xref: /libCEED/examples/fluids/qfunctions/channel.h (revision c9c2c07970382857cc7b4a28d359710237b91a3e)
188626eedSJames Wright // Copyright (c) 2017-2022, Lawrence Livermore National Security, LLC and other CEED contributors.
288626eedSJames Wright // All Rights Reserved. See the top-level LICENSE and NOTICE files for details.
388626eedSJames Wright //
488626eedSJames Wright // SPDX-License-Identifier: BSD-2-Clause
588626eedSJames Wright //
688626eedSJames Wright // This file is part of CEED:  http://github.com/ceed
788626eedSJames Wright 
888626eedSJames Wright /// @file
988626eedSJames Wright /// Operator for Navier-Stokes example using PETSc
1088626eedSJames Wright 
1188626eedSJames Wright 
1288626eedSJames Wright #ifndef channel_h
1388626eedSJames Wright #define channel_h
1488626eedSJames Wright 
15*c9c2c079SJeremy L Thompson #include <ceed.h>
1688626eedSJames Wright #include <math.h>
17dc805cc4SLeila Ghaffari #include "newtonian_state.h"
18*c9c2c079SJeremy L Thompson #include "newtonian_types.h"
1913fa47b2SJames Wright #include "utils.h"
2088626eedSJames Wright 
2188626eedSJames Wright typedef struct ChannelContext_ *ChannelContext;
2288626eedSJames Wright struct ChannelContext_ {
2388626eedSJames Wright   bool       implicit; // !< Using implicit timesteping or not
2488626eedSJames Wright   CeedScalar theta0;   // !< Reference temperature
2588626eedSJames Wright   CeedScalar P0;       // !< Reference Pressure
2688626eedSJames Wright   CeedScalar umax;     // !< Centerline velocity
2788626eedSJames Wright   CeedScalar center;   // !< Y Coordinate for center of channel
2888626eedSJames Wright   CeedScalar H;        // !< Channel half-height
2988626eedSJames Wright   CeedScalar B;        // !< Body-force driving the flow
3088626eedSJames Wright   struct NewtonianIdealGasContext_ newtonian_ctx;
3188626eedSJames Wright };
3288626eedSJames Wright 
33dc805cc4SLeila Ghaffari CEED_QFUNCTION_HELPER State Exact_Channel(CeedInt dim, CeedScalar time,
34dc805cc4SLeila Ghaffari     const CeedScalar X[], CeedInt Nf, void *ctx) {
3588626eedSJames Wright 
3688626eedSJames Wright   const ChannelContext context = (ChannelContext)ctx;
3788626eedSJames Wright   const CeedScalar theta0      = context->theta0;
3888626eedSJames Wright   const CeedScalar P0          = context->P0;
3988626eedSJames Wright   const CeedScalar umax        = context->umax;
4088626eedSJames Wright   const CeedScalar center      = context->center;
4188626eedSJames Wright   const CeedScalar H           = context->H;
42dc805cc4SLeila Ghaffari   NewtonianIdealGasContext gas = &context->newtonian_ctx;
43dc805cc4SLeila Ghaffari   const CeedScalar cp          = gas->cp;
44dc805cc4SLeila Ghaffari   const CeedScalar mu          = gas->mu;
45dc805cc4SLeila Ghaffari   const CeedScalar k           = gas->k;
46dc805cc4SLeila Ghaffari   // There is a gravity body force but it is excluded from
47dc805cc4SLeila Ghaffari   //   the potential energy due to periodicity.
