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> 15*2b916ea7SJeremy 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 // ***************************************************************************** 41e0d1a4dfSLeila Ghaffari // This helper function evaluates Chebyshev polynomials with a set of 42e0d1a4dfSLeila Ghaffari // coefficients with all their derivatives represented as a recurrence table. 43e0d1a4dfSLeila Ghaffari // ***************************************************************************** 44*2b916ea7SJeremy L Thompson CEED_QFUNCTION_HELPER void ChebyshevEval(int N, const double *Tf, double x, double eta_max, double *f) { 45e0d1a4dfSLeila Ghaffari double dX_deta = 2 / eta_max; 46e0d1a4dfSLeila Ghaffari double table[4][3] = { 47e0d1a4dfSLeila Ghaffari // Chebyshev polynomials T_0, T_1, T_2 of the first kind in (-1,1) 48*2b916ea7SJeremy L Thompson {1, x, 2 * x * x - 1}, 49*2b916ea7SJeremy L Thompson {0, 1, 4 * x }, 50*2b916ea7SJeremy L Thompson {0, 0, 4 }, 51*2b916ea7SJeremy L Thompson {0, 0, 0 } 52e0d1a4dfSLeila Ghaffari }; 53e0d1a4dfSLeila Ghaffari for (int i = 0; i < 4; i++) { 54e0d1a4dfSLeila Ghaffari // i-th derivative of f 55e0d1a4dfSLeila Ghaffari f[i] = table[i][0] * Tf[0] + table[i][1] * Tf[1] + table[i][2] * Tf[2]; 56e0d1a4dfSLeila Ghaffari } 57e0d1a4dfSLeila Ghaffari for (int i = 3; i < N; i++) { 58e0d1a4dfSLeila Ghaffari // T_n(x) = 2xT_{n-1}(x) - T_{n-2}(x) 59e0d1a4dfSLeila Ghaffari table[0][i % 3] = 2 * x * table[0][(i - 1) % 3] - table[0][(i - 2) % 3]; 60e0d1a4dfSLeila Ghaffari // Differentiate Chebyshev polynomials with the recurrence relation 61e0d1a4dfSLeila Ghaffari for (int j = 1; j < 4; j++) { 62e0d1a4dfSLeila Ghaffari // T'_{n}(x)/n = 2T_{n-1}(x) + T'_{n-2}(x)/n-2 63e0d1a4dfSLeila Ghaffari table[j][i % 3] = i * (2 * table[j - 1][(i - 1) % 3] + table[j][(i - 2) % 3] / (i - 2)); 64e0d1a4dfSLeila Ghaffari } 65e0d1a4dfSLeila Ghaffari for (int j = 0; j < 4; j++) { 66e0d1a4dfSLeila Ghaffari f[j] += table[j][i % 3] * Tf[i]; 67bb8a0c61SJames Wright } 68bb8a0c61SJames Wright } 69e0d1a4dfSLeila Ghaffari for (int i = 1; i < 4; i++) { 70e0d1a4dfSLeila Ghaffari // Transform derivatives from Chebyshev [-1, 1] to [0, eta_max]. 71e0d1a4dfSLeila Ghaffari for (int j = 0; j < i; j++) f[i] *= dX_deta; 72e0d1a4dfSLeila Ghaffari } 73bb8a0c61SJames Wright } 74bb8a0c61SJames Wright 75e0d1a4dfSLeila Ghaffari // ***************************************************************************** 76e0d1a4dfSLeila Ghaffari // This helper function computes the Blasius boundary layer solution. 77e0d1a4dfSLeila Ghaffari // ***************************************************************************** 78*2b916ea7SJeremy L Thompson State CEED_QFUNCTION_HELPER(BlasiusSolution)(const BlasiusContext blasius, const CeedScalar x[3], const CeedScalar x0, const CeedScalar x_inflow, 790d850f2eSLeila Ghaffari const CeedScalar rho_infty, CeedScalar *t12) { 80e0d1a4dfSLeila Ghaffari CeedInt N = blasius->n_cheb; 810d850f2eSLeila Ghaffari CeedScalar mu = blasius->newtonian_ctx.mu; 820d850f2eSLeila Ghaffari CeedScalar nu = mu / rho_infty; 83aef1eb53SLeila Ghaffari CeedScalar eta = x[1] * sqrt(blasius->U_inf / (nu * (x0 + x[0] - x_inflow))); 84e0d1a4dfSLeila Ghaffari CeedScalar X = 2 * (eta / blasius->eta_max) - 1.; 85aef1eb53SLeila Ghaffari CeedScalar U_inf = blasius->U_inf; 86e0d1a4dfSLeila Ghaffari CeedScalar Rd = GasConstant(&blasius->newtonian_ctx); 87e0d1a4dfSLeila Ghaffari 88e0d1a4dfSLeila Ghaffari CeedScalar f[4], h[4]; 89e0d1a4dfSLeila Ghaffari