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 12bb8a0c61SJames Wright #ifndef blasius_h 13bb8a0c61SJames Wright #define blasius_h 14bb8a0c61SJames Wright 15bb8a0c61SJames Wright #include <ceed.h> 16e0d1a4dfSLeila Ghaffari #include "newtonian_state.h" 1715a3537eSJed Brown #include "newtonian_types.h" 18704b8bbeSJames Wright #include "utils.h" 19bb8a0c61SJames Wright 20bb8a0c61SJames Wright typedef struct BlasiusContext_ *BlasiusContext; 21bb8a0c61SJames Wright struct BlasiusContext_ { 22bb8a0c61SJames Wright bool implicit; // !< Using implicit timesteping or not 232acc7cbcSKenneth E. Jansen bool weakT; // !< flag to set Temperature weakly at inflow 24bb8a0c61SJames Wright CeedScalar delta0; // !< Boundary layer height at inflow 25*aef1eb53SLeila Ghaffari CeedScalar U_inf; // !< Velocity at boundary layer edge 26*aef1eb53SLeila Ghaffari CeedScalar T_inf; // !< Temperature at boundary layer edge 27e0d1a4dfSLeila Ghaffari CeedScalar T_wall; // !< Temperature at the wall 28bb8a0c61SJames Wright CeedScalar P0; // !< Pressure at outflow 29ef2c71fdSJames Wright CeedScalar x_inflow; // !< Location of inflow in x 30e0d1a4dfSLeila Ghaffari CeedScalar n_cheb; // !< Number of Chebyshev terms 31e0d1a4dfSLeila Ghaffari CeedScalar *X; // !< Chebyshev polynomial coordinate vector 32e0d1a4dfSLeila Ghaffari CeedScalar eta_max; // !< Maximum eta in the domain 33e0d1a4dfSLeila Ghaffari CeedScalar *Tf_cheb; // !< Chebyshev coefficient for f 34e0d1a4dfSLeila Ghaffari CeedScalar *Th_cheb; // !< Chebyshev coefficient for h 35bb8a0c61SJames Wright struct NewtonianIdealGasContext_ newtonian_ctx; 36bb8a0c61SJames Wright }; 37bb8a0c61SJames Wright 38e0d1a4dfSLeila Ghaffari // ***************************************************************************** 39e0d1a4dfSLeila Ghaffari // This helper function evaluates Chebyshev polynomials with a set of 40e0d1a4dfSLeila Ghaffari // coefficients with all their derivatives represented as a recurrence table. 41e0d1a4dfSLeila Ghaffari // ***************************************************************************** 42e0d1a4dfSLeila Ghaffari CEED_QFUNCTION_HELPER void ChebyshevEval(int N, const double *Tf, double x, 43e0d1a4dfSLeila Ghaffari 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) 47e0d1a4dfSLeila Ghaffari {1, x, 2*x *x - 1}, {0, 1, 4*x}, {0, 0, 4}, {0, 0, 0} 48e0d1a4dfSLeila Ghaffari }; 49e0d1a4dfSLeila Ghaffari for (int i=0; i<4; i++) { 50e0d1a4dfSLeila Ghaffari // i-th derivative of f 51e0d1a4dfSLeila Ghaffari f[i] = table[i][0] * Tf[0] + table[i][1] * Tf[1] + table[i][2] * Tf[2]; 52e0d1a4dfSLeila Ghaffari } 53e0d1a4dfSLeila Ghaffari for (int i=3; i<N; i++) { 54e0d1a4dfSLeila Ghaffari // T_n(x) = 2xT_{n-1}(x) - T_{n-2}(x) 55e0d1a4dfSLeila Ghaffari table[0][i%3] = 2 * x * table[0][(i-1) % 3] - table[0][(i-2)%3]; 56e0d1a4dfSLeila Ghaffari // Differentiate Chebyshev polynomials with the recurrence relation 57e0d1a4dfSLeila Ghaffari for (int j=1; j<4; j++) { 58e0d1a4dfSLeila Ghaffari // T'_{n}(x)/n = 2T_{n-1}(x) + T'_{n-2}(x)/n-2 59e0d1a4dfSLeila Ghaffari table[j][i%3] = i * (2 * table[j-1][(i-1) % 3] + table[j][(i-2)%3] / (i-2)); 60e0d1a4dfSLeila Ghaffari } 61e0d1a4dfSLeila Ghaffari for (int j=0; j<4; j++) { 62e0d1a4dfSLeila Ghaffari f[j] += table[j][i%3] * Tf[i]; 63bb8a0c61SJames Wright } 64bb8a0c61SJames Wright } 65e0d1a4dfSLeila Ghaffari for (int i=1; i<4; i++) { 66e0d1a4dfSLeila Ghaffari // Transform derivatives from Chebyshev [-1, 1] to [0, eta_max]. 