FiniteVolumeGPU/SWESimulators/fluxes/WeightedAverageFlux.cu
2018-08-09 10:16:05 +02:00

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/*
This file implements the Weighted Average Flux
Copyright (C) 2016, 2017, 2018 SINTEF ICT
This program is free software: you can redistribute it and/or modify
it under the terms of the GNU General Public License as published by
the Free Software Foundation, either version 3 of the License, or
(at your option) any later version.
This program is distributed in the hope that it will be useful,
but WITHOUT ANY WARRANTY; without even the implied warranty of
MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
GNU General Public License for more details.
You should have received a copy of the GNU General Public License
along with this program. If not, see <http://www.gnu.org/licenses/>.
*/
#include "limiters.cu"
/**
* Superbee flux limiter for WAF.
* Related to superbee limiter so that WAF_superbee(r, c) = 1 - (1-|c|)*superbee(r)
* @param r_ the ratio of upwind change (see Toro 2001, p. 203/204)
* @param c_ the courant number for wave k, dt*S_k/dx
*/
__device__ float WAF_superbee(float r_, float c_) {
// r <= 0.0
if (r_ <= 0.0f) {
return 1.0f;
}
// 0.0 <= r <= 1/2
else if (r_ <= 0.5f) {
return 1.0f - 2.0f*(1.0f - fabsf(c_))*r_;
}
// 1/2 <= r <= 1
else if (r_ <= 1.0f) {
return fabs(c_);
}
// 1 <= r <= 2
else if (r_ <= 2.0f) {
return 1.0f - (1.0f - fabsf(c_))*r_;
}
// r >= 2
else {
return 2.0f*fabsf(c_) - 1.0f;
}
}
__device__ float WAF_albada(float r_, float c_) {
if (r_ <= 0.0f) {
return 1.0f;
}
else {
return 1.0f - (1.0f - fabsf(c_)) * r_ * (1.0f + r_) / (1.0f + r_*r_);
}
}
__device__ float WAF_minbee(float r_, float c_) {
r_ = fmaxf(-1.0f, fminf(2.0f, r_));
if (r_ <= 0.0f) {
return 1.0f;
}
if (r_ >= 0.0f && r_ <= 1.0f) {
return 1.0f - (1.0f - fabsf(c_)) * r_;
}
else {
return fabsf(c_);
}
}
__device__ float WAF_minmod(float r_, float c_) {
return 1.0f - (1.0f - fabsf(c_)) * fmaxf(0.0f, fminf(1.0f, r_));
}
__device__ float limiterToWAFLimiter(float r_, float c_) {
return 1.0f - (1.0f - fabsf(c_))*r_;
}
__device__ float desingularize(float x_, float eps_) {
return copysign(1.0f, x_)*fmaxf(fabsf(x_), fminf(x_*x_/(2.0f*eps_)+0.5f*eps_, eps_));
}
// Compute h in the "star region", h^dagger
__device__ __inline__ float computeHStar(float h_l, float h_r, float u_l, float u_r, float c_l, float c_r, float g_) {
//This estimate for the h* gives rise to spurious oscillations.