ChebyshevEval(N, blasius->Tf_cheb, X, blasius->eta_max, f); 90e0d1a4dfSLeila Ghaffari ChebyshevEval(N - 1, blasius->Th_cheb, X, blasius->eta_max, h); 91e0d1a4dfSLeila Ghaffari 920d850f2eSLeila Ghaffari *t12 = mu * U_inf * f[2] * sqrt(U_inf / (nu * (x0 + x[0] - x_inflow))); 93e0d1a4dfSLeila Ghaffari 94e0d1a4dfSLeila Ghaffari CeedScalar Y[5]; 95aef1eb53SLeila Ghaffari Y[1] = U_inf * f[1]; 96aef1eb53SLeila Ghaffari Y[2] = 0.5 * sqrt(nu * U_inf / (x0 + x[0] - x_inflow)) * (eta * f[1] - f[0]); 97e0d1a4dfSLeila Ghaffari Y[3] = 0.; 98aef1eb53SLeila Ghaffari Y[4] = blasius->T_inf * h[0]; 990d850f2eSLeila Ghaffari Y[0] = rho_infty / h[0] * Rd * Y[4]; 100e0d1a4dfSLeila Ghaffari return StateFromY(&blasius->newtonian_ctx, Y, x); 101bb8a0c61SJames Wright } 102bb8a0c61SJames Wright 103bb8a0c61SJames Wright // ***************************************************************************** 104bb8a0c61SJames Wright // This QFunction sets a Blasius boundary layer for the initial condition 105bb8a0c61SJames Wright // ***************************************************************************** 106*2b916ea7SJeremy L Thompson CEED_QFUNCTION(ICsBlasius)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 107bb8a0c61SJames Wright // Inputs 108bb8a0c61SJames Wright const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 109bb8a0c61SJames Wright 110bb8a0c61SJames Wright // Outputs 111bb8a0c61SJames Wright CeedScalar(*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 112bb8a0c61SJames Wright 113bb8a0c61SJames Wright const BlasiusContext context = (BlasiusContext)ctx; 114bb8a0c61SJames Wright const CeedScalar cv = context->newtonian_ctx.cv; 115bb8a0c61SJames Wright const CeedScalar mu = context->newtonian_ctx.mu; 116aef1eb53SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 117bb8a0c61SJames Wright const CeedScalar P0 = context->P0; 118bb8a0c61SJames Wright const CeedScalar delta0 = context->delta0; 119aef1eb53SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 120ef2c71fdSJames Wright const CeedScalar x_inflow = context->x_inflow; 121e0d1a4dfSLeila Ghaffari const CeedScalar gamma = HeatCapacityRatio(&context->newtonian_ctx); 122aef1eb53SLeila Ghaffari const CeedScalar e_internal = cv * T_inf; 123bb8a0c61SJames Wright const CeedScalar rho = P0 / ((gamma - 1) * e_internal); 124aef1eb53SLeila Ghaffari const CeedScalar x0 = U_inf * rho / (mu * 25 / (delta0 * delta0)); 125e0d1a4dfSLeila Ghaffari CeedScalar t12; 126bb8a0c61SJames Wright 127bb8a0c61SJames Wright // Quadrature Point Loop 128*2b916ea7SJeremy L Thompson CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 129e0d1a4dfSLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], 0.}; 130e0d1a4dfSLeila Ghaffari State s = BlasiusSolution(context, x, x0, x_inflow, rho, &t12); 131e0d1a4dfSLeila Ghaffari CeedScalar q[5] = {0}; 132e0d1a4dfSLeila Ghaffari UnpackState_U(s.U, q); 133e0d1a4dfSLeila Ghaffari for (CeedInt j = 0; j < 5; j++) q0[j][i] = q[j]; 134bb8a0c61SJames Wright 135bb8a0c61SJames Wright } // End of Quadrature Point Loop 136bb8a0c61SJames Wright return 0; 137bb8a0c61SJames Wright } 138bb8a0c61SJames Wright 139bb8a0c61SJames Wright // ***************************************************************************** 140*2b916ea7SJeremy L Thompson CEED_QFUNCTION(Blasius_Inflow)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 141bb8a0c61SJames Wright // *INDENT-OFF* 142bb8a0c61SJames Wright // Inputs 143*2b916ea7SJeremy L Thompson const CeedScalar(*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 