67e0d1a4dfSLeila Ghaffari for (int j=0; j<i; j++) f[i] *= dX_deta; 68e0d1a4dfSLeila Ghaffari } 69bb8a0c61SJames Wright } 70bb8a0c61SJames Wright 71e0d1a4dfSLeila Ghaffari // ***************************************************************************** 72e0d1a4dfSLeila Ghaffari // This helper function computes the Blasius boundary layer solution. 73e0d1a4dfSLeila Ghaffari // ***************************************************************************** 74e0d1a4dfSLeila Ghaffari State CEED_QFUNCTION_HELPER(BlasiusSolution)(const BlasiusContext blasius, 75e0d1a4dfSLeila Ghaffari const CeedScalar x[3], const CeedScalar x0, const CeedScalar x_inflow, 76e0d1a4dfSLeila Ghaffari const CeedScalar rho, CeedScalar *t12) { 77e0d1a4dfSLeila Ghaffari CeedInt N = blasius->n_cheb; 78e0d1a4dfSLeila Ghaffari CeedScalar nu = blasius->newtonian_ctx.mu / rho; 79*aef1eb53SLeila Ghaffari CeedScalar eta = x[1]*sqrt(blasius->U_inf/(nu*(x0+x[0]-x_inflow))); 80e0d1a4dfSLeila Ghaffari CeedScalar X = 2 * (eta / blasius->eta_max) - 1.; 81*aef1eb53SLeila Ghaffari CeedScalar U_inf = blasius->U_inf; 82e0d1a4dfSLeila Ghaffari CeedScalar Rd = GasConstant(&blasius->newtonian_ctx); 83e0d1a4dfSLeila Ghaffari 84e0d1a4dfSLeila Ghaffari CeedScalar f[4], h[4]; 85e0d1a4dfSLeila Ghaffari ChebyshevEval(N, blasius->Tf_cheb, X, blasius->eta_max, f); 86e0d1a4dfSLeila Ghaffari ChebyshevEval(N-1, blasius->Th_cheb, X, blasius->eta_max, h); 87e0d1a4dfSLeila Ghaffari 88*aef1eb53SLeila Ghaffari *t12 = rho*nu*U_inf*f[2]*sqrt(U_inf/(nu*(x0+x[0]-x_inflow))); 89e0d1a4dfSLeila Ghaffari 90e0d1a4dfSLeila Ghaffari CeedScalar Y[5]; 91*aef1eb53SLeila Ghaffari Y[1] = U_inf * f[1]; 92*aef1eb53SLeila Ghaffari Y[2] = 0.5*sqrt(nu*U_inf/(x0+x[0]-x_inflow))*(eta*f[1] - f[0]); 93e0d1a4dfSLeila Ghaffari Y[3] = 0.; 94*aef1eb53SLeila Ghaffari Y[4] = blasius->T_inf * h[0]; 95e0d1a4dfSLeila Ghaffari Y[0] = rho * Rd * Y[4]; 96e0d1a4dfSLeila Ghaffari return StateFromY(&blasius->newtonian_ctx, Y, x); 97bb8a0c61SJames Wright } 98bb8a0c61SJames Wright 99bb8a0c61SJames Wright // ***************************************************************************** 100bb8a0c61SJames Wright // This QFunction sets a Blasius boundary layer for the initial condition 101bb8a0c61SJames Wright // ***************************************************************************** 102bb8a0c61SJames Wright CEED_QFUNCTION(ICsBlasius)(void *ctx, CeedInt Q, 103bb8a0c61SJames Wright const CeedScalar *const *in, CeedScalar *const *out) { 104bb8a0c61SJames Wright // Inputs 105bb8a0c61SJames Wright const CeedScalar (*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 106bb8a0c61SJames Wright 107bb8a0c61SJames Wright // Outputs 108bb8a0c61SJames Wright CeedScalar (*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 109bb8a0c61SJames Wright 110bb8a0c61SJames Wright const BlasiusContext context = (BlasiusContext)ctx; 111bb8a0c61SJames Wright const CeedScalar cv = context->newtonian_ctx.cv; 112bb8a0c61SJames Wright const CeedScalar mu = context->newtonian_ctx.mu; 113*aef1eb53SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 114bb8a0c61SJames Wright const CeedScalar P0 = context->P0; 115bb8a0c61SJames Wright const CeedScalar delta0 = context->delta0; 116*aef1eb53SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 117ef2c71fdSJames Wright const CeedScalar x_inflow = context->x_inflow; 118e0d1a4dfSLeila Ghaffari const CeedScalar gamma = HeatCapacityRatio(&context->newtonian_ctx); 119*aef1eb53SLeila Ghaffari const CeedScalar e_internal = cv * T_inf; 120bb8a0c61SJames Wright const CeedScalar rho = P0 / ((gamma - 1) * e_internal); 121*aef1eb53SLeila Ghaffari const CeedScalar x0 = U_inf*rho / (mu*25/(delta0*delta0)); 122e0d1a4dfSLeila Ghaffari CeedScalar t12; 123bb8a0c61SJames Wright 124bb8a0c61SJames Wright // Quadrature Point Loop 125bb8a0c61SJames Wright CeedPragmaSIMD 126bb8a0c61SJames Wright for (CeedInt i=0; i<Q; i++) { 127e0d1a4dfSLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], 0.