xref: /honee/qfunctions/channel.h (revision cbe60e318f71d8fedc7dbd515907b9b7df1392f5)
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 
15bb8a0c61SJames Wright #include <math.h>
16c58dce4fSJed Brown #include <ceed/ceed.h>
1715a3537eSJed Brown #include "newtonian_types.h"
18*cbe60e31SLeila Ghaffari #include "newtonian_state.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 
33*cbe60e31SLeila Ghaffari CEED_QFUNCTION_HELPER State Exact_Channel(CeedInt dim, CeedScalar time,
34*cbe60e31SLeila 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;
42*cbe60e31SLeila Ghaffari   NewtonianIdealGasContext gas = &context->newtonian_ctx;
43*cbe60e31SLeila Ghaffari   const CeedScalar cp          = gas->cp;
44*cbe60e31SLeila Ghaffari   const CeedScalar mu          = gas->mu;
45*cbe60e31SLeila Ghaffari   const CeedScalar k           = gas->k;
46*cbe60e31SLeila Ghaffari   // There is a gravity body force but it is excluded from
47*cbe60e31SLeila Ghaffari   //   the potential energy due to periodicity.
48*cbe60e31SLeila Ghaffari   gas->g[0] = 0.;
49*cbe60e31SLeila Ghaffari   gas->g[1] = 0.;
50*cbe60e31SLeila Ghaffari   gas->g[2] = 0.;
51bb8a0c61SJames Wright 
52bb8a0c61SJames Wright   const CeedScalar y     = X[1];
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)
56c58dce4fSJed Brown                                    * (1 - Square(Square((y-center)/H))));
57*cbe60e31SLeila Ghaffari   CeedScalar Y[5] = {0.};
58*cbe60e31SLeila Ghaffari   Y[0] = P0;
59*cbe60e31SLeila Ghaffari   Y[1] = umax*(1 - Square((y-center)/H));
60*cbe60e31SLeila Ghaffari   Y[2] = 0.;
61*cbe60e31SLeila Ghaffari   Y[3] = 0.;
62*cbe60e31SLeila Ghaffari   Y[4] = theta;
63bb8a0c61SJames Wright 
64*cbe60e31SLeila Ghaffari   return StateFromY(gas, Y, X);
65bb8a0c61SJames Wright }
66bb8a0c61SJames Wright 
67bb8a0c61SJames Wright // *****************************************************************************
68*cbe60e31SLeila 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 
78*cbe60e31SLeila Ghaffari   // Context
79*cbe60e31SLeila Ghaffari   const ChannelContext context = (ChannelContext)ctx;
80*cbe60e31SLeila 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]};
85*cbe60e31SLeila Ghaffari     State s = Exact_Channel(3, 0., x, 5, ctx);
86*cbe60e31SLeila Ghaffari     if (context->newtonian_ctx.primitive) {
87*cbe60e31SLeila Ghaffari       q0[0][i] = s.Y.pressure;
88*cbe60e31SLeila Ghaffari       for (CeedInt j=0; j<3; j++)
89*cbe60e31SLeila Ghaffari         q0[j+1][i] = s.Y.velocity[j];
90*cbe60e31SLeila Ghaffari       q0[4][i] = s.Y.temperature;
91*cbe60e31SLeila Ghaffari     } else {
92*cbe60e31SLeila Ghaffari       q0[0][i] = s.U.density;
93*cbe60e31SLeila Ghaffari       for (CeedInt j=0; j<3; j++)
94*cbe60e31SLeila Ghaffari         q0[j+1][i] = s.U.momentum[j];
95*cbe60e31SLeila Ghaffari       q0[4][i] = s.U.E_total;
96*cbe60e31SLeila Ghaffari     }
97bb8a0c61SJames Wright 
98bb8a0c61SJames Wright   } // End of Quadrature Point Loop
99bb8a0c61SJames Wright   return 0;
100bb8a0c61SJames Wright }
101bb8a0c61SJames Wright 
102bb8a0c61SJames Wright // *****************************************************************************
103bb8a0c61SJames Wright CEED_QFUNCTION(Channel_Inflow)(void *ctx, CeedInt Q,
104bb8a0c61SJames Wright                                const CeedScalar *const *in,
105bb8a0c61SJames Wright                                CeedScalar *const *out) {
106bb8a0c61SJames Wright   // *INDENT-OFF*
107bb8a0c61SJames Wright   // Inputs
108bb8a0c61SJames Wright   const CeedScalar (*q)[CEED_Q_VLA]          = (const CeedScalar(*)[CEED_Q_VLA])in[0],
109dd64951cSJames Wright                    (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2],
110dd64951cSJames Wright                    (*X)[CEED_Q_VLA]          = (const CeedScalar(*)[CEED_Q_VLA])in[3];
111bb8a0c61SJames Wright 
112bb8a0c61SJames Wright   // Outputs
113bb8a0c61SJames Wright   CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0];
114bb8a0c61SJames Wright   // *INDENT-ON*
115bb8a0c61SJames Wright   const ChannelContext context = (ChannelContext)ctx;
116bb8a0c61SJames Wright   const bool implicit     = context->implicit;
117bb8a0c61SJames Wright   const CeedScalar cv     = context->newtonian_ctx.cv;
118bb8a0c61SJames Wright   const CeedScalar cp     = context->newtonian_ctx.cp;
119bb8a0c61SJames Wright   const CeedScalar gamma  = cp/cv;
120bb8a0c61SJames Wright 
121bb8a0c61SJames Wright   CeedPragmaSIMD
122bb8a0c61SJames Wright   // Quadrature Point Loop
123bb8a0c61SJames Wright   for (CeedInt i=0; i<Q; i++) {
124bb8a0c61SJames Wright     // Setup
125bb8a0c61SJames Wright     // -- Interp-to-Interp q_data
126bb8a0c61SJames Wright     // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q).
