1ae2b091fSJames Wright // SPDX-FileCopyrightText: Copyright (c) 2017-2024, HONEE contributors. 2ae2b091fSJames Wright // SPDX-License-Identifier: Apache-2.0 OR BSD-2-Clause 3af8870a9STimothy Aiken 4af8870a9STimothy Aiken /// @file 504e40bb6SJeremy L Thompson /// Shock tube initial condition and Euler equation operator for Navier-Stokes example using PETSc - modified from eulervortex.h 6af8870a9STimothy Aiken 7af8870a9STimothy Aiken // Model from: 804e40bb6SJeremy L Thompson // On the Order of Accuracy and Numerical Performance of Two Classes of Finite Volume WENO Schemes, Zhang, Zhang, and Shu (2011). 9493642f1SJames Wright #include <ceed.h> 10d0cce58aSJeremy L Thompson #include <math.h> 112b916ea7SJeremy L Thompson 12704b8bbeSJames Wright #include "utils.h" 13af8870a9STimothy Aiken 143636f6a4SJames Wright typedef struct SetupContextShock_ *SetupContextShock; 153636f6a4SJames Wright struct SetupContextShock_ { 16af8870a9STimothy Aiken CeedScalar theta0; 17af8870a9STimothy Aiken CeedScalar thetaC; 18af8870a9STimothy Aiken CeedScalar P0; 19af8870a9STimothy Aiken CeedScalar N; 20af8870a9STimothy Aiken CeedScalar cv; 21af8870a9STimothy Aiken CeedScalar cp; 22af8870a9STimothy Aiken CeedScalar time; 23af8870a9STimothy Aiken CeedScalar mid_point; 24af8870a9STimothy Aiken CeedScalar P_high; 25af8870a9STimothy Aiken CeedScalar rho_high; 26af8870a9STimothy Aiken CeedScalar P_low; 27af8870a9STimothy Aiken CeedScalar rho_low; 28af8870a9STimothy Aiken }; 29af8870a9STimothy Aiken 30af8870a9STimothy Aiken typedef struct ShockTubeContext_ *ShockTubeContext; 31af8870a9STimothy Aiken struct ShockTubeContext_ { 32af8870a9STimothy Aiken CeedScalar Cyzb; 33af8870a9STimothy Aiken CeedScalar Byzb; 34af8870a9STimothy Aiken CeedScalar c_tau; 35af8870a9STimothy Aiken bool implicit; 36af8870a9STimothy Aiken bool yzb; 37af8870a9STimothy Aiken int stabilization; 38af8870a9STimothy Aiken }; 39af8870a9STimothy Aiken 40af8870a9STimothy Aiken // ***************************************************************************** 41af8870a9STimothy Aiken // This function sets the initial conditions 42af8870a9STimothy Aiken // 43af8870a9STimothy Aiken // Temperature: 44af8870a9STimothy Aiken // T = P / (rho * R) 45af8870a9STimothy Aiken // Density: 46af8870a9STimothy Aiken // rho = 1.0 if x <= mid_point 47af8870a9STimothy Aiken // = 0.125 if x > mid_point 48af8870a9STimothy Aiken // Pressure: 49af8870a9STimothy Aiken // P = 1.0 if x <= mid_point 50af8870a9STimothy Aiken // = 0.1 if x > mid_point 51af8870a9STimothy Aiken // Velocity: 52af8870a9STimothy Aiken // u = 0 53af8870a9STimothy Aiken // Velocity/Momentum Density: 54af8870a9STimothy Aiken // Ui = rho ui 55af8870a9STimothy Aiken // Total Energy: 56af8870a9STimothy Aiken // E = P / (gamma - 1) + rho (u u)/2 57af8870a9STimothy Aiken // 58af8870a9STimothy Aiken // Constants: 59af8870a9STimothy Aiken // cv , Specific heat, constant volume 60af8870a9STimothy Aiken // cp , Specific heat, constant pressure 61af8870a9STimothy Aiken // mid_point , Location of initial domain mid_point 62af8870a9STimothy Aiken // gamma = cp / cv, Specific heat ratio 63af8870a9STimothy Aiken // 64af8870a9STimothy Aiken // ***************************************************************************** 65af8870a9STimothy Aiken 66af8870a9STimothy Aiken // ***************************************************************************** 6704e40bb6SJeremy L Thompson // This helper function provides support for the exact, time-dependent solution (currently not implemented) and IC formulation for Euler traveling 6804e40bb6SJeremy L Thompson // vortex 69af8870a9STimothy Aiken // ***************************************************************************** 702b916ea7SJeremy L Thompson CEED_QFUNCTION_HELPER CeedInt Exact_ShockTube(CeedInt dim, CeedScalar time, const CeedScalar X[], CeedInt Nf, CeedScalar q[], void *ctx) { 71af8870a9STimothy Aiken // Context 723636f6a4SJames Wright const SetupContextShock context = (SetupContextShock)ctx; 73af8870a9STimothy Aiken const CeedScalar mid_point = context->mid_point; // Midpoint of the domain 74af8870a9STimothy Aiken const CeedScalar P_high = context->P_high; // Driver section pressure 75af8870a9STimothy Aiken const CeedScalar rho_high = context->rho_high; // Driver section density 76af8870a9STimothy Aiken const CeedScalar P_low = context->P_low; // Driven section pressure 77af8870a9STimothy Aiken const CeedScalar rho_low = context->rho_low; // Driven section density 78af8870a9STimothy Aiken 79af8870a9STimothy Aiken // Setup 80af8870a9STimothy Aiken const CeedScalar gamma = 1.4; // ratio of specific heats 81af8870a9STimothy Aiken const CeedScalar x = X[0]; // Coordinates 82af8870a9STimothy Aiken 83af8870a9STimothy Aiken CeedScalar rho, P, u[3] = {0.}; 84af8870a9STimothy Aiken 85af8870a9STimothy Aiken // Initial Conditions 8667263decSKenneth E. Jansen if (x <= mid_point + 200 * CEED_EPSILON) { 87af8870a9STimothy Aiken rho = rho_high; 88af8870a9STimothy Aiken P = P_high; 89af8870a9STimothy Aiken } else { 90af8870a9STimothy Aiken rho = rho_low; 91af8870a9STimothy Aiken P = P_low; 92af8870a9STimothy Aiken } 93af8870a9STimothy Aiken 94af8870a9STimothy Aiken // Assign exact solution 95af8870a9STimothy Aiken q[0] = rho; 96af8870a9STimothy Aiken q[1] = rho * u[0]; 97af8870a9STimothy Aiken q[2] = rho * u[1]; 98af8870a9STimothy Aiken q[3] = rho * u[2]; 99af8870a9STimothy Aiken q[4] = P / (gamma - 1.0) + rho * (u[0] * u[0]) / 2.; 100af8870a9STimothy Aiken 101af8870a9STimothy Aiken return 0; 102af8870a9STimothy Aiken } 103af8870a9STimothy Aiken 104af8870a9STimothy Aiken // ***************************************************************************** 105af8870a9STimothy Aiken // Helper function for computing flux Jacobian 106af8870a9STimothy Aiken // ***************************************************************************** 1072b916ea7SJeremy L Thompson CEED_QFUNCTION_HELPER void ConvectiveFluxJacobian_Euler(CeedScalar dF[3][5][5], const CeedScalar rho, const CeedScalar u[3], const CeedScalar E, 108af8870a9STimothy Aiken const CeedScalar gamma) { 109af8870a9STimothy Aiken CeedScalar u_sq = u[0] * u[0] + u[1] * u[1] + u[2] * u[2]; // Velocity square 110af8870a9STimothy Aiken for (CeedInt i = 0; i < 3; i++) { // Jacobian matrices for 3 directions 111af8870a9STimothy Aiken for (CeedInt j = 0; j < 3; j++) { // Rows of each Jacobian matrix 112af8870a9STimothy Aiken dF[i][j + 1][0] = ((i == j) ? ((gamma - 1.) * (u_sq / 2.)) : 0.) - u[i] * u[j]; 113af8870a9STimothy Aiken for (CeedInt k = 0; k < 3; k++) { // Columns of each Jacobian matrix 114af8870a9STimothy Aiken dF[i][0][k + 1] = ((i == k) ? 