xref: /libCEED/examples/petsc/qfunctions/bps/bp1sphere.h (revision d36c159f42e9222d4587decadab914cf55859f56)
1 // Copyright (c) 2017, Lawrence Livermore National Security, LLC. Produced at
2 // the Lawrence Livermore National Laboratory. LLNL-CODE-734707. All Rights
3 // reserved. See files LICENSE and NOTICE for details.
4 //
5 // This file is part of CEED, a collection of benchmarks, miniapps, software
6 // libraries and APIs for efficient high-order finite element and spectral
7 // element discretizations for exascale applications. For more information and
8 // source code availability see http://github.com/ceed.
9 //
10 // The CEED research is supported by the Exascale Computing Project 17-SC-20-SC,
11 // a collaborative effort of two U.S. Department of Energy organizations (Office
12 // of Science and the National Nuclear Security Administration) responsible for
13 // the planning and preparation of a capable exascale ecosystem, including
14 // software, applications, hardware, advanced system engineering and early
15 // testbed platforms, in support of the nation's exascale computing imperative.
16 
17 /// @file
18 /// libCEED QFunctions for mass operator example for a scalar field on the sphere using PETSc
19 
20 #ifndef bp1sphere_h
21 #define bp1sphere_h
22 
23 #ifndef __CUDACC__
24 #  include <math.h>
25 #endif
26 
27 // *****************************************************************************
28 // This QFunction sets up the geometric factors required for integration and
29 //   coordinate transformations when reference coordinates have a different
30 //   dimension than the one of physical coordinates
31 //
32 // Reference (parent) 2D coordinates: X \in [-1, 1]^2
33 //
34 // Global 3D physical coordinates given by the mesh: xx \in [-R, R]^3
35 //   with R radius of the sphere
36 //
37 // Local 3D physical coordinates on the 2D manifold: x \in [-l, l]^3
38 //   with l half edge of the cube inscribed in the sphere
39 //
40 // Change of coordinates matrix computed by the library:
41 //   (physical 3D coords relative to reference 2D coords)
42 //   dxx_j/dX_i (indicial notation) [3 * 2]
43 //
44 // Change of coordinates x (on the 2D manifold) relative to xx (phyisical 3D):
45 //   dx_i/dxx_j (indicial notation) [3 * 3]
46 //
47 // Change of coordinates x (on the 2D manifold) relative to X (reference 2D):
48 //   (by chain rule)
49 //   dx_i/dX_j [3 * 2] = dx_i/dxx_k [3 * 3] * dxx_k/dX_j [3 * 2]
50 //
51 // modJ is given by the magnitude of the cross product of the columns of dx_i/dX_j
52 //
53 // The quadrature data is stored in the array qdata.
54 //
55 // We require the determinant of the Jacobian to properly compute integrals of
56 //   the form: int( u v )
57 //
58 // Qdata: modJ * w
59 //
60 // *****************************************************************************
61 
62 // *****************************************************************************
63 CEED_QFUNCTION(SetupMassGeo)(void *ctx, const CeedInt Q,
64                              const CeedScalar *const *in,
65                              CeedScalar *const *out) {
66   // Inputs
67   const CeedScalar *X = in[0], *J = in[1], *w = in[2];
68   // Outputs
69   CeedScalar *qdata = out[0];
70 
71   // Quadrature Point Loop
72   CeedPragmaSIMD
73   for (CeedInt i=0; i<Q; i++) {
74     // Read global Cartesian coordinates
75     const CeedScalar xx[3] = {X[i+0*Q],
76                               X[i+1*Q],
77                               X[i+2*Q]
78                              };
79 
80     // Read dxxdX Jacobian entries, stored as
81     // 0 3
82     // 1 4
83     // 2 5
84     const CeedScalar dxxdX[3][2] = {{J[i+Q*0],
85                                      J[i+Q*3]},
86                                     {J[i+Q*1],
87                                      J[i+Q*4]},
88                                     {J[i+Q*2],
89                                      J[i+Q*5]}
90                                    };
91 
92     // Setup