127bb8a0c61SJames Wright     // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q).
128bb8a0c61SJames Wright     // We can effect this by swapping the sign on this weight
129bb8a0c61SJames Wright     const CeedScalar wdetJb  = (implicit ? -1. : 1.) * q_data_sur[0][i];
130bb8a0c61SJames Wright 
131bb8a0c61SJames Wright     // Calcualte prescribed inflow values
132bb8a0c61SJames Wright     const CeedScalar x[3] = {X[0][i], X[1][i], X[2][i]};
133*cbe60e31SLeila Ghaffari     State s = Exact_Channel(3, 0., x, 5, ctx);
134bb8a0c61SJames Wright     CeedScalar q_exact[5] = {0.};
135*cbe60e31SLeila Ghaffari     q_exact[0] = s.U.density;
136*cbe60e31SLeila Ghaffari     for (CeedInt j=0; j<3; j++)
137*cbe60e31SLeila Ghaffari       q_exact[j+1] = s.U.momentum[j];
138*cbe60e31SLeila Ghaffari     q_exact[4] = s.U.E_total;
139704b8bbeSJames Wright     const CeedScalar E_kinetic_exact = 0.5*Dot3(&q_exact[1], &q_exact[1])
140704b8bbeSJames Wright                                        / q_exact[0];
141bb8a0c61SJames Wright     const CeedScalar velocity[3] = {q_exact[1]/q_exact[0],
142bb8a0c61SJames Wright                                     q_exact[2]/q_exact[0],
143bb8a0c61SJames Wright                                     q_exact[3]/q_exact[0]
144bb8a0c61SJames Wright                                    };
145bb8a0c61SJames Wright     const CeedScalar theta = (q_exact[4] - E_kinetic_exact) / (q_exact[0]*cv);
146bb8a0c61SJames Wright 
147bb8a0c61SJames Wright     // Find pressure using state inside the domain
148bb8a0c61SJames Wright     const CeedScalar rho = q[0][i];
149bb8a0c61SJames Wright     const CeedScalar u[3] = {q[1][i]/rho, q[2][i]/rho, q[3][i]/rho};
150704b8bbeSJames Wright     const CeedScalar E_internal = q[4][i] - .5 * rho * Dot3(u,u);
151bb8a0c61SJames Wright     const CeedScalar P = E_internal * (gamma - 1.);
152bb8a0c61SJames Wright 
153bb8a0c61SJames Wright     // Find inflow state using calculated P and prescribed velocity, theta0
154bb8a0c61SJames Wright     const CeedScalar e_internal = cv * theta;
155bb8a0c61SJames Wright     const CeedScalar rho_in = P / ((gamma - 1) * e_internal);
156704b8bbeSJames Wright     const CeedScalar E_kinetic = .5 * rho_in * Dot3(velocity, velocity);
157bb8a0c61SJames Wright     const CeedScalar E = rho_in * e_internal + E_kinetic;
158bb8a0c61SJames Wright     // ---- Normal vect
159bb8a0c61SJames Wright     const CeedScalar norm[3] = {q_data_sur[1][i],
160bb8a0c61SJames Wright                                 q_data_sur[2][i],
161bb8a0c61SJames Wright                                 q_data_sur[3][i]
162bb8a0c61SJames Wright                                };
163bb8a0c61SJames Wright 
164bb8a0c61SJames Wright     // The Physics
165bb8a0c61SJames Wright     // Zero v so all future terms can safely sum into it
166493642f1SJames Wright     for (CeedInt j=0; j<5; j++) v[j][i] = 0.;
167bb8a0c61SJames Wright 
168704b8bbeSJames Wright     const CeedScalar u_normal = Dot3(norm, velocity);
169bb8a0c61SJames Wright 
170bb8a0c61SJames Wright     // The Physics
171bb8a0c61SJames Wright     // -- Density
172bb8a0c61SJames Wright     v[0][i] -= wdetJb * rho_in * u_normal;
173bb8a0c61SJames Wright 
174bb8a0c61SJames Wright     // -- Momentum
175493642f1SJames Wright     for (CeedInt j=0; j<3; j++)
176bb8a0c61SJames Wright       v[j+1][i] -= wdetJb * (rho_in * u_normal * velocity[j] +
177bb8a0c61SJames Wright                              norm[j] * P);
178bb8a0c61SJames Wright 
179bb8a0c61SJames Wright     // -- Total Energy Density
180bb8a0c61SJames Wright     v[4][i] -= wdetJb * u_normal * (E + P);
181bb8a0c61SJames Wright 
182bb8a0c61SJames Wright   } // End Quadrature Point Loop
183bb8a0c61SJames Wright   return 0;
184bb8a0c61SJames Wright }
185bb8a0c61SJames Wright 
186bb8a0c61SJames Wright // *****************************************************************************