1. : 0.); 1152b916ea7SJeremy L Thompson dF[i][j + 1][k + 1] = ((j == k) ? u[i] : 0.) + ((i == k) ? u[j] : 0.) - ((i == j) ? u[k] : 0.) * (gamma - 1.); 1162b916ea7SJeremy L Thompson dF[i][4][k + 1] = ((i == k) ? (E * gamma / rho - (gamma - 1.) * u_sq / 2.) : 0.) - (gamma - 1.) * u[i] * u[k]; 117af8870a9STimothy Aiken } 118af8870a9STimothy Aiken dF[i][j + 1][4] = ((i == j) ? (gamma - 1.) : 0.); 119af8870a9STimothy Aiken } 120af8870a9STimothy Aiken dF[i][4][0] = u[i] * ((gamma - 1.) * u_sq - E * gamma / rho); 121af8870a9STimothy Aiken dF[i][4][4] = u[i] * gamma; 122af8870a9STimothy Aiken } 123af8870a9STimothy Aiken } 124af8870a9STimothy Aiken 125af8870a9STimothy Aiken // ***************************************************************************** 12604e40bb6SJeremy L Thompson // Helper function for calculating the covariant length scale in the direction of some 3 element input vector 127af8870a9STimothy Aiken // 128af8870a9STimothy Aiken // Where 129af8870a9STimothy Aiken // vec = vector that length is measured in the direction of 130af8870a9STimothy Aiken // h = covariant element length along vec 131af8870a9STimothy Aiken // ***************************************************************************** 1322b916ea7SJeremy L Thompson CEED_QFUNCTION_HELPER CeedScalar Covariant_length_along_vector(CeedScalar vec[3], const CeedScalar dXdx[3][3]) { 133af8870a9STimothy Aiken CeedScalar vec_dot_jacobian[3] = {0.0}; 134*78e8b7daSJames Wright 135*78e8b7daSJames Wright MatVec3(dXdx, vec, CEED_TRANSPOSE, vec_dot_jacobian); 136*78e8b7daSJames Wright return 2.0 * Norm3(vec) / Norm3(vec_dot_jacobian); 137af8870a9STimothy Aiken } 138af8870a9STimothy Aiken 139af8870a9STimothy Aiken // ***************************************************************************** 140af8870a9STimothy Aiken // Helper function for computing Tau elements (stabilization constant) 141af8870a9STimothy Aiken // Model from: 142af8870a9STimothy Aiken // Stabilized Methods for Compressible Flows, Hughes et al 2010 143af8870a9STimothy Aiken // 144af8870a9STimothy Aiken // Spatial criterion #2 - Tau is a 3x3 diagonal matrix 145af8870a9STimothy Aiken // Tau[i] = c_tau h[i] Xi(Pe) / rho(A[i]) (no sum) 146af8870a9STimothy Aiken // 147af8870a9STimothy Aiken // Where 148af8870a9STimothy Aiken // c_tau = stabilization constant (0.5 is reported as "optimal") 149af8870a9STimothy Aiken // h[i] = 2 length(dxdX[i]) 150af8870a9STimothy Aiken // Pe = Peclet number ( Pe = sqrt(u u) / dot(dXdx,u) diffusivity ) 151af8870a9STimothy Aiken // Xi(Pe) = coth Pe - 1. / Pe (1. at large local Peclet number ) 15204e40bb6SJeremy L Thompson // rho(A[i]) = spectral radius of the convective flux Jacobian i, wave speed in direction i 153af8870a9STimothy Aiken // ***************************************************************************** 1542b916ea7SJeremy L Thompson CEED_QFUNCTION_HELPER void