xref: /honee/qfunctions/blasius.h (revision aef1eb5380903bd55ea4d009b07c78f59013fb38)
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
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