}; 128e0d1a4dfSLeila Ghaffari State s = BlasiusSolution(context, x, x0, x_inflow, rho, &t12); 129e0d1a4dfSLeila Ghaffari CeedScalar q[5] = {0}; 130e0d1a4dfSLeila Ghaffari UnpackState_U(s.U, q); 131e0d1a4dfSLeila Ghaffari for (CeedInt j=0; j<5; j++) q0[j][i] = q[j]; 132bb8a0c61SJames Wright 133bb8a0c61SJames Wright } // End of Quadrature Point Loop 134bb8a0c61SJames Wright return 0; 135bb8a0c61SJames Wright } 136bb8a0c61SJames Wright 137bb8a0c61SJames Wright // ***************************************************************************** 138bb8a0c61SJames Wright CEED_QFUNCTION(Blasius_Inflow)(void *ctx, CeedInt Q, 139bb8a0c61SJames Wright const CeedScalar *const *in, 140bb8a0c61SJames Wright CeedScalar *const *out) { 141bb8a0c61SJames Wright // *INDENT-OFF* 142bb8a0c61SJames Wright // Inputs 143bb8a0c61SJames Wright const CeedScalar (*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 144dd64951cSJames Wright (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 145dd64951cSJames Wright (*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 146bb8a0c61SJames Wright 147bb8a0c61SJames Wright // Outputs 148bb8a0c61SJames Wright CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 149bb8a0c61SJames Wright // *INDENT-ON* 150bb8a0c61SJames Wright const BlasiusContext context = (BlasiusContext)ctx; 151bb8a0c61SJames Wright const bool implicit = context->implicit; 152bb8a0c61SJames Wright const CeedScalar mu = context->newtonian_ctx.mu; 153bb8a0c61SJames Wright const CeedScalar cv = context->newtonian_ctx.cv; 154e0d1a4dfSLeila Ghaffari const CeedScalar Rd = GasConstant(&context->newtonian_ctx); 155e0d1a4dfSLeila Ghaffari const CeedScalar gamma = HeatCapacityRatio(&context->newtonian_ctx); 156*aef1eb53SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 157bb8a0c61SJames Wright const CeedScalar P0 = context->P0; 158bb8a0c61SJames Wright const CeedScalar delta0 = context->delta0; 159*aef1eb53SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 160ef2c71fdSJames Wright const CeedScalar x_inflow = context->x_inflow; 1612acc7cbcSKenneth E. Jansen const bool weakT = context->weakT; 162*aef1eb53SLeila Ghaffari const CeedScalar rho_0 = P0 / (Rd * T_inf); 163*aef1eb53SLeila Ghaffari const CeedScalar x0 = U_inf*rho_0 / (mu*25/ Square(delta0)); 164bb8a0c61SJames Wright 165bb8a0c61SJames Wright CeedPragmaSIMD 166bb8a0c61SJames Wright // Quadrature Point Loop 167bb8a0c61SJames Wright for (CeedInt i=0; i<Q; i++) { 168bb8a0c61SJames Wright // Setup 169bb8a0c61SJames Wright // -- Interp-to-Interp q_data 170bb8a0c61SJames Wright // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q). 171bb8a0c61SJames Wright // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q). 172bb8a0c61SJames Wright // We can effect this by swapping the sign on this weight 173bb8a0c61SJames Wright const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i]; 174bb8a0c61SJames Wright 1752acc7cbcSKenneth E. Jansen // Calculate inflow values 176e0d1a4dfSLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], 0.