Tau_spatial(CeedScalar Tau_x[3], const CeedScalar dXdx[3][3], const CeedScalar u[3], const CeedScalar sound_speed, 1552b916ea7SJeremy L Thompson const CeedScalar c_tau) { 156493642f1SJames Wright for (CeedInt i = 0; i < 3; i++) { 157af8870a9STimothy Aiken // length of element in direction i 158*78e8b7daSJames Wright CeedScalar h = 2 / sqrt(Square(dXdx[0][i]) + Square(dXdx[1][i]) + Square(dXdx[2][i])); 159af8870a9STimothy Aiken // fastest wave in direction i 160af8870a9STimothy Aiken CeedScalar fastest_wave = fabs(u[i]) + sound_speed; 161af8870a9STimothy Aiken Tau_x[i] = c_tau * h / fastest_wave; 162af8870a9STimothy Aiken } 163af8870a9STimothy Aiken } 164af8870a9STimothy Aiken 165af8870a9STimothy Aiken // ***************************************************************************** 166af8870a9STimothy Aiken // This QFunction sets the initial conditions for shock tube 167af8870a9STimothy Aiken // ***************************************************************************** 1682b916ea7SJeremy L Thompson CEED_QFUNCTION(ICsShockTube)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 169af8870a9STimothy Aiken const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 170af8870a9STimothy Aiken CeedScalar(*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 171af8870a9STimothy Aiken 172b193fadcSJames Wright CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 173af8870a9STimothy Aiken const CeedScalar x[] = {X[0][i], X[1][i], X[2][i]}; 174af8870a9STimothy Aiken CeedScalar q[5]; 175af8870a9STimothy Aiken 176af8870a9STimothy Aiken Exact_ShockTube(3, 0., x, 5, q, ctx); 177af8870a9STimothy Aiken 1782b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 5; j++) q0[j][i] = q[j]; 179b193fadcSJames Wright } 180af8870a9STimothy Aiken return 0; 181af8870a9STimothy Aiken } 182af8870a9STimothy Aiken 183af8870a9STimothy Aiken // ***************************************************************************** 18404e40bb6SJeremy L Thompson // This QFunction implements the following formulation of Euler equations with explicit time stepping method 185af8870a9STimothy Aiken // 18604e40bb6SJeremy L Thompson // This is 3D Euler for compressible gas dynamics in conservation form with state variables of density, momentum density, and total energy density. 187af8870a9STimothy Aiken // 188af8870a9STimothy Aiken // State Variables: q = ( rho, U1, U2, U3, E ) 189af8870a9STimothy Aiken // rho - Mass Density 190af8870a9STimothy Aiken // Ui - Momentum Density, Ui = rho ui 191af8870a9STimothy Aiken // E - Total Energy Density, E = P / (gamma - 1) + rho (u u)/2 192af8870a9STimothy Aiken // 193af8870a9STimothy Aiken // Euler Equations: 194af8870a9STimothy Aiken // drho/dt + div( U ) = 0 195af8870a9STimothy Aiken // dU/dt + div( rho (u x u) + P I3 ) = 0 196af8870a9STimothy Aiken // dE/dt + div( (E + P) u ) = 0 197af8870a9STimothy Aiken // 198af8870a9STimothy Aiken // Equation of State: 199af8870a9STimothy Aiken // P = (gamma - 1) (E - rho (u u) / 2) 200af8870a9STimothy Aiken // 201af8870a9STimothy Aiken // Constants: 202af8870a9STimothy Aiken // cv , Specific heat, constant volume 203af8870a9STimothy Aiken // cp , Specific heat, constant