xref: /honee/qfunctions/channel.h (revision 3d65b166467e11bf054ebd404213121dbd593270)
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 channel_h
12bb8a0c61SJames Wright #define channel_h
13bb8a0c61SJames Wright 
14d0cce58aSJeremy L Thompson #include <ceed.h>
15bb8a0c61SJames Wright #include <math.h>
162b916ea7SJeremy L Thompson 
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 
332b916ea7SJeremy L Thompson CEED_QFUNCTION_HELPER State Exact_Channel(CeedInt dim, CeedScalar time, const CeedScalar X[], CeedInt Nf, void *ctx) {
34bb8a0c61SJames Wright   const ChannelContext     context = (ChannelContext)ctx;
35bb8a0c61SJames Wright   const CeedScalar         theta0  = context->theta0;
36bb8a0c61SJames Wright   const CeedScalar         P0      = context->P0;
37bb8a0c61SJames Wright   const CeedScalar         umax    = context->umax;
38bb8a0c61SJames Wright   const CeedScalar         center  = context->center;
39bb8a0c61SJames Wright   const CeedScalar         H       = context->H;
40cbe60e31SLeila Ghaffari   NewtonianIdealGasContext gas     = &context->newtonian_ctx;
41cbe60e31SLeila Ghaffari   const CeedScalar         cp      = gas->cp;
42cbe60e31SLeila Ghaffari   const CeedScalar         mu      = gas->mu;
43cbe60e31SLeila Ghaffari   const CeedScalar         k       = gas->k;
44cbe60e31SLeila Ghaffari   // There is a gravity body force but it is excluded from
45cbe60e31SLeila Ghaffari   //   the potential energy due to periodicity.
46d1b9ef12SLeila Ghaffari   //     g = (g, 0, 0)
47d1b9ef12SLeila Ghaffari   //     x = (0, x_2, x_3)
48d1b9ef12SLeila Ghaffari   //     e_potential = dot(g, x) = 0
49d1b9ef12SLeila Ghaffari   const CeedScalar x[3] = {0, X[1], X[2]};
50bb8a0c61SJames Wright 
51bb8a0c61SJames Wright   const CeedScalar Pr    = mu / (cp * k);
52bb8a0c61SJames Wright   const CeedScalar Ec    = (umax * umax) / (cp * theta0);
532b916ea7SJeremy L Thompson   const CeedScalar theta = theta0 * (1 + (Pr * Ec / 3) * (1 - Square(Square((x[1] - center) / H))));
54cbe60e31SLeila Ghaffari   CeedScalar       Y[5]  = {0.};
55cbe60e31SLeila Ghaffari   Y[0]                   = P0;
56d1b9ef12SLeila Ghaffari   Y[1]                   = umax * (1 - Square((x[1] - center) / H));
57cbe60e31SLeila Ghaffari   Y[2]                   = 0.;
58cbe60e31SLeila Ghaffari   Y[3]                   = 0.;
59cbe60e31SLeila Ghaffari   Y[4]                   = theta;
60bb8a0c61SJames Wright 
61d1b9ef12SLeila Ghaffari   return StateFromY(gas, Y, x);
62bb8a0c61SJames Wright }
63bb8a0c61SJames Wright 
64bb8a0c61SJames Wright // *****************************************************************************
65cbe60e31SLeila Ghaffari // This QFunction set the initial condition
66bb8a0c61SJames Wright // *****************************************************************************
672b916ea7SJeremy L Thompson CEED_QFUNCTION(ICsChannel)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) {
68bb8a0c61SJames Wright   // Inputs
69bb8a0c61SJames Wright   const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0];
70bb8a0c61SJames Wright 
71bb8a0c61SJames Wright   // Outputs
72bb8a0c61SJames Wright   CeedScalar(*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0];
73bb8a0c61SJames Wright 
74cbe60e31SLeila Ghaffari   // Context
75cbe60e31SLeila Ghaffari   const ChannelContext context = (ChannelContext)ctx;
76cbe60e31SLeila Ghaffari 
77bb8a0c61SJames Wright   // Quadrature Point Loop
782b916ea7SJeremy L Thompson   CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) {
79bb8a0c61SJames Wright     const CeedScalar x[]  = {X[0][i], X[1][i], X[2][i]};
80cbe60e31SLeila Ghaffari     State            s    = Exact_Channel(3, 0., x, 5, ctx);
81d1b9ef12SLeila Ghaffari     CeedScalar       q[5] = {0};
823636f6a4SJames Wright     switch (context->newtonian_ctx.state_var) {
833636f6a4SJames Wright       case STATEVAR_CONSERVATIVE:
84d1b9ef12SLeila Ghaffari         UnpackState_U(s.U, q);
853636f6a4SJames Wright         break;
863636f6a4SJames Wright       case STATEVAR_PRIMITIVE:
873636f6a4SJames Wright         UnpackState_Y(s.Y, q);
883636f6a4SJames Wright         break;
893636f6a4SJames Wright     }
90d1b9ef12SLeila Ghaffari 
912b916ea7SJeremy L Thompson     for (CeedInt j = 0; j < 5; j++) q0[j][i] = q[j];
92bb8a0c61SJames Wright 
93bb8a0c61SJames Wright   }  // End of Quadrature Point Loop
