xref: /honee/qfunctions/channel.h (revision 3636f6a432a14bcac5c6abf08c00ac5c2941efb7)
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 channel_h
13bb8a0c61SJames Wright #define channel_h
14bb8a0c61SJames Wright 
15d0cce58aSJeremy L Thompson #include <ceed.h>
16bb8a0c61SJames Wright #include <math.h>
17cbe60e31SLeila Ghaffari #include "newtonian_state.h"
18d0cce58aSJeremy L Thompson #include "newtonian_types.h"
19704b8bbeSJames Wright #include "utils.h"
20bb8a0c61SJames Wright 
21bb8a0c61SJames Wright typedef struct ChannelContext_ *ChannelContext;
22bb8a0c61SJames Wright struct ChannelContext_ {
23bb8a0c61SJames Wright   bool       implicit; // !< Using implicit timesteping or not
24bb8a0c61SJames Wright   CeedScalar theta0;   // !< Reference temperature
25bb8a0c61SJames Wright   CeedScalar P0;       // !< Reference Pressure
26bb8a0c61SJames Wright   CeedScalar umax;     // !< Centerline velocity
27bb8a0c61SJames Wright   CeedScalar center;   // !< Y Coordinate for center of channel
28bb8a0c61SJames Wright   CeedScalar H;        // !< Channel half-height
29bb8a0c61SJames Wright   CeedScalar B;        // !< Body-force driving the flow
30bb8a0c61SJames Wright   struct NewtonianIdealGasContext_ newtonian_ctx;
31bb8a0c61SJames Wright };
32bb8a0c61SJames Wright 
33cbe60e31SLeila Ghaffari CEED_QFUNCTION_HELPER State Exact_Channel(CeedInt dim, CeedScalar time,
34cbe60e31SLeila Ghaffari     const CeedScalar X[], CeedInt Nf, void *ctx) {
35bb8a0c61SJames Wright 
36bb8a0c61SJames Wright   const ChannelContext context = (ChannelContext)ctx;
37bb8a0c61SJames Wright   const CeedScalar theta0      = context->theta0;
38bb8a0c61SJames Wright   const CeedScalar P0          = context->P0;
39bb8a0c61SJames Wright   const CeedScalar umax        = context->umax;
40bb8a0c61SJames Wright   const CeedScalar center      = context->center;
41bb8a0c61SJames Wright   const CeedScalar H           = context->H;
42cbe60e31SLeila Ghaffari   NewtonianIdealGasContext gas = &context->newtonian_ctx;
43cbe60e31SLeila Ghaffari   const CeedScalar cp          = gas->cp;
44cbe60e31SLeila Ghaffari   const CeedScalar mu          = gas->mu;
45cbe60e31SLeila Ghaffari   const CeedScalar k           = gas->k;
46cbe60e31SLeila Ghaffari   // There is a gravity body force but it is excluded from
47cbe60e31SLeila Ghaffari   //   the potential energy due to periodicity.
48d1b9ef12SLeila Ghaffari   //     g = (g, 0, 0)
49d1b9ef12SLeila Ghaffari   //     x = (0, x_2, x_3)
50d1b9ef12SLeila Ghaffari   //     e_potential = dot(g, x) = 0
51d1b9ef12SLeila Ghaffari   const CeedScalar x[3] = {0, X[1], X[2]};
52bb8a0c61SJames Wright 
53bb8a0c61SJames Wright   const CeedScalar Pr    = mu / (cp*k);
54bb8a0c61SJames Wright   const CeedScalar Ec    = (umax*umax) / (cp*theta0);
55c58dce4fSJed Brown   const CeedScalar theta = theta0*(1 + (Pr*Ec/3)
56d1b9ef12SLeila Ghaffari                                    * (1 - Square(Square((x[1]-center)/H))));
57cbe60e31SLeila Ghaffari   CeedScalar Y[5] = {0.};
58cbe60e31SLeila Ghaffari   Y[0] = P0;
59d1b9ef12SLeila Ghaffari   Y[1] = umax*(1 - Square((x[1]-center)/H));
60cbe60e31SLeila Ghaffari   Y[2] = 0.;
61cbe60e31SLeila Ghaffari   Y[3] = 0.;
62cbe60e31SLeila Ghaffari   Y[4] = theta;
63bb8a0c61SJames Wright 
64d1b9ef12SLeila Ghaffari   return StateFromY(gas, Y, x);
65bb8a0c61SJames Wright }
66bb8a0c61SJames Wright 
67bb8a0c61SJames Wright // *****************************************************************************
68cbe60e31SLeila Ghaffari // This QFunction set the initial condition
69bb8a0c61SJames Wright // *****************************************************************************