pressure 204af8870a9STimothy Aiken // g , Gravity 205af8870a9STimothy Aiken // gamma = cp / cv, Specific heat ratio 206af8870a9STimothy Aiken // ***************************************************************************** 2072b916ea7SJeremy L Thompson CEED_QFUNCTION(EulerShockTube)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) { 2083d65b166SJames Wright const CeedScalar(*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 2093d65b166SJames Wright const CeedScalar(*dq)[5][CEED_Q_VLA] = (const CeedScalar(*)[5][CEED_Q_VLA])in[1]; 210ade49511SJames Wright const CeedScalar(*q_data) = in[2]; 2113d65b166SJames Wright CeedScalar(*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 2123d65b166SJames Wright CeedScalar(*dv)[5][CEED_Q_VLA] = (CeedScalar(*)[5][CEED_Q_VLA])out[1]; 213af8870a9STimothy Aiken 214af8870a9STimothy Aiken const CeedScalar gamma = 1.4; 215af8870a9STimothy Aiken 216af8870a9STimothy Aiken ShockTubeContext context = (ShockTubeContext)ctx; 217af8870a9STimothy Aiken const CeedScalar Cyzb = context->Cyzb; 218af8870a9STimothy Aiken const CeedScalar Byzb = context->Byzb; 219af8870a9STimothy Aiken const CeedScalar c_tau = context->c_tau; 220af8870a9STimothy Aiken 221b193fadcSJames Wright CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) { 222af8870a9STimothy Aiken // Setup 223af8870a9STimothy Aiken // -- Interp in 224af8870a9STimothy Aiken const CeedScalar rho = q[0][i]; 2252b916ea7SJeremy L Thompson const CeedScalar u[3] = {q[1][i] / rho, q[2][i] / rho, q[3][i] / rho}; 226af8870a9STimothy Aiken const CeedScalar E = q[4][i]; 2272b916ea7SJeremy L Thompson const CeedScalar drho[3] = {dq[0][0][i], dq[1][0][i], dq[2][0][i]}; 2282b916ea7SJeremy L Thompson const CeedScalar dU[3][3] = { 2292b916ea7SJeremy L Thompson {dq[0][1][i], dq[1][1][i], dq[2][1][i]}, 2302b916ea7SJeremy L Thompson {dq[0][2][i], dq[1][2][i], dq[2][2][i]}, 2312b916ea7SJeremy L Thompson {dq[0][3][i], dq[1][3][i], dq[2][3][i]} 232af8870a9STimothy Aiken }; 2332b916ea7SJeremy L Thompson const CeedScalar dE[3] = {dq[0][4][i], dq[1][4][i], dq[2][4][i]}; 234ade49511SJames Wright CeedScalar wdetJ, dXdx[3][3]; 235ade49511SJames Wright QdataUnpack_3D(Q, i, q_data, &wdetJ, dXdx); 236af8870a9STimothy Aiken // dU/dx 237af8870a9STimothy Aiken CeedScalar du[3][3] = {{0}}; 238af8870a9STimothy Aiken CeedScalar drhodx[3] = {0}; 239af8870a9STimothy Aiken CeedScalar dEdx[3] = {0}; 240af8870a9STimothy Aiken CeedScalar dUdx[3][3] = {{0}}; 241af8870a9STimothy Aiken CeedScalar dXdxdXdxT[3][3] = {{0}}; 242493642f1SJames Wright for (CeedInt j = 0; j < 3; j++) { 243493642f1SJames Wright for (CeedInt k = 0; k < 3; k++) { 244af8870a9STimothy Aiken du[j][k] = (dU[j][k] - drho[k] * u[j]) / rho; 245af8870a9STimothy Aiken drhodx[j] += drho[k] * dXdx[k][j]; 246af8870a9STimothy Aiken dEdx[j] += dE[k] * dXdx[k][j]; 247493642f1SJames Wright for (CeedInt l = 0; l < 3; l++) { 248af8870a9STimothy Aiken dUdx[j][k] += dU[j][l] * dXdx[l][k]; 249af8870a9STimothy Aiken dXdxdXdxT[j][k] += dXdx[j][l] * dXdx[k][l]; // dXdx_j,k * dXdx_k,j 250af8870a9STimothy Aiken } 251af8870a9STimothy Aiken } 252af8870a9STimothy Aiken } 253af8870a9STimothy Aiken 2542b916ea7SJeremy