//return 0.5f * (h_l+h_r) - 0.25f * (u_r-u_l)*(h_l+h_r)/(c_l+c_r);
const float h_tmp = 0.5f * (c_l + c_r) + 0.25f * (u_l - u_r);
return h_tmp*h_tmp / g_;
}
/**
* Weighted average flux (Toro 2001, p 200) for interface {i+1/2}
* @param r_ The flux limiter parameter (see Toro 2001, p. 203)
* @param Q_l2 Q_{i-1}
* @param Q_l1 Q_{i}
* @param Q_r1 Q_{i+1}
* @param Q_r2 Q_{i+2}
*/
__device__ float3 WAF_1D_flux(const float3 Q_l2, const float3 Q_l1, const float3 Q_r1, const float3 Q_r2, const float g_, const float dx_, const float dt_) {
const float h_l = Q_l1.x;
const float h_r = Q_r1.x;
const float h_l2 = Q_l2.x;
const float h_r2 = Q_r2.x;
// Calculate velocities
const float u_l = Q_l1.y / h_l;
const float u_r = Q_r1.y / h_r;
const float u_l2 = Q_l2.y / h_l2;
const float u_r2 = Q_r2.y / h_r2;
const float v_l = Q_l1.z / h_l;
const float v_r = Q_r1.z / h_r;
const float v_l2 = Q_l2.z / h_l2;
const float v_r2 = Q_r2.z / h_r2;
// Estimate the potential wave speeds
const float c_l = sqrt(g_*h_l);
const float c_r = sqrt(g_*h_r);
const float c_l2 = sqrt(g_*h_l2);
const float c_r2 = sqrt(g_*h_r2);
// Compute h in the "star region", h^dagger
const float h_dag_l = computeHStar(h_l2, h_l, u_l2, u_l, c_l2, c_l, g_);
const float h_dag = computeHStar( h_l, h_r, u_l, u_r, c_l, c_r, g_);
const float h_dag_r = computeHStar( h_r, h_r2, u_r, u_r2, c_r, c_r2, g_);
const float q_l_tmp = sqrt(0.5f * ( (h_dag+h_l)*h_dag ) ) / h_l;
const float q_r_tmp = sqrt(0.5f * ( (h_dag+h_r)*h_dag ) ) / h_r;
const float q_l = (h_dag > h_l) ? q_l_tmp : 1.0f;
const float q_r = (h_dag > h_r) ? q_r_tmp : 1.0f;
// Compute wave speed estimates
const float S_l = u_l - c_l*q_l;
const float S_r = u_r + c_r*q_r;
const float S_star = ( S_l*h_r*(u_r - S_r) - S_r*h_l*(u_l - S_l) ) / ( h_r*(u_r - S_r) - h_l*(u_l - S_l) );
const float3 Q_star_l = h_l * (S_l - u_l) / (S_l - S_star) * make_float3(1.0, S_star, v_l);
const float3 Q_star_r = h_r * (S_r - u_r) / (S_r - S_star) * make_float3(1.0, S_star, v_r);
// Estimate the fluxes in the four regions
const float3 F_1 = F_func(Q_l1, g_);
const float3 F_4 = F_func(Q_r1, g_);
const float3 F_2 = F_1 + S_l*(Q_star_l - Q_l1);
const float3 F_3 = F_4 + S_r*(Q_star_r - Q_r1);
//const float3 F_2 = F_func(Q_star_l, g_);
//const float3 F_3 = F_func(Q_star_r, g_);
// Compute the courant numbers for the waves
const float c_1 = S_l * dt_ / dx_;
const float c_2 = S_star * dt_ / dx_;
const float c_3 = S_r * dt_ / dx_;
// Compute the "upwind change" vectors for the i-3/2 and i+3/2 interfaces
const float eps = 1.0e-6f;
const float r_1 = desingularize( (c_1 > 0.0f) ? (h_dag_l - h_l2) : (h_dag_r - h_r), eps) / desingularize((h_dag - h_l), eps);
const float r_2 = desingularize( (c_2 > 0.0f) ? (v_l - v_l2) : (v_r2 - v_r), eps ) / desingularize((v_r - v_l), eps);
const float r_3 = desingularize( (c_3 > 0.0f) ? (h_l - h_dag_l) : (h_r2 - h_dag_r), eps ) / desingularize((h_r - h_dag), eps);
// Compute the limiter
// We use h for the nonlinear waves, and v for the middle shear wave
const float A_1 = copysign(1.0f, c_1) * limiterToWAFLimiter(generalized_minmod(r_1, 1.9f), c_1);
const float A_2 = copysign(1.0f, c_2) * limiterToWAFLimiter(generalized_minmod(r_2, 1.9f), c_2);
const float A_3 = copysign(1.0f, c_3) * limiterToWAFLimiter(generalized_minmod(r_3, 1.9f), c_3);
//Average the fluxes
const float3 flux = 0.5f*( F_1 + F_4 )
- 0.5f*( A_1 * (F_2 - F_1)
+ A_2 * (F_3 - F_2)
+ A_3 * (F_4 - F_3) );
return flux;
}