94bb8a0c61SJames Wright   return 0;
95bb8a0c61SJames Wright }
96bb8a0c61SJames Wright 
97bb8a0c61SJames Wright // *****************************************************************************
98d1b9ef12SLeila Ghaffari // This QFunction set the inflow boundary condition for conservative variables
99d1b9ef12SLeila Ghaffari // *****************************************************************************
1002b916ea7SJeremy L Thompson CEED_QFUNCTION(Channel_Inflow)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) {
101bb8a0c61SJames Wright   // Inputs
102*3d65b166SJames Wright   const CeedScalar(*q)[CEED_Q_VLA]          = (const CeedScalar(*)[CEED_Q_VLA])in[0];
103*3d65b166SJames Wright   const CeedScalar(*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2];
104*3d65b166SJames Wright   const CeedScalar(*X)[CEED_Q_VLA]          = (const CeedScalar(*)[CEED_Q_VLA])in[3];
105bb8a0c61SJames Wright 
106bb8a0c61SJames Wright   // Outputs
107bb8a0c61SJames Wright   CeedScalar(*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0];
108*3d65b166SJames Wright 
109bb8a0c61SJames Wright   const ChannelContext     context  = (ChannelContext)ctx;
110bb8a0c61SJames Wright   const bool               implicit = context->implicit;
111d1b9ef12SLeila Ghaffari   NewtonianIdealGasContext gas      = &context->newtonian_ctx;
112d1b9ef12SLeila Ghaffari   const CeedScalar         cv       = gas->cv;
113*3d65b166SJames Wright   const CeedScalar         gamma    = HeatCapacityRatio(&context->newtonian_ctx);
114bb8a0c61SJames Wright 
115bb8a0c61SJames Wright   // Quadrature Point Loop
116*3d65b166SJames Wright   CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) {
117bb8a0c61SJames Wright     // Setup
118bb8a0c61SJames Wright     // -- Interp-to-Interp q_data
119bb8a0c61SJames Wright     // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q).
120bb8a0c61SJames Wright     // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q).
121bb8a0c61SJames Wright     // We can effect this by swapping the sign on this weight
122bb8a0c61SJames Wright     const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i];
123bb8a0c61SJames Wright 
124d1b9ef12SLeila Ghaffari     // There is a gravity body force but it is excluded from
125d1b9ef12SLeila Ghaffari     //   the potential energy due to periodicity.
126d1b9ef12SLeila Ghaffari     //     g = (g, 0, 0)
127d1b9ef12SLeila Ghaffari     //     x = (0, x_2, x_3)
128d1b9ef12SLeila Ghaffari     //     e_potential = dot(g, x) = 0
129d1b9ef12SLeila Ghaffari     const CeedScalar x[3] = {0, X[1][i], X[2][i]};
130d1b9ef12SLeila Ghaffari 
131bb8a0c61SJames Wright     // Calcualte prescribed inflow values
132d1b9ef12SLeila Ghaffari     State      s_exact    = Exact_Channel(3, 0., x, 5, ctx);
133bb8a0c61SJames Wright     CeedScalar q_exact[5] = {0.};
134d1b9ef12SLeila Ghaffari     UnpackState_U(s_exact.U, q_exact);
135bb8a0c61SJames Wright 
136bb8a0c61SJames Wright     // Find pressure using state inside the domain
137d1b9ef12SLeila Ghaffari     CeedScalar q_inside[5] = {0};
1382b916ea7SJeremy L Thompson     for (CeedInt j = 0; j < 5; j++) q_inside[j] = q[j][i];
139d1b9ef12SLeila Ghaffari     State            s_inside = StateFromU(gas, q_inside, x);
140d1b9ef12SLeila Ghaffari     const CeedScalar P        = s_inside.Y.pressure;
141bb8a0c61SJames Wright 
142bb8a0c61SJames Wright     // Find inflow state using calculated P and prescribed velocity, theta0
143d1b9ef12SLeila Ghaffari     const CeedScalar e_internal = cv * s_exact.Y.temperature;
144bb8a0c61SJames Wright     const CeedScalar rho_in     = P / ((gamma - 1) * e_internal);
1452b916ea7SJeremy L Thompson     const CeedScalar E_kinetic  = .5 * rho_in * Dot3(s_exact.Y.velocity, s_exact.Y.velocity);
146bb8a0c61SJames Wright     const CeedScalar E          = rho_in * e_internal + E_kinetic;
147d1b9ef12SLeila Ghaffari 
148bb8a0c61SJames Wright     // ---- Normal vect
1492b916ea7SJeremy L Thompson     const CeedScalar norm[3] = {q_data_sur[1][i], q_data_sur[2][i], q_data_sur[3][i]};
150bb8a0c61SJames Wright     // The Physics
151bb8a0c61SJames Wright     // Zero v so all future terms can safely sum into it
152493642f1SJames Wright     for (CeedInt j = 0; j < 5; j++) v[j][i] = 0.;
153bb8a0c61SJames Wright 
154d1b9ef12SLeila Ghaffari     const CeedScalar u_normal = Dot3(norm, s_exact.Y.velocity);
