xref: /honee/qfunctions/channel.h (revision d1b9ef12923730ac357e6e30d052a0445e411f3e)
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"
18cbe60e31SLeila 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 
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.
48*d1b9ef12SLeila Ghaffari   //     g = (g, 0, 0)
49*d1b9ef12SLeila Ghaffari   //     x = (0, x_2, x_3)
50*d1b9ef12SLeila Ghaffari   //     e_potential = dot(g, x) = 0
51*d1b9ef12SLeila 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)
56*d1b9ef12SLeila Ghaffari                                    * (1 - Square(Square((x[1]-center)/H))));
57cbe60e31SLeila Ghaffari   CeedScalar Y[5] = {0.};
58cbe60e31SLeila Ghaffari   Y[0] = P0;
59*d1b9ef12SLeila 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 
64*d1b9ef12SLeila 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);
86*d1b9ef12SLeila Ghaffari     CeedScalar q[5] = {0};
87*d1b9ef12SLeila Ghaffari     if (context->newtonian_ctx.is_primitive)
88*d1b9ef12SLeila Ghaffari       UnpackState_Y(s.Y, q);
89*d1b9ef12SLeila Ghaffari     else
90*d1b9ef12SLeila Ghaffari       UnpackState_U(s.U, q);
91*d1b9ef12SLeila Ghaffari 
92*d1b9ef12SLeila Ghaffari     for (CeedInt j=0; j<5; j++)
93*d1b9ef12SLeila Ghaffari       q0[j][i] = q[j];
94bb8a0c61SJames Wright 
95bb8a0c61SJames Wright   } // End of Quadrature Point Loop
96bb8a0c61SJames Wright   return 0;
97bb8a0c61SJames Wright }
98bb8a0c61SJames Wright 
99bb8a0c61SJames Wright // *****************************************************************************
100*d1b9ef12SLeila Ghaffari // This QFunction set the inflow boundary condition for conservative variables
101*d1b9ef12SLeila Ghaffari // *****************************************************************************
102bb8a0c61SJames Wright CEED_QFUNCTION(Channel_Inflow)(void *ctx, CeedInt Q,
103bb8a0c61SJames Wright                                const CeedScalar *const *in,
104bb8a0c61SJames Wright                                CeedScalar *const *out) {
105bb8a0c61SJames Wright   // *INDENT-OFF*
106bb8a0c61SJames Wright   // Inputs
107bb8a0c61SJames Wright   const CeedScalar (*q)[CEED_Q_VLA]          = (const CeedScalar(*)[CEED_Q_VLA])in[0],
108dd64951cSJames Wright                    (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2],
109dd64951cSJames Wright                    (*X)[CEED_Q_VLA]          = (const CeedScalar(*)[CEED_Q_VLA])in[3];
110bb8a0c61SJames Wright 
111bb8a0c61SJames Wright   // Outputs
112bb8a0c61SJames Wright   CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0];
113bb8a0c61SJames Wright   // *INDENT-ON*
114bb8a0c61SJames Wright   const ChannelContext context = (ChannelContext)ctx;
115bb8a0c61SJames Wright   const bool implicit          = context->implicit;
116*d1b9ef12SLeila Ghaffari   NewtonianIdealGasContext gas = &context->newtonian_ctx;
117*d1b9ef12SLeila Ghaffari   const CeedScalar cv          = gas->cv;
118*d1b9ef12SLeila Ghaffari   const CeedScalar cp          = gas->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 
131*d1b9ef12SLeila Ghaffari     // There is a gravity body force but it is excluded from
132*d1b9ef12SLeila Ghaffari     //   the potential energy due to periodicity.