482b89d87eSLeila Ghaffari   //     g = (g, 0, 0)
492b89d87eSLeila Ghaffari   //     x = (0, x_2, x_3)
502b89d87eSLeila Ghaffari   //     e_potential = dot(g, x) = 0
512b89d87eSLeila Ghaffari   const CeedScalar x[3] = {0, X[1], X[2]};
5288626eedSJames Wright 
5388626eedSJames Wright   const CeedScalar Pr    = mu / (cp*k);
5488626eedSJames Wright   const CeedScalar Ec    = (umax*umax) / (cp*theta0);
55c32eb7cbSJed Brown   const CeedScalar theta = theta0*(1 + (Pr*Ec/3)
562b89d87eSLeila Ghaffari                                    * (1 - Square(Square((x[1]-center)/H))));
57dc805cc4SLeila Ghaffari   CeedScalar Y[5] = {0.};
58dc805cc4SLeila Ghaffari   Y[0] = P0;
592b89d87eSLeila Ghaffari   Y[1] = umax*(1 - Square((x[1]-center)/H));
60dc805cc4SLeila Ghaffari   Y[2] = 0.;
61dc805cc4SLeila Ghaffari   Y[3] = 0.;
62dc805cc4SLeila Ghaffari   Y[4] = theta;
6388626eedSJames Wright 
642b89d87eSLeila Ghaffari   return StateFromY(gas, Y, x);
6588626eedSJames Wright }
6688626eedSJames Wright 
6788626eedSJames Wright // *****************************************************************************
68dc805cc4SLeila Ghaffari // This QFunction set the initial condition
6988626eedSJames Wright // *****************************************************************************
7088626eedSJames Wright CEED_QFUNCTION(ICsChannel)(void *ctx, CeedInt Q,
7188626eedSJames Wright                            const CeedScalar *const *in, CeedScalar *const *out) {
7288626eedSJames Wright   // Inputs
7388626eedSJames Wright   const CeedScalar (*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0];
7488626eedSJames Wright 
7588626eedSJames Wright   // Outputs
7688626eedSJames Wright   CeedScalar (*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0];
7788626eedSJames Wright 
78dc805cc4SLeila Ghaffari   // Context
79dc805cc4SLeila Ghaffari   const ChannelContext context = (ChannelContext)ctx;
80dc805cc4SLeila Ghaffari 
8188626eedSJames Wright   // Quadrature Point Loop
8288626eedSJames Wright   CeedPragmaSIMD
8388626eedSJames Wright   for (CeedInt i=0; i<Q; i++) {
8488626eedSJames Wright     const CeedScalar x[] = {X[0][i], X[1][i], X[2][i]};
85dc805cc4SLeila Ghaffari     State s = Exact_Channel(3, 0., x, 5, ctx);
862b89d87eSLeila Ghaffari     CeedScalar q[5] = {0};
872b89d87eSLeila Ghaffari     if (context->newtonian_ctx.is_primitive)
882b89d87eSLeila Ghaffari       UnpackState_Y(s.Y, q);
892b89d87eSLeila Ghaffari     else
902b89d87eSLeila Ghaffari       UnpackState_U(s.U, q);
912b89d87eSLeila Ghaffari 
922b89d87eSLeila Ghaffari     for (CeedInt j=0; j<5; j++)
932b89d87eSLeila Ghaffari       q0[j][i] = q[j];
9488626eedSJames Wright 
9588626eedSJames Wright   } // End of Quadrature Point Loop
9688626eedSJames Wright   return 0;
9788626eedSJames Wright }
9888626eedSJames Wright 
9988626eedSJames Wright // *****************************************************************************
1002b89d87eSLeila Ghaffari // This QFunction set the inflow boundary condition for conservative variables
1012b89d87eSLeila Ghaffari // *****************************************************************************
10288626eedSJames Wright CEED_QFUNCTION(Channel_Inflow)(void *ctx, CeedInt Q,
10388626eedSJames Wright                                const CeedScalar *const *in,
10488626eedSJames Wright                                CeedScalar *const *out) {
10588626eedSJames Wright   // *INDENT-OFF*
10688626eedSJames Wright   // Inputs
10788626eedSJames Wright   const CeedScalar (*q)[CEED_Q_VLA]          = (const CeedScalar(*)[CEED_Q_VLA])in[0],
108e8b03feeSJames Wright                    (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2],
109e8b03feeSJames Wright                    (*X)[CEED_Q_VLA]          = (const CeedScalar(*)[CEED_Q_VLA])in[3];
11088626eedSJames Wright 
11188626eedSJames Wright   // Outputs
11288626eedSJames Wright   CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0];
11388626eedSJames Wright   // *INDENT-ON*
11488626eedSJames Wright   const ChannelContext context = (ChannelContext)ctx;
11588626eedSJames Wright   const bool implicit          = context->implicit;
1162b89d87eSLeila Ghaffari   NewtonianIdealGasContext gas = &context->newtonian_ctx;
1172b89d87eSLeila Ghaffari   const CeedScalar cv          = gas->cv;
1182b89d87eSLeila Ghaffari   const CeedScalar cp          = gas->cp;
11988626eedSJames Wright   const CeedScalar gamma       = cp / cv;
12088626eedSJames Wright 
12188626eedSJames Wright   CeedPragmaSIMD
12288626eedSJames Wright   // Quadrature Point Loop
12388626eedSJames Wright   for (CeedInt i=0; i<Q; i++) {
12488626eedSJames Wright     // Setup
12588626eedSJames Wright     // -- Interp-to-Interp q_data
12688626eedSJames Wright     // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q).