}; 177bb8a0c61SJames Wright CeedScalar t12; 178e0d1a4dfSLeila Ghaffari State s = BlasiusSolution(context, x, x0, x_inflow, rho_0, &t12); 179bb8a0c61SJames Wright 1802acc7cbcSKenneth E. Jansen // enabling user to choose between weak T and weak rho inflow 1812acc7cbcSKenneth E. Jansen CeedScalar rho,E_internal, P, E_kinetic; 1822acc7cbcSKenneth E. Jansen if (weakT) { 1832acc7cbcSKenneth E. Jansen // rho should be from the current solution 1842acc7cbcSKenneth E. Jansen rho = q[0][i]; 185*aef1eb53SLeila Ghaffari // Temperature is being set weakly (T_inf) and for constant cv this sets E_internal 186*aef1eb53SLeila Ghaffari E_internal = rho * cv * T_inf; 1872acc7cbcSKenneth E. Jansen // Find pressure using 188*aef1eb53SLeila Ghaffari P = rho*Rd*T_inf; // interior rho with exterior T 189e0d1a4dfSLeila Ghaffari E_kinetic = .5 * rho * Dot3(s.Y.velocity, s.Y.velocity); 1902acc7cbcSKenneth E. Jansen } else { 191*aef1eb53SLeila Ghaffari // Fixing rho weakly on the inflow to a value consistent with T_inf and P0 1922acc7cbcSKenneth E. Jansen rho = rho_0; 193e0d1a4dfSLeila Ghaffari E_kinetic = .5 * rho * Dot3(s.Y.velocity, s.Y.velocity); 1942acc7cbcSKenneth E. Jansen E_internal = q[4][i] - E_kinetic; // uses set rho and u but E from solution 1952acc7cbcSKenneth E. Jansen P = E_internal * (gamma - 1.); 1962acc7cbcSKenneth E. Jansen } 1972acc7cbcSKenneth E. Jansen const CeedScalar E = E_internal + E_kinetic; 198bb8a0c61SJames Wright // ---- Normal vect 199bb8a0c61SJames Wright const CeedScalar norm[3] = {q_data_sur[1][i], 200bb8a0c61SJames Wright q_data_sur[2][i], 201bb8a0c61SJames Wright q_data_sur[3][i] 202bb8a0c61SJames Wright }; 203bb8a0c61SJames Wright 204bb8a0c61SJames Wright // The Physics 205bb8a0c61SJames Wright // Zero v so all future terms can safely sum into it 206493642f1SJames Wright for (CeedInt j=0; j<5; j++) v[j][i] = 0.; 207bb8a0c61SJames Wright 208e0d1a4dfSLeila Ghaffari const CeedScalar u_normal = Dot3(norm, s.Y.velocity); 2099abe94a0SJed Brown const CeedScalar viscous_flux[3] = {-t12 *norm[1], -t12 *norm[0], 0}; 210bb8a0c61SJames Wright 211bb8a0c61SJames Wright // The Physics 212bb8a0c61SJames Wright // -- Density 213bb8a0c61SJames Wright v[0][i] -= wdetJb * rho * u_normal; // interior rho 214bb8a0c61SJames Wright 215bb8a0c61SJames Wright // -- Momentum 216493642f1SJames Wright for (CeedInt j=0; j<3; j++) 217e0d1a4dfSLeila Ghaffari v[j+1][i] -= wdetJb * (rho * u_normal * s.Y.velocity[j] // interior rho 2189abe94a0SJed Brown + norm[j] * P // mixed P 2199abe94a0SJed Brown + viscous_flux[j]); 220bb8a0c61SJames Wright 221bb8a0c61SJames Wright // -- Total Energy Density 222e0d1a4dfSLeila Ghaffari v[4][i] -= wdetJb * (u_normal * (E + P) + Dot3(viscous_flux, s.Y.velocity)); 223bb8a0c61SJames Wright 224bb8a0c61SJames Wright } // End Quadrature Point Loop 225bb8a0c61SJames Wright return 0; 226bb8a0c61SJames Wright } 227bb8a0c61SJames Wright 228e0d1a4dfSLeila Ghaffari // ***************************************************************************** 229f0b65372SJed Brown CEED_QFUNCTION(Blasius_Inflow_Jacobian)(void *ctx, CeedInt Q, 230f0b65372SJed Brown const CeedScalar *const *in, 231f0b65372SJed Brown CeedScalar *const *out) { 232f0b65372SJed Brown // *INDENT-OFF* 233f0b65372SJed Brown // Inputs 234f0b65372SJed Brown const CeedScalar (*dq)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 23568ae065aSJames Wright (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 23668ae065aSJames Wright (*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 237f0b65372SJed