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 // ***************************************************************************** 41*04e40bb6SJeremy 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]; 99e0d1a4dfSLeila Ghaffari return StateFromY(&blasius->newtonian_ctx, Y, x); 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 // Inputs 107bb8a0c61SJames Wright const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 108bb8a0c61SJames Wright 109bb8a0c61SJames Wright // Outputs 110bb8a0c61SJames Wright CeedScalar(*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 111bb8a0c61SJames Wright 112bb8a0c61SJames Wright const BlasiusContext context = (BlasiusContext)ctx; 113bb8a0c61SJames Wright const CeedScalar cv = context->newtonian_ctx.cv; 114bb8a0c61SJames Wright const CeedScalar mu = context->newtonian_ctx.mu; 115aef1eb53SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 116bb8a0c61SJames Wright const CeedScalar P0 = context->P0; 117bb8a0c61SJames Wright const CeedScalar delta0 = context->delta0; 118aef1eb53SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 119ef2c71fdSJames Wright const CeedScalar x_inflow = context->x_inflow; 120e0d1a4dfSLeila Ghaffari const CeedScalar gamma = HeatCapacityRatio(&context->newtonian_ctx); 121aef1eb53SLeila Ghaffari const CeedScalar e_internal = cv * T_inf; 122bb8a0c61SJames Wright const CeedScalar rho = P0 / ((gamma - 1) * e_internal); 123aef1eb53SLeila Ghaffari const CeedScalar x0 = U_inf * rho / (mu * 25 / (delta0 * delta0)); 124e0d1a4dfSLeila Ghaffari CeedScalar t12; 125bb8a0c61SJames Wright 126bb8a0c61SJames Wright // Quadrature Point Loop 1272b916ea7SJeremy L Thompson CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 128e0d1a4dfSLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], 0.}; 129e0d1a4dfSLeila Ghaffari State s = BlasiusSolution(context, x, x0, x_inflow, rho, &t12); 130e0d1a4dfSLeila Ghaffari CeedScalar q[5] = {0}; 131e0d1a4dfSLeila Ghaffari UnpackState_U(s.U, q); 132e0d1a4dfSLeila Ghaffari for (CeedInt j = 0; j < 5; j++) q0[j][i] = q[j]; 133bb8a0c61SJames Wright 134bb8a0c61SJames Wright } // End of Quadrature Point Loop 135bb8a0c61SJames Wright return 0; 136bb8a0c61SJames Wright } 137bb8a0c61SJames Wright 138bb8a0c61SJames Wright // ***************************************************************************** 1392b916ea7SJeremy L Thompson CEED_QFUNCTION(Blasius_Inflow)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 140bb8a0c61SJames Wright // Inputs 1413d65b166SJames Wright const CeedScalar(*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 1423d65b166SJames Wright const CeedScalar(*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2]; 1433d65b166SJames Wright const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 144bb8a0c61SJames Wright 145bb8a0c61SJames Wright // Outputs 146bb8a0c61SJames Wright CeedScalar(*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 1473d65b166SJames Wright 148bb8a0c61SJames Wright const BlasiusContext context = (BlasiusContext)ctx; 149bb8a0c61SJames Wright const bool implicit = context->implicit; 1500d850f2eSLeila Ghaffari NewtonianIdealGasContext gas = &context->newtonian_ctx; 151bb8a0c61SJames Wright const CeedScalar mu = context->newtonian_ctx.mu; 152e0d1a4dfSLeila Ghaffari const CeedScalar Rd = GasConstant(&context->newtonian_ctx); 153aef1eb53SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 154bb8a0c61SJames Wright const CeedScalar P0 = context->P0; 155bb8a0c61SJames Wright const CeedScalar delta0 = context->delta0; 