L Thompson const CeedScalar E_kinetic = 0.5 * rho * (u[0] * u[0] + u[1] * u[1] + u[2] * u[2]), E_internal = E - E_kinetic, 255af8870a9STimothy Aiken P = E_internal * (gamma - 1); // P = pressure 256af8870a9STimothy Aiken 257af8870a9STimothy Aiken // The Physics 258af8870a9STimothy Aiken // Zero v and dv so all future terms can safely sum into it 259493642f1SJames Wright for (CeedInt j = 0; j < 5; j++) { 260af8870a9STimothy Aiken v[j][i] = 0; 2612b916ea7SJeremy L Thompson for (CeedInt k = 0; k < 3; k++) dv[k][j][i] = 0; 262af8870a9STimothy Aiken } 263af8870a9STimothy Aiken 264af8870a9STimothy Aiken // -- Density 265af8870a9STimothy Aiken // ---- u rho 2662b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 3; j++) dv[j][0][i] += wdetJ * (rho * u[0] * dXdx[j][0] + rho * u[1] * dXdx[j][1] + rho * u[2] * dXdx[j][2]); 267af8870a9STimothy Aiken // -- Momentum 268af8870a9STimothy Aiken // ---- rho (u x u) + P I3 2692b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 3; j++) { 2702b916ea7SJeremy L Thompson for (CeedInt k = 0; k < 3; k++) { 2712b916ea7SJeremy L Thompson dv[k][j + 1][i] += wdetJ * ((rho * u[j] * u[0] + (j == 0 ? P : 0)) * dXdx[k][0] + (rho * u[j] * u[1] + (j == 1 ? P : 0)) * dXdx[k][1] + 272af8870a9STimothy Aiken (rho * u[j] * u[2] + (j == 2 ? P : 0)) * dXdx[k][2]); 2732b916ea7SJeremy L Thompson } 2742b916ea7SJeremy L Thompson } 275af8870a9STimothy Aiken // -- Total Energy Density 276af8870a9STimothy Aiken // ---- (E + P) u 2772b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 3; j++) dv[j][4][i] += wdetJ * (E + P) * (u[0] * dXdx[j][0] + u[1] * dXdx[j][1] + u[2] * dXdx[j][2]); 278af8870a9STimothy Aiken 279af8870a9STimothy Aiken // -- YZB stabilization 280af8870a9STimothy Aiken if (context->yzb) { 281af8870a9STimothy Aiken CeedScalar drho_norm = 0.0; // magnitude of the density gradient 282af8870a9STimothy Aiken CeedScalar j_vec[3] = {0.0}; // unit vector aligned with the density gradient 283af8870a9STimothy Aiken CeedScalar h_shock = 0.0; // element lengthscale 284af8870a9STimothy Aiken CeedScalar acoustic_vel = 0.0; // characteristic velocity, acoustic speed 285af8870a9STimothy Aiken CeedScalar tau_shock = 0.0; // timescale 286af8870a9STimothy Aiken CeedScalar nu_shock = 0.0; // artificial diffusion 287af8870a9STimothy Aiken 288af8870a9STimothy Aiken // Unit vector aligned with the density gradient 289*78e8b7daSJames Wright drho_norm = Norm3(drhodx); 2902b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 3; j++) j_vec[j] = drhodx[j] / (drho_norm + 1e-20); 291af8870a9STimothy Aiken 292af8870a9STimothy Aiken if (drho_norm == 0.0) { 293af8870a9STimothy Aiken nu_shock = 0.0; 294af8870a9STimothy Aiken } else { 295af8870a9STimothy Aiken h_shock = Covariant_length_along_vector(j_vec, dXdx); 296af8870a9STimothy Aiken h_shock /= Cyzb; 297af8870a9STimothy Aiken acoustic_vel = sqrt(gamma * P / rho); 298af8870a9STimothy Aiken tau_shock = h_shock / (2 * acoustic_vel) * pow(drho_norm * h_shock / rho, Byzb); 299af8870a9STimothy Aiken nu_shock = fabs(tau_shock * acoustic_vel * acoustic_vel); 300af8870a9STimothy Aiken } 301af8870a9STimothy Aiken 3022b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 