Brown 238f0b65372SJed Brown // Outputs 239f0b65372SJed Brown CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 240f0b65372SJed Brown // *INDENT-ON* 241f0b65372SJed Brown const BlasiusContext context = (BlasiusContext)ctx; 242f0b65372SJed Brown const bool implicit = context->implicit; 243f0b65372SJed Brown const CeedScalar mu = context->newtonian_ctx.mu; 244f0b65372SJed Brown const CeedScalar cv = context->newtonian_ctx.cv; 245e0d1a4dfSLeila Ghaffari const CeedScalar Rd = GasConstant(&context->newtonian_ctx); 246e0d1a4dfSLeila Ghaffari const CeedScalar gamma = HeatCapacityRatio(&context->newtonian_ctx); 247*aef1eb53SLeila Ghaffari const CeedScalar T_inf = context->T_inf; 248f0b65372SJed Brown const CeedScalar P0 = context->P0; 249f0b65372SJed Brown const CeedScalar delta0 = context->delta0; 250*aef1eb53SLeila Ghaffari const CeedScalar U_inf = context->U_inf; 251f0b65372SJed Brown const bool weakT = context->weakT; 252*aef1eb53SLeila Ghaffari const CeedScalar rho_0 = P0 / (Rd * T_inf); 253*aef1eb53SLeila Ghaffari const CeedScalar x0 = U_inf*rho_0 / (mu*25/ (delta0*delta0)); 254f0b65372SJed Brown 255f0b65372SJed Brown CeedPragmaSIMD 256f0b65372SJed Brown // Quadrature Point Loop 257f0b65372SJed Brown for (CeedInt i=0; i<Q; i++) { 258f0b65372SJed Brown // Setup 259f0b65372SJed Brown // -- Interp-to-Interp q_data 260f0b65372SJed Brown // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q). 261f0b65372SJed Brown // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q). 262f0b65372SJed Brown // We can effect this by swapping the sign on this weight 263f0b65372SJed Brown const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i]; 264f0b65372SJed Brown 265f0b65372SJed Brown // Calculate inflow values 266e0d1a4dfSLeila Ghaffari const CeedScalar x[3] = {X[0][i], X[1][i], 0.}; 267f0b65372SJed Brown CeedScalar t12; 268e0d1a4dfSLeila Ghaffari State s = BlasiusSolution(context, x, x0, 0, rho_0, &t12); 269f0b65372SJed Brown 270f0b65372SJed Brown // enabling user to choose between weak T and weak rho inflow 271f0b65372SJed Brown CeedScalar drho, dE, dP; 272f0b65372SJed Brown if (weakT) { 273f0b65372SJed Brown // rho should be from the current solution 274f0b65372SJed Brown drho = dq[0][i]; 275*aef1eb53SLeila Ghaffari CeedScalar dE_internal = drho * cv * T_inf; 276e0d1a4dfSLeila Ghaffari CeedScalar dE_kinetic = .5 * drho * Dot3(s.Y.velocity, s.Y.velocity); 277f0b65372SJed Brown dE = dE_internal + dE_kinetic; 278*aef1eb53SLeila Ghaffari dP = drho * Rd * T_inf; // interior rho with exterior T 279f0b65372SJed Brown } else { // rho specified, E_internal from solution 280f0b65372SJed Brown drho = 0; 281f0b65372SJed Brown dE = dq[4][i]; 282f0b65372SJed Brown dP = dE * (gamma - 1.); 283f0b65372SJed Brown } 284f0b65372SJed Brown const CeedScalar norm[3] = {q_data_sur[1][i], 285f0b65372SJed Brown q_data_sur[2][i], 286f0b65372SJed Brown q_data_sur[3][i] 287f0b65372SJed Brown }; 288f0b65372SJed Brown 289e0d1a4dfSLeila Ghaffari const CeedScalar u_normal = Dot3(norm, s.Y.velocity); 290f0b65372SJed Brown 291f0b65372SJed Brown v[0][i] = - wdetJb * drho * u_normal; 292f0b65372SJed Brown for (int j=0; j<3; j++) 293e0d1a4dfSLeila Ghaffari v[j+1][i] = -wdetJb * (drho * u_normal * s.Y.velocity[j] + norm[j] * dP); 294f0b65372SJed Brown v[4][i] = - wdetJb * u_normal * (dE + dP); 295f0b65372SJed Brown } // End Quadrature Point Loop 296f0b65372SJed Brown return 0; 297f0b65372SJed Brown } 298f0b65372SJed Brown 299bb8a0c61SJames Wright #endif // blasius_h 300