70bb8a0c61SJames Wright CEED_QFUNCTION(ICsChannel)(void *ctx, CeedInt Q,
71bb8a0c61SJames Wright                            const CeedScalar *const *in, CeedScalar *const *out) {
72bb8a0c61SJames Wright   // Inputs
73bb8a0c61SJames Wright   const CeedScalar (*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0];
74bb8a0c61SJames Wright 
75bb8a0c61SJames Wright   // Outputs
76bb8a0c61SJames Wright   CeedScalar (*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0];
77bb8a0c61SJames Wright 
78cbe60e31SLeila Ghaffari   // Context
79cbe60e31SLeila Ghaffari   const ChannelContext context = (ChannelContext)ctx;
80cbe60e31SLeila Ghaffari 
81bb8a0c61SJames Wright   // Quadrature Point Loop
82bb8a0c61SJames Wright   CeedPragmaSIMD
83bb8a0c61SJames Wright   for (CeedInt i=0; i<Q; i++) {
84bb8a0c61SJames Wright     const CeedScalar x[] = {X[0][i], X[1][i], X[2][i]};
85cbe60e31SLeila Ghaffari     State s = Exact_Channel(3, 0., x, 5, ctx);
86d1b9ef12SLeila Ghaffari     CeedScalar q[5] = {0};
87*3636f6a4SJames Wright     switch (context->newtonian_ctx.state_var) {
88*3636f6a4SJames Wright     case STATEVAR_CONSERVATIVE:
89d1b9ef12SLeila Ghaffari       UnpackState_U(s.U, q);
90*3636f6a4SJames Wright       break;
91*3636f6a4SJames Wright     case STATEVAR_PRIMITIVE:
92*3636f6a4SJames Wright       UnpackState_Y(s.Y, q);
93*3636f6a4SJames Wright       break;
94*3636f6a4SJames Wright     }
95d1b9ef12SLeila Ghaffari 
96d1b9ef12SLeila Ghaffari     for (CeedInt j=0; j<5; j++)
97d1b9ef12SLeila Ghaffari       q0[j][i] = q[j];
98bb8a0c61SJames Wright 
99bb8a0c61SJames Wright   } // End of Quadrature Point Loop
100bb8a0c61SJames Wright   return 0;
101bb8a0c61SJames Wright }
102bb8a0c61SJames Wright 
103bb8a0c61SJames Wright // *****************************************************************************
104d1b9ef12SLeila Ghaffari // This QFunction set the inflow boundary condition for conservative variables
105d1b9ef12SLeila Ghaffari // *****************************************************************************
106bb8a0c61SJames Wright CEED_QFUNCTION(Channel_Inflow)(void *ctx, CeedInt Q,
107bb8a0c61SJames Wright                                const CeedScalar *const *in,
108bb8a0c61SJames Wright                                CeedScalar *const *out) {
109bb8a0c61SJames Wright   // *INDENT-OFF*
110bb8a0c61SJames Wright   // Inputs
111bb8a0c61SJames Wright   const CeedScalar (*q)[CEED_Q_VLA]          = (const CeedScalar(*)[CEED_Q_VLA])in[0],
112dd64951cSJames Wright                    (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2],
113dd64951cSJames Wright                    (*X)[CEED_Q_VLA]          = (const CeedScalar(*)[CEED_Q_VLA])in[3];
114bb8a0c61SJames Wright 
115bb8a0c61SJames Wright   // Outputs
116bb8a0c61SJames Wright   CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0];
117bb8a0c61SJames Wright   // *INDENT-ON*
118bb8a0c61SJames Wright   const ChannelContext context = (ChannelContext)ctx;
119bb8a0c61SJames Wright   const bool implicit          = context->implicit;
120d1b9ef12SLeila Ghaffari   NewtonianIdealGasContext gas = &context->newtonian_ctx;
121d1b9ef12SLeila Ghaffari   const CeedScalar cv          = gas->cv;
122d1b9ef12SLeila Ghaffari   const CeedScalar cp          = gas->cp;
123bb8a0c61SJames Wright   const CeedScalar gamma       = cp / cv;
124bb8a0c61SJames Wright 
125bb8a0c61SJames Wright   CeedPragmaSIMD
126bb8a0c61SJames Wright   // Quadrature Point Loop
127bb8a0c61SJames Wright   for (CeedInt i=0; i<Q; i++) {
128bb8a0c61SJames Wright     // Setup
129bb8a0c61SJames Wright     // -- Interp-to-Interp q_data
130bb8a0c61SJames Wright     // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q).