187bb8a0c61SJames Wright CEED_QFUNCTION(Channel_Outflow)(void *ctx, CeedInt Q,
188bb8a0c61SJames Wright                                 const CeedScalar *const *in,
189bb8a0c61SJames Wright                                 CeedScalar *const *out) {
190bb8a0c61SJames Wright   // *INDENT-OFF*
191bb8a0c61SJames Wright   // Inputs
192bb8a0c61SJames Wright   const CeedScalar (*q)[CEED_Q_VLA]          = (const CeedScalar(*)[CEED_Q_VLA])in[0],
193dd64951cSJames Wright                    (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2];
194dd64951cSJames Wright 
195bb8a0c61SJames Wright   // Outputs
196bb8a0c61SJames Wright   CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0];
197bb8a0c61SJames Wright   // *INDENT-ON*
198bb8a0c61SJames Wright 
199bb8a0c61SJames Wright   const ChannelContext context = (ChannelContext)ctx;
200bb8a0c61SJames Wright   const bool implicit     = context->implicit;
201bb8a0c61SJames Wright   const CeedScalar P0     = context->P0;
202bb8a0c61SJames Wright 
203bb8a0c61SJames Wright   CeedPragmaSIMD
204bb8a0c61SJames Wright   // Quadrature Point Loop
205bb8a0c61SJames Wright   for (CeedInt i=0; i<Q; i++) {
206bb8a0c61SJames Wright     // Setup
207bb8a0c61SJames Wright     // -- Interp in
208bb8a0c61SJames Wright     const CeedScalar rho      =  q[0][i];
209bb8a0c61SJames Wright     const CeedScalar u[3]     = {q[1][i] / rho,
210bb8a0c61SJames Wright                                  q[2][i] / rho,
211bb8a0c61SJames Wright                                  q[3][i] / rho
212bb8a0c61SJames Wright                                 };
213bb8a0c61SJames Wright     const CeedScalar E        =  q[4][i];
214bb8a0c61SJames Wright 
215bb8a0c61SJames Wright     // -- Interp-to-Interp q_data
216bb8a0c61SJames Wright     // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q).
217bb8a0c61SJames Wright     // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q).
218bb8a0c61SJames Wright     // We can effect this by swapping the sign on this weight
219bb8a0c61SJames Wright     const CeedScalar wdetJb  = (implicit ? -1. : 1.) * q_data_sur[0][i];
220bb8a0c61SJames Wright 
221bb8a0c61SJames Wright     // ---- Normal vect
222bb8a0c61SJames Wright     const CeedScalar norm[3] = {q_data_sur[1][i],
223bb8a0c61SJames Wright                                 q_data_sur[2][i],
224bb8a0c61SJames Wright                                 q_data_sur[3][i]
225bb8a0c61SJames Wright                                };
226bb8a0c61SJames Wright 
227bb8a0c61SJames Wright     // The Physics
228bb8a0c61SJames Wright     // Zero v so all future terms can safely sum into it
229493642f1SJames Wright     for (CeedInt j=0; j<5; j++) v[j][i] = 0.;
230bb8a0c61SJames Wright 
231bb8a0c61SJames Wright     // Implementing outflow condition
232bb8a0c61SJames Wright     const CeedScalar P         = P0; // pressure
233704b8bbeSJames Wright     const CeedScalar u_normal  = Dot3(norm, u); // Normal velocity
234bb8a0c61SJames Wright     // The Physics
235bb8a0c61SJames Wright     // -- Density
236bb8a0c61SJames Wright     v[0][i] -= wdetJb * rho * u_normal;
237bb8a0c61SJames Wright 
238bb8a0c61SJames Wright     // -- Momentum
239493642f1SJames Wright     for (CeedInt j=0; j<3; j++)
240bb8a0c61SJames Wright       v[j+1][i] -= wdetJb *(rho * u_normal * u[j] + norm[j] * P);
241bb8a0c61SJames Wright 
242bb8a0c61SJames Wright     // -- Total Energy Density
243bb8a0c61SJames Wright     v[4][i] -= wdetJb * u_normal * (E + P);
244bb8a0c61SJames Wright 
245bb8a0c61SJames Wright   } // End Quadrature Point Loop
246bb8a0c61SJames Wright   return 0;
247bb8a0c61SJames Wright }
248*cbe60e31SLeila Ghaffari 
249*cbe60e31SLeila Ghaffari // *****************************************************************************
250bb8a0c61SJames Wright #endif // channel_h
251