12788626eedSJames Wright     // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q).
12888626eedSJames Wright     // We can effect this by swapping the sign on this weight
12988626eedSJames Wright     const CeedScalar wdetJb  = (implicit ? -1. : 1.) * q_data_sur[0][i];
13088626eedSJames Wright 
1312b89d87eSLeila Ghaffari     // There is a gravity body force but it is excluded from
1322b89d87eSLeila Ghaffari     //   the potential energy due to periodicity.
1332b89d87eSLeila Ghaffari     //     g = (g, 0, 0)
1342b89d87eSLeila Ghaffari     //     x = (0, x_2, x_3)
1352b89d87eSLeila Ghaffari     //     e_potential = dot(g, x) = 0
1362b89d87eSLeila Ghaffari     const CeedScalar x[3] = {0, X[1][i], X[2][i]};
1372b89d87eSLeila Ghaffari 
13888626eedSJames Wright     // Calcualte prescribed inflow values
1392b89d87eSLeila Ghaffari     State s_exact = Exact_Channel(3, 0., x, 5, ctx);
14088626eedSJames Wright     CeedScalar q_exact[5] = {0.};
1412b89d87eSLeila Ghaffari     UnpackState_U(s_exact.U, q_exact);
14288626eedSJames Wright 
14388626eedSJames Wright     // Find pressure using state inside the domain
1442b89d87eSLeila Ghaffari     CeedScalar q_inside[5] = {0};
1459b7dec89SJames Wright     for (CeedInt j=0; j<5; j++)
1462b89d87eSLeila Ghaffari       q_inside[j] = q[j][i];
1472b89d87eSLeila Ghaffari     State s_inside = StateFromU(gas, q_inside, x);
1482b89d87eSLeila Ghaffari     const CeedScalar P = s_inside.Y.pressure;
14988626eedSJames Wright 
15088626eedSJames Wright     // Find inflow state using calculated P and prescribed velocity, theta0
1512b89d87eSLeila Ghaffari     const CeedScalar e_internal = cv * s_exact.Y.temperature;
15288626eedSJames Wright     const CeedScalar rho_in = P / ((gamma - 1) * e_internal);
1532b89d87eSLeila Ghaffari     const CeedScalar E_kinetic = .5 * rho_in * Dot3(s_exact.Y.velocity,
1542b89d87eSLeila Ghaffari                                  s_exact.Y.velocity);
15588626eedSJames Wright     const CeedScalar E = rho_in * e_internal + E_kinetic;
1562b89d87eSLeila Ghaffari 
15788626eedSJames Wright     // ---- Normal vect
15888626eedSJames Wright     const CeedScalar norm[3] = {q_data_sur[1][i],
15988626eedSJames Wright                                 q_data_sur[2][i],
16088626eedSJames Wright                                 q_data_sur[3][i]
16188626eedSJames Wright                                };
16288626eedSJames Wright     // The Physics
16388626eedSJames Wright     // Zero v so all future terms can safely sum into it
164ba6664aeSJames Wright     for (CeedInt j=0; j<5; j++) v[j][i] = 0.;
16588626eedSJames Wright 
1662b89d87eSLeila Ghaffari     const CeedScalar u_normal = Dot3(norm, s_exact.Y.velocity);
16788626eedSJames Wright 
16888626eedSJames Wright     // The Physics
16988626eedSJames Wright     // -- Density
17088626eedSJames Wright     v[0][i] -= wdetJb * rho_in * u_normal;
17188626eedSJames Wright 
17288626eedSJames Wright     // -- Momentum
173ba6664aeSJames Wright     for (CeedInt j=0; j<3; j++)
1742b89d87eSLeila Ghaffari       v[j+1][i] -= wdetJb * (rho_in * u_normal * s_exact.Y.velocity[j] +
17588626eedSJames Wright                              norm[j] * P);
17688626eedSJames Wright 
17788626eedSJames Wright     // -- Total Energy Density
17888626eedSJames Wright     v[4][i] -= wdetJb * u_normal * (E + P);
17988626eedSJames Wright 
18088626eedSJames Wright   } // End Quadrature Point Loop
18188626eedSJames Wright   return 0;
18288626eedSJames Wright }
18388626eedSJames Wright 
18488626eedSJames Wright // *****************************************************************************
1852b89d87eSLeila Ghaffari // This QFunction set the outflow boundary condition for conservative variables
1862b89d87eSLeila Ghaffari // *****************************************************************************