131bb8a0c61SJames Wright     // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q).
132bb8a0c61SJames Wright     // We can effect this by swapping the sign on this weight
133bb8a0c61SJames Wright     const CeedScalar wdetJb  = (implicit ? -1. : 1.) * q_data_sur[0][i];
134bb8a0c61SJames Wright 
135d1b9ef12SLeila Ghaffari     // There is a gravity body force but it is excluded from
136d1b9ef12SLeila Ghaffari     //   the potential energy due to periodicity.
137d1b9ef12SLeila Ghaffari     //     g = (g, 0, 0)
138d1b9ef12SLeila Ghaffari     //     x = (0, x_2, x_3)
139d1b9ef12SLeila Ghaffari     //     e_potential = dot(g, x) = 0
140d1b9ef12SLeila Ghaffari     const CeedScalar x[3] = {0, X[1][i], X[2][i]};
141d1b9ef12SLeila Ghaffari 
142bb8a0c61SJames Wright     // Calcualte prescribed inflow values
143d1b9ef12SLeila Ghaffari     State s_exact = Exact_Channel(3, 0., x, 5, ctx);
144bb8a0c61SJames Wright     CeedScalar q_exact[5] = {0.};
145d1b9ef12SLeila Ghaffari     UnpackState_U(s_exact.U, q_exact);
146bb8a0c61SJames Wright 
147bb8a0c61SJames Wright     // Find pressure using state inside the domain
148d1b9ef12SLeila Ghaffari     CeedScalar q_inside[5] = {0};
1498ed70ad9SJames Wright     for (CeedInt j=0; j<5; j++)
150d1b9ef12SLeila Ghaffari       q_inside[j] = q[j][i];
151d1b9ef12SLeila Ghaffari     State s_inside = StateFromU(gas, q_inside, x);
152d1b9ef12SLeila Ghaffari     const CeedScalar P = s_inside.Y.pressure;
153bb8a0c61SJames Wright 
154bb8a0c61SJames Wright     // Find inflow state using calculated P and prescribed velocity, theta0
155d1b9ef12SLeila Ghaffari     const CeedScalar e_internal = cv * s_exact.Y.temperature;
156bb8a0c61SJames Wright     const CeedScalar rho_in = P / ((gamma - 1) * e_internal);
157d1b9ef12SLeila Ghaffari     const CeedScalar E_kinetic = .5 * rho_in * Dot3(s_exact.Y.velocity,
158d1b9ef12SLeila Ghaffari                                  s_exact.Y.velocity);
159bb8a0c61SJames Wright     const CeedScalar E = rho_in * e_internal + E_kinetic;
160d1b9ef12SLeila Ghaffari 
161bb8a0c61SJames Wright     // ---- Normal vect
162bb8a0c61SJames Wright     const CeedScalar norm[3] = {q_data_sur[1][i],
163bb8a0c61SJames Wright                                 q_data_sur[2][i],
164bb8a0c61SJames Wright                                 q_data_sur[3][i]
165bb8a0c61SJames Wright                                };
166bb8a0c61SJames Wright     // The Physics
167bb8a0c61SJames Wright     // Zero v so all future terms can safely sum into it
168493642f1SJames Wright     for (CeedInt j=0; j<5; j++) v[j][i] = 0.;
169bb8a0c61SJames Wright 
170d1b9ef12SLeila Ghaffari     const CeedScalar u_normal = Dot3(norm, s_exact.Y.velocity);
171bb8a0c61SJames Wright 
172bb8a0c61SJames Wright     // The Physics
173bb8a0c61SJames Wright     // -- Density
174bb8a0c61SJames Wright     v[0][i] -= wdetJb * rho_in * u_normal;
175bb8a0c61SJames Wright 
176bb8a0c61SJames Wright     // -- Momentum
177493642f1SJames Wright     for (CeedInt j=0; j<3; j++)
178d1b9ef12SLeila Ghaffari       v[j+1][i] -= wdetJb * (rho_in * u_normal * s_exact.Y.velocity[j] +
179bb8a0c61SJames Wright                              norm[j] * P);
180bb8a0c61SJames Wright 
181bb8a0c61SJames Wright     // -- Total Energy Density
182bb8a0c61SJames Wright     v[4][i] -= wdetJb * u_normal * (E + P);
183bb8a0c61SJames Wright 
184bb8a0c61SJames Wright   } // End Quadrature Point Loop
185bb8a0c61SJames Wright   return 0;
186bb8a0c61SJames Wright }
187bb8a0c61SJames Wright 
188bb8a0c61SJames Wright // *****************************************************************************
189d1b9ef12SLeila Ghaffari // This QFunction set the outflow boundary condition for conservative variables
190d1b9ef12SLeila Ghaffari // *****************************************************************************