156aef1eb53SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 157ef2c71fdSJames Wright const CeedScalar x_inflow = context->x_inflow; 1582acc7cbcSKenneth E. Jansen const bool weakT = context->weakT; 159aef1eb53SLeila Ghaffari const CeedScalar rho_0 = P0 / (Rd * T_inf); 160aef1eb53SLeila Ghaffari const CeedScalar x0 = U_inf * rho_0 / (mu * 25 / Square(delta0)); 161bb8a0c61SJames Wright 162bb8a0c61SJames Wright // Quadrature Point Loop 1633d65b166SJames Wright CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 164bb8a0c61SJames Wright // Setup 165bb8a0c61SJames Wright // -- Interp-to-Interp q_data 166bb8a0c61SJames Wright // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q). 167bb8a0c61SJames Wright // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q). 168bb8a0c61SJames Wright // We can effect this by swapping the sign on this weight 169bb8a0c61SJames Wright const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i]; 170bb8a0c61SJames Wright 1712acc7cbcSKenneth E. Jansen // Calculate inflow values 172e0d1a4dfSLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], 0.}; 173bb8a0c61SJames Wright CeedScalar t12; 174e0d1a4dfSLeila Ghaffari State s = BlasiusSolution(context, x, x0, x_inflow, rho_0, &t12); 1750d850f2eSLeila Ghaffari CeedScalar qi[5]; 1760d850f2eSLeila Ghaffari for (CeedInt j = 0; j < 5; j++) qi[j] = q[j][i]; 1770d850f2eSLeila Ghaffari State s_int = StateFromU(gas, qi, x); 178bb8a0c61SJames Wright 1792acc7cbcSKenneth E. Jansen // enabling user to choose between weak T and weak rho inflow 1800d850f2eSLeila Ghaffari if (weakT) { // density from the current solution 1810d850f2eSLeila Ghaffari s.U.density = s_int.U.density; 1820d850f2eSLeila Ghaffari s.Y = StatePrimitiveFromConservative(gas, s.U, x); 1830d850f2eSLeila Ghaffari } else { // Total energy from current solution 1840d850f2eSLeila Ghaffari s.U.E_total = s_int.U.E_total; 1850d850f2eSLeila Ghaffari s.Y = StatePrimitiveFromConservative(gas, s.U, x); 1862acc7cbcSKenneth E. Jansen } 1870d850f2eSLeila Ghaffari 188bb8a0c61SJames Wright // ---- Normal vect 1892b916ea7SJeremy L Thompson const CeedScalar norm[3] = {q_data_sur[1][i], q_data_sur[2][i], q_data_sur[3][i]}; 190bb8a0c61SJames Wright 1910d850f2eSLeila Ghaffari StateConservative Flux_inviscid[3]; 1920d850f2eSLeila Ghaffari FluxInviscid(&context->newtonian_ctx, s, Flux_inviscid); 193bb8a0c61SJames Wright 1942b916ea7SJeremy L Thompson const CeedScalar stress[3][3] = { 1952b916ea7SJeremy L Thompson {0, t12, 0}, 1962b916ea7SJeremy L Thompson {t12, 0, 0}, 1972b916ea7SJeremy L Thompson {0, 0, 0} 1982b916ea7SJeremy L Thompson }; 1990d850f2eSLeila Ghaffari const CeedScalar Fe[3] = {0}; // TODO: viscous energy flux needs grad temperature 2000d850f2eSLeila Ghaffari CeedScalar Flux[5]; 2010d850f2eSLeila Ghaffari FluxTotal_Boundary(Flux_inviscid, stress, Fe, norm, Flux); 2022b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 5; j++) v[j][i] = -wdetJb * Flux[j]; 203bb8a0c61SJames Wright } // End Quadrature Point Loop 204bb8a0c61SJames Wright return 0; 205bb8a0c61SJames Wright } 206bb8a0c61SJames Wright 207e0d1a4dfSLeila Ghaffari // ***************************************************************************** 2082b916ea7SJeremy L Thompson CEED_QFUNCTION(Blasius_Inflow_Jacobian)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 209f0b65372SJed Brown // Inputs 2103d65b166SJames Wright const CeedScalar(*dq)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 2113d65b166SJames Wright const CeedScalar(*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2]; 2123d65b166SJames Wright