18788626eedSJames Wright CEED_QFUNCTION(Channel_Outflow)(void *ctx, CeedInt Q,
18888626eedSJames Wright                                 const CeedScalar *const *in,
18988626eedSJames Wright                                 CeedScalar *const *out) {
19088626eedSJames Wright   // *INDENT-OFF*
19188626eedSJames Wright   // Inputs
19288626eedSJames Wright   const CeedScalar (*q)[CEED_Q_VLA]          = (const CeedScalar(*)[CEED_Q_VLA])in[0],
193e8b03feeSJames Wright                    (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2];
194e8b03feeSJames Wright 
19588626eedSJames Wright   // Outputs
19688626eedSJames Wright   CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0];
19788626eedSJames Wright   // *INDENT-ON*
19888626eedSJames Wright 
19988626eedSJames Wright   const ChannelContext context = (ChannelContext)ctx;
20088626eedSJames Wright   const bool implicit     = context->implicit;
20188626eedSJames Wright   const CeedScalar P0     = context->P0;
20288626eedSJames Wright 
20388626eedSJames Wright   CeedPragmaSIMD
20488626eedSJames Wright   // Quadrature Point Loop
20588626eedSJames Wright   for (CeedInt i=0; i<Q; i++) {
20688626eedSJames Wright     // Setup
20788626eedSJames Wright     // -- Interp in
20888626eedSJames Wright     const CeedScalar rho      =  q[0][i];
20988626eedSJames Wright     const CeedScalar u[3]     = {q[1][i] / rho,
21088626eedSJames Wright                                  q[2][i] / rho,
21188626eedSJames Wright                                  q[3][i] / rho
21288626eedSJames Wright                                 };
21388626eedSJames Wright     const CeedScalar E        =  q[4][i];
21488626eedSJames Wright 
21588626eedSJames Wright     // -- Interp-to-Interp q_data
21688626eedSJames Wright     // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q).
21788626eedSJames Wright     // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q).
21888626eedSJames Wright     // We can effect this by swapping the sign on this weight
21988626eedSJames Wright     const CeedScalar wdetJb  = (implicit ? -1. : 1.) * q_data_sur[0][i];
22088626eedSJames Wright 
22188626eedSJames Wright     // ---- Normal vect
22288626eedSJames Wright     const CeedScalar norm[3] = {q_data_sur[1][i],
22388626eedSJames Wright                                 q_data_sur[2][i],
22488626eedSJames Wright                                 q_data_sur[3][i]
22588626eedSJames Wright                                };
22688626eedSJames Wright     // The Physics
22788626eedSJames Wright     // Zero v so all future terms can safely sum into it
228ba6664aeSJames Wright     for (CeedInt j=0; j<5; j++) v[j][i] = 0.;
22988626eedSJames Wright 
23088626eedSJames Wright     // Implementing outflow condition
23188626eedSJames Wright     const CeedScalar P         = P0; // pressure
23213fa47b2SJames Wright     const CeedScalar u_normal  = Dot3(norm, u); // Normal velocity
23388626eedSJames Wright     // The Physics
23488626eedSJames Wright     // -- Density
23588626eedSJames Wright     v[0][i] -= wdetJb * rho * u_normal;
23688626eedSJames Wright 
23788626eedSJames Wright     // -- Momentum
238ba6664aeSJames Wright     for (CeedInt j=0; j<3; j++)
23988626eedSJames Wright       v[j+1][i] -= wdetJb *(rho * u_normal * u[j] + norm[j] * P);
24088626eedSJames Wright 
24188626eedSJames Wright     // -- Total Energy Density
24288626eedSJames Wright     v[4][i] -= wdetJb * u_normal * (E + P);
24388626eedSJames Wright 
24488626eedSJames Wright   } // End Quadrature Point Loop
24588626eedSJames Wright   return 0;
24688626eedSJames Wright }
247dc805cc4SLeila Ghaffari 
248dc805cc4SLeila Ghaffari // *****************************************************************************
24988626eedSJames Wright #endif // channel_h
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