191bb8a0c61SJames Wright CEED_QFUNCTION(Channel_Outflow)(void *ctx, CeedInt Q,
192bb8a0c61SJames Wright                                 const CeedScalar *const *in,
193bb8a0c61SJames Wright                                 CeedScalar *const *out) {
194bb8a0c61SJames Wright   // *INDENT-OFF*
195bb8a0c61SJames Wright   // Inputs
196bb8a0c61SJames Wright   const CeedScalar (*q)[CEED_Q_VLA]          = (const CeedScalar(*)[CEED_Q_VLA])in[0],
197dd64951cSJames Wright                    (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2];
198dd64951cSJames Wright 
199bb8a0c61SJames Wright   // Outputs
200bb8a0c61SJames Wright   CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0];
201bb8a0c61SJames Wright   // *INDENT-ON*
202bb8a0c61SJames Wright 
203bb8a0c61SJames Wright   const ChannelContext context = (ChannelContext)ctx;
204bb8a0c61SJames Wright   const bool implicit     = context->implicit;
205bb8a0c61SJames Wright   const CeedScalar P0     = context->P0;
206bb8a0c61SJames Wright 
207bb8a0c61SJames Wright   CeedPragmaSIMD
208bb8a0c61SJames Wright   // Quadrature Point Loop
209bb8a0c61SJames Wright   for (CeedInt i=0; i<Q; i++) {
210bb8a0c61SJames Wright     // Setup
211bb8a0c61SJames Wright     // -- Interp in
212bb8a0c61SJames Wright     const CeedScalar rho      =  q[0][i];
213bb8a0c61SJames Wright     const CeedScalar u[3]     = {q[1][i] / rho,
214bb8a0c61SJames Wright                                  q[2][i] / rho,
215bb8a0c61SJames Wright                                  q[3][i] / rho
216bb8a0c61SJames Wright                                 };
217bb8a0c61SJames Wright     const CeedScalar E        =  q[4][i];
218bb8a0c61SJames Wright 
219bb8a0c61SJames Wright     // -- Interp-to-Interp q_data
220bb8a0c61SJames Wright     // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q).
221bb8a0c61SJames Wright     // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q).
222bb8a0c61SJames Wright     // We can effect this by swapping the sign on this weight
223bb8a0c61SJames Wright     const CeedScalar wdetJb  = (implicit ? -1. : 1.) * q_data_sur[0][i];
224bb8a0c61SJames Wright 
225bb8a0c61SJames Wright     // ---- Normal vect
226bb8a0c61SJames Wright     const CeedScalar norm[3] = {q_data_sur[1][i],
227bb8a0c61SJames Wright                                 q_data_sur[2][i],
228bb8a0c61SJames Wright                                 q_data_sur[3][i]
229bb8a0c61SJames Wright                                };
230bb8a0c61SJames Wright     // The Physics
231bb8a0c61SJames Wright     // Zero v so all future terms can safely sum into it
232493642f1SJames Wright     for (CeedInt j=0; j<5; j++) v[j][i] = 0.;
233bb8a0c61SJames Wright 
234bb8a0c61SJames Wright     // Implementing outflow condition
235bb8a0c61SJames Wright     const CeedScalar P         = P0; // pressure
236704b8bbeSJames Wright     const CeedScalar u_normal  = Dot3(norm, u); // Normal velocity
237bb8a0c61SJames Wright     // The Physics
238bb8a0c61SJames Wright     // -- Density
239bb8a0c61SJames Wright     v[0][i] -= wdetJb * rho * u_normal;
240bb8a0c61SJames Wright 
241bb8a0c61SJames Wright     // -- Momentum
242493642f1SJames Wright     for (CeedInt j=0; j<3; j++)
243bb8a0c61SJames Wright       v[j+1][i] -= wdetJb *(rho * u_normal * u[j] + norm[j] * P);
244bb8a0c61SJames Wright 
245bb8a0c61SJames Wright     // -- Total Energy Density
246bb8a0c61SJames Wright     v[4][i] -= wdetJb * u_normal * (E + P);
247bb8a0c61SJames Wright 
248bb8a0c61SJames Wright   } // End Quadrature Point Loop
249bb8a0c61SJames Wright   return 0;
250bb8a0c61SJames Wright }
251cbe60e31SLeila Ghaffari 
252cbe60e31SLeila Ghaffari // *****************************************************************************
253bb8a0c61SJames Wright #endif // channel_h
254