144dd64951cSJames Wright (*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]; 148bb8a0c61SJames Wright // *INDENT-ON* 149bb8a0c61SJames Wright const BlasiusContext context = (BlasiusContext)ctx; 150bb8a0c61SJames Wright const bool 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 163bb8a0c61SJames Wright CeedPragmaSIMD 164bb8a0c61SJames Wright // Quadrature Point Loop 165bb8a0c61SJames Wright for (CeedInt i = 0; i < Q; i++) { 166bb8a0c61SJames Wright // Setup 167bb8a0c61SJames Wright // -- Interp-to-Interp q_data 168bb8a0c61SJames Wright // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q). 169bb8a0c61SJames Wright // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q). 170bb8a0c61SJames Wright // We can effect this by swapping the sign on this weight 171bb8a0c61SJames Wright const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i]; 172bb8a0c61SJames Wright 1732acc7cbcSKenneth E. Jansen // Calculate inflow values 174e0d1a4dfSLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], 0.}; 175bb8a0c61SJames Wright CeedScalar t12; 176e0d1a4dfSLeila Ghaffari State s = BlasiusSolution(context, x, x0, x_inflow, rho_0, &t12); 1770d850f2eSLeila Ghaffari CeedScalar qi[5]; 1780d850f2eSLeila Ghaffari for (CeedInt j = 0; j < 5; j++) qi[j] = q[j][i]; 1790d850f2eSLeila Ghaffari State s_int = StateFromU(gas, qi, x); 180bb8a0c61SJames Wright 1812acc7cbcSKenneth E. Jansen // enabling user to choose between weak T and weak rho inflow 1820d850f2eSLeila Ghaffari if (weakT) { // density from the current solution 1830d850f2eSLeila Ghaffari s.U.density = s_int.U.density; 1840d850f2eSLeila Ghaffari s.Y = StatePrimitiveFromConservative(gas, s.U, x); 1850d850f2eSLeila Ghaffari } else { // Total energy from current solution 1860d850f2eSLeila Ghaffari s.U.E_total = s_int.U.E_total; 1870d850f2eSLeila Ghaffari s.Y = StatePrimitiveFromConservative(gas, s.U, x); 1882acc7cbcSKenneth E. Jansen } 1890d850f2eSLeila Ghaffari 190bb8a0c61SJames Wright // ---- Normal vect 191*2b916ea7SJeremy L Thompson const CeedScalar norm[3] = {q_data_sur[1][i], q_data_sur[2][i], q_data_sur[3][i]}; 192bb8a0c61SJames Wright 1930d850f2eSLeila Ghaffari StateConservative Flux_inviscid[3]; 1940d850f2eSLeila Ghaffari FluxInviscid(&context->newtonian_ctx, s, Flux_inviscid); 195bb8a0c61SJames Wright 196*2b916ea7SJeremy L Thompson const CeedScalar stress[3][3] = { 197*2b916ea7SJeremy L Thompson {0, t12, 0}, 198*2b916ea7SJeremy L Thompson {t12, 0, 0}, 199*2b916ea7SJeremy L Thompson {0, 0, 0} 200*2b916ea7SJeremy L Thompson }; 2010d850f2eSLeila Ghaffari const CeedScalar Fe[3] = {0}; // TODO: viscous energy flux needs grad temperature 2020d850f2eSLeila Ghaffari CeedScalar Flux[5]; 2030d850f2eSLeila Ghaffari FluxTotal_Boundary(Flux_inviscid, stress, Fe, norm, Flux); 204*2b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 5; j++) v[j][i] = -wdetJb * Flux[j]; 205bb8a0c61SJames Wright } // End Quadrature Point Loop 206bb8a0c61SJames Wright return 0; 207bb8a0c61SJames Wright } 208bb8a0c61SJames Wright 209e0d1a4dfSLeila Ghaffari // ***************************************************************************** 210*2b916ea7SJeremy L Thompson CEED_QFUNCTION(Blasius_Inflow_Jacobian)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 211f0b65372SJed Brown // *INDENT-OFF* 212f0b65372SJed Brown // Inputs 213*2b916ea7SJeremy L Thompson const CeedScalar(*dq)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 21468ae065aSJames Wright (*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 