93     // x = xx (xx^T xx)^{-1/2}
94     // dx/dxx = I (xx^T xx)^{-1/2} - xx xx^T (xx^T xx)^{-3/2}
95     const CeedScalar modxxsq = xx[0]*xx[0]+xx[1]*xx[1]+xx[2]*xx[2];
96     CeedScalar xxsq[3][3];
97     for (int j=0; j<3; j++)
98       for (int k=0; k<3; k++)
99         xxsq[j][k] = xx[j]*xx[k] / (sqrt(modxxsq) * modxxsq);
100 
101     const CeedScalar dxdxx[3][3] = {{1./sqrt(modxxsq) - xxsq[0][0],
102                                      -xxsq[0][1],
103                                      -xxsq[0][2]},
104                                     {-xxsq[1][0],
105                                      1./sqrt(modxxsq) - xxsq[1][1],
106                                      -xxsq[1][2]},
107                                     {-xxsq[2][0],
108                                      -xxsq[2][1],
109                                      1./sqrt(modxxsq) - xxsq[2][2]}
110                                    };
111 
112     CeedScalar dxdX[3][2];
113     for (int j=0; j<3; j++)
114       for (int k=0; k<2; k++) {
115         dxdX[j][k] = 0;
116         for (int l=0; l<3; l++)
117           dxdX[j][k] += dxdxx[j][l]*dxxdX[l][k];
118       }
119 
120     // J is given by the cross product of the columns of dxdX
121     const CeedScalar J[3] = {dxdX[1][0]*dxdX[2][1] - dxdX[2][0]*dxdX[1][1],
122                              dxdX[2][0]*dxdX[0][1] - dxdX[0][0]*dxdX[2][1],
123                              dxdX[0][0]*dxdX[1][1] - dxdX[1][0]*dxdX[0][1]
124                             };
125 
126     // Use the magnitude of J as our detJ (volume scaling factor)
127     const CeedScalar modJ = sqrt(J[0]*J[0]+J[1]*J[1]+J[2]*J[2]);
128 
129     // Interp-to-Interp qdata
130     qdata[i+Q*0] = modJ * w[i];
131   } // End of Quadrature Point Loop
132 
133   return 0;
134 }
135 
136 // *****************************************************************************
137 // This QFunction sets up the rhs and true solution for the problem
138 // *****************************************************************************
139 
140 // -----------------------------------------------------------------------------
141 CEED_QFUNCTION(SetupMassRhs)(void *ctx, const CeedInt Q,
142                              const CeedScalar *const *in,
143                              CeedScalar *const *out) {
144   // Inputs
145   const CeedScalar *X = in[0], *qdata = in[1];
146   // Outputs
147   CeedScalar *true_soln = out[0], *rhs = out[1];
148 
149   // Context
150   const CeedScalar *context = (const CeedScalar*)ctx;
151   const CeedScalar R        = context[0];
152 
153   // Quadrature Point Loop
154   CeedPragmaSIMD
155   for (CeedInt i=0; i<Q; i++) {
156     // Compute latitude
157     const CeedScalar theta =  asin(X[i+2*Q] / R);
158 
159     // Use absolute value of latitute for true solution
160     true_soln[i] = fabs(theta);
161 
162     rhs[i] = qdata[i] * true_soln[i];
163   } // End of Quadrature Point Loop
164 
165   return 0;
166 }
167 
168 // *****************************************************************************
169 // This QFunction applies the mass operator for a scalar field.
170 //
171 // Inputs:
172 //   u     - Input vector at quadrature points
173 //   qdata - Geometric factors
174 //
175 // Output:
176 //   v     - Output vector (test functions) at quadrature points
177 //
178 // *****************************************************************************
179 
180 // -----------------------------------------------------------------------------
181 CEED_QFUNCTION(Mass)(void *ctx, const CeedInt Q,
182                      const CeedScalar *const *in, CeedScalar *const *out) {
183   // Inputs
184   const CeedScalar *u = in[0], *qdata = in[1];
185   // Outputs
186   CeedScalar *v = out[0];
187 
188   // Quadrature Point Loop
189   CeedPragmaSIMD
190   for (CeedInt i=0; i<Q; i++)
191     v[i] = qdata[i] * u[i];
192 
193   return 0;
194 }
195 // -----------------------------------------------------------------------------
196 
197 #endif // bp1sphere_h
198