const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 213f0b65372SJed Brown 214f0b65372SJed Brown // Outputs 215f0b65372SJed Brown CeedScalar(*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 2163d65b166SJames Wright 217f0b65372SJed Brown const BlasiusContext context = (BlasiusContext)ctx; 218f0b65372SJed Brown const bool implicit = context->implicit; 219f0b65372SJed Brown const CeedScalar mu = context->newtonian_ctx.mu; 220f0b65372SJed Brown const CeedScalar cv = context->newtonian_ctx.cv; 221e0d1a4dfSLeila Ghaffari const CeedScalar Rd = GasConstant(&context->newtonian_ctx); 222e0d1a4dfSLeila Ghaffari const CeedScalar gamma = HeatCapacityRatio(&context->newtonian_ctx); 223aef1eb53SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 224f0b65372SJed Brown const CeedScalar P0 = context->P0; 225f0b65372SJed Brown const CeedScalar delta0 = context->delta0; 226aef1eb53SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 227f0b65372SJed Brown const bool weakT = context->weakT; 228aef1eb53SLeila Ghaffari const CeedScalar rho_0 = P0 / (Rd * T_inf); 229aef1eb53SLeila Ghaffari const CeedScalar x0 = U_inf * rho_0 / (mu * 25 / (delta0 * delta0)); 230f0b65372SJed Brown 231f0b65372SJed Brown // Quadrature Point Loop 2323d65b166SJames Wright CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 233f0b65372SJed Brown // Setup 234f0b65372SJed Brown // -- Interp-to-Interp q_data 235f0b65372SJed Brown // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q). 236f0b65372SJed Brown // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q). 237f0b65372SJed Brown // We can effect this by swapping the sign on this weight 238f0b65372SJed Brown const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i]; 239f0b65372SJed Brown 240f0b65372SJed Brown // Calculate inflow values 2410d850f2eSLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], X[2][i]}; 242f0b65372SJed Brown CeedScalar t12; 243e0d1a4dfSLeila Ghaffari State s = BlasiusSolution(context, x, x0, 0, rho_0, &t12); 244f0b65372SJed Brown 245f0b65372SJed Brown // enabling user to choose between weak T and weak rho inflow 246f0b65372SJed Brown CeedScalar drho, dE, dP; 247f0b65372SJed Brown if (weakT) { 248f0b65372SJed Brown // rho should be from the current solution 249f0b65372SJed Brown drho = dq[0][i]; 250aef1eb53SLeila Ghaffari CeedScalar dE_internal = drho * cv * T_inf; 251e0d1a4dfSLeila Ghaffari CeedScalar dE_kinetic = .5 * drho * Dot3(s.Y.velocity, s.Y.velocity); 252f0b65372SJed Brown dE = dE_internal + dE_kinetic; 253aef1eb53SLeila Ghaffari dP = drho * Rd * T_inf; // interior rho with exterior T 254f0b65372SJed Brown } else { // rho specified, E_internal from solution 255f0b65372SJed Brown drho = 0; 256f0b65372SJed Brown dE = dq[4][i]; 257f0b65372SJed Brown dP = dE * (gamma - 1.); 258f0b65372SJed Brown } 2592b916ea7SJeremy L Thompson const CeedScalar norm[3] = {q_data_sur[1][i], q_data_sur[2][i], q_data_sur[3][i]}; 260f0b65372SJed Brown 261e0d1a4dfSLeila Ghaffari const CeedScalar u_normal = Dot3(norm, s.Y.velocity); 262f0b65372SJed Brown 263f0b65372SJed Brown v[0][i] = -wdetJb * drho * u_normal; 2642b916ea7SJeremy L Thompson for (int j = 0; j < 3; j++) { 265e0d1a4dfSLeila Ghaffari v[j + 1][i] = -wdetJb * (drho * u_normal * s.Y.velocity[j] + norm[j] * dP); 2662b916ea7SJeremy L Thompson } 267f0b65372SJed Brown v[4][i] = -wdetJb * u_normal * (dE + dP); 268f0b65372SJed Brown } // End Quadrature Point Loop 269f0b65372SJed Brown return 0; 270f0b65372SJed Brown } 271f0b65372SJed Brown 272bb8a0c61SJames Wright #endif // blasius_h 273