215f0b65372SJed Brown 216f0b65372SJed Brown // Outputs 217f0b65372SJed Brown CeedScalar(*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 218f0b65372SJed Brown // *INDENT-ON* 219f0b65372SJed Brown const BlasiusContext context = (BlasiusContext)ctx; 220f0b65372SJed Brown const bool implicit = context->implicit; 221f0b65372SJed Brown const CeedScalar mu = context->newtonian_ctx.mu; 222f0b65372SJed Brown const CeedScalar cv = context->newtonian_ctx.cv; 223e0d1a4dfSLeila Ghaffari const CeedScalar Rd = GasConstant(&context->newtonian_ctx); 224e0d1a4dfSLeila Ghaffari const CeedScalar gamma = HeatCapacityRatio(&context->newtonian_ctx); 225aef1eb53SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 226f0b65372SJed Brown const CeedScalar P0 = context->P0; 227f0b65372SJed Brown const CeedScalar delta0 = context->delta0; 228aef1eb53SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 229f0b65372SJed Brown const bool weakT = context->weakT; 230aef1eb53SLeila Ghaffari const CeedScalar rho_0 = P0 / (Rd * T_inf); 231aef1eb53SLeila Ghaffari const CeedScalar x0 = U_inf * rho_0 / (mu * 25 / (delta0 * delta0)); 232f0b65372SJed Brown 233f0b65372SJed Brown CeedPragmaSIMD 234f0b65372SJed Brown // Quadrature Point Loop 235f0b65372SJed Brown for (CeedInt i = 0; i < Q; i++) { 236f0b65372SJed Brown // Setup 237f0b65372SJed Brown // -- Interp-to-Interp q_data 238f0b65372SJed Brown // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q). 239f0b65372SJed Brown // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q). 240f0b65372SJed Brown // We can effect this by swapping the sign on this weight 241f0b65372SJed Brown const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i]; 242f0b65372SJed Brown 243f0b65372SJed Brown // Calculate inflow values 2440d850f2eSLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], X[2][i]}; 245f0b65372SJed Brown CeedScalar t12; 246e0d1a4dfSLeila Ghaffari State s = BlasiusSolution(context, x, x0, 0, rho_0, &t12); 247f0b65372SJed Brown 248f0b65372SJed Brown // enabling user to choose between weak T and weak rho inflow 249f0b65372SJed Brown CeedScalar drho, dE, dP; 250f0b65372SJed Brown if (weakT) { 251f0b65372SJed Brown // rho should be from the current solution 252f0b65372SJed Brown drho = dq[0][i]; 253aef1eb53SLeila Ghaffari CeedScalar dE_internal = drho * cv * T_inf; 254e0d1a4dfSLeila Ghaffari CeedScalar dE_kinetic = .5 * drho * Dot3(s.Y.velocity, s.Y.velocity); 255f0b65372SJed Brown dE = dE_internal + dE_kinetic; 256aef1eb53SLeila Ghaffari dP = drho * Rd * T_inf; // interior rho with exterior T 257f0b65372SJed Brown } else { // rho specified, E_internal from solution 258f0b65372SJed Brown drho = 0; 259f0b65372SJed Brown dE = dq[4][i]; 260f0b65372SJed Brown dP = dE * (gamma - 1.); 261f0b65372SJed Brown } 262*2b916ea7SJeremy L Thompson const CeedScalar norm[3] = {q_data_sur[1][i], q_data_sur[2][i], q_data_sur[3][i]}; 263f0b65372SJed Brown 264e0d1a4dfSLeila Ghaffari const CeedScalar u_normal = Dot3(norm, s.Y.velocity); 265f0b65372SJed Brown 266f0b65372SJed Brown v[0][i] = -wdetJb * drho * u_normal; 267*2b916ea7SJeremy L Thompson for (int j = 0; j < 3; j++) { 268e0d1a4dfSLeila Ghaffari v[j + 1][i] = -wdetJb * (drho * u_normal * s.Y.velocity[j] + norm[j] * dP); 269*2b916ea7SJeremy L Thompson } 270f0b65372SJed Brown v[4][i] = -wdetJb * u_normal * (dE + dP); 271f0b65372SJed Brown } // End Quadrature Point Loop 272f0b65372SJed Brown return 0; 273f0b65372SJed Brown } 274f0b65372SJed Brown 275bb8a0c61SJames Wright #endif // blasius_h 276