155bb8a0c61SJames Wright 
156bb8a0c61SJames Wright     // The Physics
157bb8a0c61SJames Wright     // -- Density
158bb8a0c61SJames Wright     v[0][i] -= wdetJb * rho_in * u_normal;
159bb8a0c61SJames Wright 
160bb8a0c61SJames Wright     // -- Momentum
1612b916ea7SJeremy L Thompson     for (CeedInt j = 0; j < 3; j++) v[j + 1][i] -= wdetJb * (rho_in * u_normal * s_exact.Y.velocity[j] + norm[j] * P);
162bb8a0c61SJames Wright 
163bb8a0c61SJames Wright     // -- Total Energy Density
164bb8a0c61SJames Wright     v[4][i] -= wdetJb * u_normal * (E + P);
165bb8a0c61SJames Wright 
166bb8a0c61SJames Wright   }  // End Quadrature Point Loop
167bb8a0c61SJames Wright   return 0;
168bb8a0c61SJames Wright }
169bb8a0c61SJames Wright 
170bb8a0c61SJames Wright // *****************************************************************************
171d1b9ef12SLeila Ghaffari // This QFunction set the outflow boundary condition for conservative variables
172d1b9ef12SLeila Ghaffari // *****************************************************************************
1732b916ea7SJeremy L Thompson CEED_QFUNCTION(Channel_Outflow)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) {
174bb8a0c61SJames Wright   // Inputs
175*3d65b166SJames Wright   const CeedScalar(*q)[CEED_Q_VLA]          = (const CeedScalar(*)[CEED_Q_VLA])in[0];
176*3d65b166SJames Wright   const CeedScalar(*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2];
177dd64951cSJames Wright 
178bb8a0c61SJames Wright   // Outputs
179bb8a0c61SJames Wright   CeedScalar(*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0];
180bb8a0c61SJames Wright 
181bb8a0c61SJames Wright   const ChannelContext context  = (ChannelContext)ctx;
182bb8a0c61SJames Wright   const bool           implicit = context->implicit;
183bb8a0c61SJames Wright   const CeedScalar     P0       = context->P0;
184bb8a0c61SJames Wright 
185bb8a0c61SJames Wright   // Quadrature Point Loop
186*3d65b166SJames Wright   CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) {
187bb8a0c61SJames Wright     // Setup
188bb8a0c61SJames Wright     // -- Interp in
189bb8a0c61SJames Wright     const CeedScalar rho  = q[0][i];
1902b916ea7SJeremy L Thompson     const CeedScalar u[3] = {q[1][i] / rho, q[2][i] / rho, q[3][i] / rho};
191bb8a0c61SJames Wright     const CeedScalar E    = q[4][i];
192bb8a0c61SJames Wright 
193bb8a0c61SJames Wright     // -- Interp-to-Interp q_data
194bb8a0c61SJames Wright     // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q).
195bb8a0c61SJames Wright     // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q).
196bb8a0c61SJames Wright     // We can effect this by swapping the sign on this weight
197bb8a0c61SJames Wright     const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i];
198bb8a0c61SJames Wright 
199bb8a0c61SJames Wright     // ---- Normal vect
2002b916ea7SJeremy L Thompson     const CeedScalar norm[3] = {q_data_sur[1][i], q_data_sur[2][i], q_data_sur[3][i]};
201bb8a0c61SJames Wright     // The Physics
202bb8a0c61SJames Wright     // Zero v so all future terms can safely sum into it
203493642f1SJames Wright     for (CeedInt j = 0; j < 5; j++) v[j][i] = 0.;
204bb8a0c61SJames Wright 
205bb8a0c61SJames Wright     // Implementing outflow condition
206bb8a0c61SJames Wright     const CeedScalar P        = P0;             // pressure
207704b8bbeSJames Wright     const CeedScalar u_normal = Dot3(norm, u);  // Normal velocity
208bb8a0c61SJames Wright     // The Physics
209bb8a0c61SJames Wright     // -- Density
210bb8a0c61SJames Wright     v[0][i] -= wdetJb * rho * u_normal;
211bb8a0c61SJames Wright 
212bb8a0c61SJames Wright     // -- Momentum
2132b916ea7SJeremy L Thompson     for (CeedInt j = 0; j < 3; j++) v[j + 1][i] -= wdetJb * (rho * u_normal * u[j] + norm[j] * P);
214bb8a0c61SJames Wright 
215bb8a0c61SJames Wright     // -- Total Energy Density
216bb8a0c61SJames Wright     v[4][i] -= wdetJb * u_normal * (E + P);
217bb8a0c61SJames Wright 
218bb8a0c61SJames Wright   }  // End Quadrature Point Loop
219bb8a0c61SJames Wright   return 0;
220bb8a0c61SJames Wright }
221cbe60e31SLeila Ghaffari 
222cbe60e31SLeila Ghaffari // *****************************************************************************
223bb8a0c61SJames Wright #endif  // channel_h
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