3; j++) dv[j][0][i] -= wdetJ * nu_shock * drhodx[j]; 303af8870a9STimothy Aiken 3042b916ea7SJeremy L Thompson for (CeedInt k = 0; k < 3; k++) { 3052b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 3; j++) dv[j][k][i] -= wdetJ * nu_shock * du[k][j]; 3062b916ea7SJeremy L Thompson } 307af8870a9STimothy Aiken 3082b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 3; j++) dv[j][4][i] -= wdetJ * nu_shock * dEdx[j]; 309af8870a9STimothy Aiken } 310af8870a9STimothy Aiken 311af8870a9STimothy Aiken // Stabilization 312af8870a9STimothy Aiken // Need the Jacobian for the advective fluxes for stabilization 313af8870a9STimothy Aiken // indexed as: jacob_F_conv[direction][flux component][solution component] 314af8870a9STimothy Aiken CeedScalar jacob_F_conv[3][5][5] = {{{0.}}}; 315af8870a9STimothy Aiken ConvectiveFluxJacobian_Euler(jacob_F_conv, rho, u, E, gamma); 316af8870a9STimothy Aiken 317af8870a9STimothy Aiken // dqdx collects drhodx, dUdx and dEdx in one vector 318af8870a9STimothy Aiken CeedScalar dqdx[5][3]; 319493642f1SJames Wright for (CeedInt j = 0; j < 3; j++) { 320af8870a9STimothy Aiken dqdx[0][j] = drhodx[j]; 321af8870a9STimothy Aiken dqdx[4][j] = dEdx[j]; 3222b916ea7SJeremy L Thompson for (CeedInt k = 0; k < 3; k++) dqdx[k + 1][j] = dUdx[k][j]; 323af8870a9STimothy Aiken } 324af8870a9STimothy Aiken 325af8870a9STimothy Aiken // strong_conv = dF/dq * dq/dx (Strong convection) 326af8870a9STimothy Aiken CeedScalar strong_conv[5] = {0}; 3272b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 3; j++) { 3282b916ea7SJeremy L Thompson for (CeedInt k = 0; k < 5; k++) { 3292b916ea7SJeremy L Thompson for (CeedInt l = 0; l < 5; l++) strong_conv[k] += jacob_F_conv[j][k][l] * dqdx[l][j]; 3302b916ea7SJeremy L Thompson } 3312b916ea7SJeremy L Thompson } 332af8870a9STimothy Aiken 333af8870a9STimothy Aiken // Stabilization 334af8870a9STimothy Aiken // -- Tau elements 335af8870a9STimothy Aiken const CeedScalar sound_speed = sqrt(gamma * P / rho); 336af8870a9STimothy Aiken CeedScalar Tau_x[3] = {0.}; 337af8870a9STimothy Aiken Tau_spatial(Tau_x, dXdx, u, sound_speed, c_tau); 338af8870a9STimothy Aiken 339af8870a9STimothy Aiken CeedScalar stab[5][3] = {0}; 340af8870a9STimothy Aiken switch (context->stabilization) { 341af8870a9STimothy Aiken case 0: // Galerkin 342af8870a9STimothy Aiken break; 343af8870a9STimothy Aiken case 1: // SU 3442b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 3; j++) { 3452b916ea7SJeremy L Thompson for (CeedInt k = 0; k < 5; k++) { 346493642f1SJames Wright for (CeedInt l = 0; l < 5; l++) { 347af8870a9STimothy Aiken stab[k][j] += jacob_F_conv[j][k][l] * Tau_x[j] * strong_conv[l]; 348af8870a9STimothy Aiken } 3492b916ea7SJeremy L Thompson } 3502b916ea7SJeremy L Thompson } 3512b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 5; j++) { 3522b916ea7SJeremy L Thompson for (CeedInt k = 0; k < 3; k++) dv[k][j][i] -= wdetJ * (stab[j][0] * dXdx[k][0] + stab[j][1] * dXdx[k][1] + stab[j][2] * dXdx[k][2]); 3532b916ea7SJeremy L Thompson } 354af8870a9STimothy Aiken break; 355af8870a9STimothy Aiken } 356b193fadcSJames Wright } 357af8870a9STimothy Aiken return 0; 358af8870a9STimothy Aiken } 359