila Ghaffari FluxTotal_Boundary(Flux_inviscid, stress, Fe, norm, Flux); 1962b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 5; j++) v[j][i] = -wdetJb * Flux[j]; 197ade49511SJames Wright } 198bb8a0c61SJames Wright return 0; 199bb8a0c61SJames Wright } 200bb8a0c61SJames Wright 201e0d1a4dfSLeila Ghaffari // ***************************************************************************** 2022b916ea7SJeremy L Thompson CEED_QFUNCTION(Blasius_Inflow_Jacobian)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 203f0b65372SJed Brown // Inputs 2043d65b166SJames Wright const CeedScalar(*dq)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 205ade49511SJames Wright const CeedScalar(*q_data_sur) = in[2]; 2063d65b166SJames Wright const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 207f0b65372SJed Brown 208f0b65372SJed Brown // Outputs 209f0b65372SJed Brown CeedScalar(*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 2103d65b166SJames Wright 211f0b65372SJed Brown const BlasiusContext context = (BlasiusContext)ctx; 212ade49511SJames Wright const bool is_implicit = context->implicit; 213f0b65372SJed Brown const CeedScalar mu = context->newtonian_ctx.mu; 214f0b65372SJed Brown const CeedScalar cv = context->newtonian_ctx.cv; 215e0d1a4dfSLeila Ghaffari const CeedScalar Rd = GasConstant(&context->newtonian_ctx); 216e0d1a4dfSLeila Ghaffari const CeedScalar gamma = HeatCapacityRatio(&context->newtonian_ctx); 217aef1eb53SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 218f0b65372SJed Brown const CeedScalar P0 = context->P0; 219f0b65372SJed Brown const CeedScalar delta0 = context->delta0; 220aef1eb53SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 221f0b65372SJed Brown const bool weakT = context->weakT; 222aef1eb53SLeila Ghaffari const CeedScalar rho_0 = P0 / (Rd * T_inf); 223aef1eb53SLeila Ghaffari const CeedScalar x0 = U_inf * rho_0 / (mu * 25 / (delta0 * delta0)); 224f0b65372SJed Brown 2253d65b166SJames Wright CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 226ade49511SJames Wright CeedScalar wdetJb, norm[3]; 227ade49511SJames Wright QdataBoundaryUnpack_3D(Q, i, q_data_sur, &wdetJb, NULL, norm); 228ade49511SJames Wright wdetJb *= is_implicit ? -1. : 1.; 229f0b65372SJed Brown 230f0b65372SJed Brown // Calculate inflow values 2310d850f2eSLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], X[2][i]}; 232f0b65372SJed Brown CeedScalar t12; 233e0d1a4dfSLeila Ghaffari State s = BlasiusSolution(context, x, x0, 0, rho_0, &t12); 234f0b65372SJed Brown 235f0b65372SJed Brown // enabling user to choose between weak T and weak rho inflow 236f0b65372SJed Brown CeedScalar drho, dE, dP; 237f0b65372SJed Brown if (weakT) { 238f0b65372SJed Brown // rho should be from the current solution 239f0b65372SJed Brown drho = dq[0][i]; 240aef1eb53SLeila Ghaffari CeedScalar dE_internal = drho * cv * T_inf; 241e0d1a4dfSLeila Ghaffari CeedScalar dE_kinetic = .5 * drho * Dot3(s.Y.velocity, s.Y.velocity); 242f0b65372SJed Brown dE = dE_internal + dE_kinetic; 243aef1eb53SLeila Ghaffari dP = drho * Rd * T_inf; // interior rho with exterior T 244f0b65372SJed Brown } else { // rho specified, E_internal from solution 245f0b65372SJed Brown drho = 0; 246f0b65372SJed Brown dE = dq[4][i]; 247f0b65372SJed Brown dP = dE * (gamma - 1.); 248f0b65372SJed Brown } 249f0b65372SJed Brown 250e0d1a4dfSLeila Ghaffari const CeedScalar u_normal = Dot3(norm, s.Y.velocity); 251f0b65372SJed Brown 252f0b65372SJed Brown v[0][i] = -wdetJb * drho * u_normal; 2532b916ea7SJeremy L Thompson for (int j = 0; j < 3; j++) { 254e0d1a4dfSLeila Ghaffari v[j + 1][i] = -wdetJb * (drho * u_normal * s.Y.velocity[j] + norm[j] * dP); 2552b916ea7SJeremy L Thompson } 256f0b65372SJed Brown v[4][i] = -wdetJb * u_normal * (dE + dP); 257ade49511SJames Wright } 258f0b65372SJed Brown return 0; 259f0b65372SJed Brown } 260f0b65372SJed Brown 261bb8a0c61SJames Wright #endif // blasius_h 262