133*d1b9ef12SLeila Ghaffari     //     g = (g, 0, 0)
134*d1b9ef12SLeila Ghaffari     //     x = (0, x_2, x_3)
135*d1b9ef12SLeila Ghaffari     //     e_potential = dot(g, x) = 0
136*d1b9ef12SLeila Ghaffari     const CeedScalar x[3] = {0, X[1][i], X[2][i]};
137*d1b9ef12SLeila Ghaffari 
138bb8a0c61SJames Wright     // Calcualte prescribed inflow values
139*d1b9ef12SLeila Ghaffari     State s_exact = Exact_Channel(3, 0., x, 5, ctx);
140bb8a0c61SJames Wright     CeedScalar q_exact[5] = {0.};
141*d1b9ef12SLeila Ghaffari     UnpackState_U(s_exact.U, q_exact);
142bb8a0c61SJames Wright 
143bb8a0c61SJames Wright     // Find pressure using state inside the domain
144*d1b9ef12SLeila Ghaffari     CeedScalar q_inside[5] = {0};
145*d1b9ef12SLeila Ghaffari     for (CeedInt j; j<5; j++)
146*d1b9ef12SLeila Ghaffari       q_inside[j] = q[j][i];
147*d1b9ef12SLeila Ghaffari     State s_inside = StateFromU(gas, q_inside, x);
148*d1b9ef12SLeila Ghaffari     const CeedScalar P = s_inside.Y.pressure;
149bb8a0c61SJames Wright 
150bb8a0c61SJames Wright     // Find inflow state using calculated P and prescribed velocity, theta0
151*d1b9ef12SLeila Ghaffari     const CeedScalar e_internal = cv * s_exact.Y.temperature;
152bb8a0c61SJames Wright     const CeedScalar rho_in = P / ((gamma - 1) * e_internal);
153*d1b9ef12SLeila Ghaffari     const CeedScalar E_kinetic = .5 * rho_in * Dot3(s_exact.Y.velocity,
154*d1b9ef12SLeila Ghaffari                                  s_exact.Y.velocity);
155bb8a0c61SJames Wright     const CeedScalar E = rho_in * e_internal + E_kinetic;
156*d1b9ef12SLeila Ghaffari 
157bb8a0c61SJames Wright     // ---- Normal vect
158bb8a0c61SJames Wright     const CeedScalar norm[3] = {q_data_sur[1][i],
159bb8a0c61SJames Wright                                 q_data_sur[2][i],
160bb8a0c61SJames Wright                                 q_data_sur[3][i]
161bb8a0c61SJames Wright                                };
162bb8a0c61SJames Wright     // The Physics
163bb8a0c61SJames Wright     // Zero v so all future terms can safely sum into it
164493642f1SJames Wright     for (CeedInt j=0; j<5; j++) v[j][i] = 0.;
165bb8a0c61SJames Wright 
166*d1b9ef12SLeila Ghaffari     const CeedScalar u_normal = Dot3(norm, s_exact.Y.velocity);
167bb8a0c61SJames Wright 
168bb8a0c61SJames Wright     // The Physics
169bb8a0c61SJames Wright     // -- Density
170bb8a0c61SJames Wright     v[0][i] -= wdetJb * rho_in * u_normal;
171bb8a0c61SJames Wright 
172bb8a0c61SJames Wright     // -- Momentum
173493642f1SJames Wright     for (CeedInt j=0; j<3; j++)
174*d1b9ef12SLeila Ghaffari       v[j+1][i] -= wdetJb * (rho_in * u_normal * s_exact.Y.velocity[j] +
175bb8a0c61SJames Wright                              norm[j] * P);
176bb8a0c61SJames Wright 
177bb8a0c61SJames Wright     // -- Total Energy Density
178bb8a0c61SJames Wright     v[4][i] -= wdetJb * u_normal * (E + P);
179bb8a0c61SJames Wright 
180bb8a0c61SJames Wright   } // End Quadrature Point Loop
181bb8a0c61SJames Wright   return 0;
182bb8a0c61SJames Wright }
183bb8a0c61SJames Wright 
184bb8a0c61SJames Wright // *****************************************************************************
185*d1b9ef12SLeila Ghaffari // This QFunction set the outflow boundary condition for conservative variables
186*d1b9ef12SLeila Ghaffari // *****************************************************************************
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     // The Physics
227bb8a0c61SJames Wright     // Zero v so all future terms can safely sum into it
228493642f1SJames Wright     for (CeedInt j=0; j<5; j++) v[j][i] = 0.;
229bb8a0c61SJames Wright 
230bb8a0c61SJames Wright     // Implementing outflow condition
231bb8a0c61SJames Wright     const CeedScalar P         = P0; // pressure
232704b8bbeSJames Wright     const CeedScalar u_normal  = Dot3(norm, u); // Normal velocity
233bb8a0c61SJames Wright     // The Physics
234bb8a0c61SJames Wright     // -- Density
235bb8a0c61SJames Wright     v[0][i] -= wdetJb * rho * u_normal;
236bb8a0c61SJames Wright 
237bb8a0c61SJames Wright     // -- Momentum
238493642f1SJames Wright     for (CeedInt j=0; j<3; j++)
239bb8a0c61SJames Wright       v[j+1][i] -= wdetJb *(rho * u_normal * u[j] + norm[j] * P);
240bb8a0c61SJames Wright 
241bb8a0c61SJames Wright     // -- Total Energy Density
242bb8a0c61SJames Wright     v[4][i] -= wdetJb * u_normal * (E + P);
243bb8a0c61SJames Wright 
244bb8a0c61SJames Wright   } // End Quadrature Point Loop
245bb8a0c61SJames Wright   return 0;
246bb8a0c61SJames Wright }
247cbe60e31SLeila Ghaffari 
248cbe60e31SLeila Ghaffari // *****************************************************************************
249bb8a0c61SJames Wright #endif // channel_h
250