Files
test2/intern/cycles/kernel/light/distant.h
Brecht Van Lommel e813e46327 Cycles: Refactor lights to be objects
This is an intermediate steps towards making lights actual geometry.
Light is now a subclass of Geometry, which simplifies some code.

The geometry is not added to the BVH yet, which would be the next
step and improve light intersection performance with many lights.

This makes object attributes work on lights.

Co-authored-by: Lukas Stockner <lukas@lukasstockner.de>
Pull Request: https://projects.blender.org/blender/blender/pulls/134846
2025-02-24 23:44:14 +01:00

168 lines
5.1 KiB
C++

/* SPDX-FileCopyrightText: 2011-2022 Blender Foundation
*
* SPDX-License-Identifier: Apache-2.0 */
#pragma once
#include "kernel/geom/object.h"
#include "kernel/light/common.h"
#include "util/math_fast.h"
CCL_NAMESPACE_BEGIN
ccl_device_inline void distant_light_uv(KernelGlobals kg,
const ccl_global KernelLight *klight,
const float3 D,
ccl_private float *u,
ccl_private float *v)
{
/* Map direction (x, y, z) to disk [-0.5, 0.5]^2:
* r^2 = (1 - z) / (1 - cos(klight->distant.angle))
* u_ = 0.5 * x * r / sin_angle(D, -klight->co)
* v_ = 0.5 * y * r / sin_angle(D, -klight->co) */
const float fac = klight->distant.half_inv_sin_half_angle / len(D - klight->co);
/* Get u axis and v axis. */
const Transform itfm = lamp_get_inverse_transform(kg, klight);
const float u_ = dot(D, make_float3(itfm.x)) * fac;
const float v_ = dot(D, make_float3(itfm.y)) * fac;
/* NOTE: Return barycentric coordinates in the same notation as Embree and OptiX. */
*u = v_ + 0.5f;
*v = -u_ - v_;
}
ccl_device_inline bool distant_light_sample(KernelGlobals kg,
const ccl_global KernelLight *klight,
const float2 rand,
ccl_private LightSample *ls)
{
float unused;
ls->Ng = sample_uniform_cone(
klight->co, klight->distant.one_minus_cosangle, rand, &unused, &ls->pdf);
ls->P = ls->Ng;
ls->D = -ls->Ng;
ls->t = FLT_MAX;
ls->eval_fac = klight->distant.eval_fac;
distant_light_uv(kg, klight, ls->D, &ls->u, &ls->v);
return true;
}
/* Special intersection check.
* Returns true if the distant_light_sample_from_intersection() for this light would return true.
*
* The intersection parameters t, u, v are optimized for the shadow ray towards a dedicated light:
* u = v = 0, t = FLT_MAX.
*/
ccl_device bool distant_light_intersect(const ccl_global KernelLight *klight,
const ccl_private Ray *ccl_restrict ray,
ccl_private float *t,
ccl_private float *u,
ccl_private float *v)
{
kernel_assert(klight->type == LIGHT_DISTANT);
if (klight->distant.angle == 0.0f) {
return false;
}
if (vector_angle(-klight->co, ray->D) > klight->distant.angle) {
return false;
}
*t = FLT_MAX;
*u = 0.0f;
*v = 0.0f;
return true;
}
ccl_device bool distant_light_sample_from_intersection(KernelGlobals kg,
const float3 ray_D,
const int lamp,
ccl_private LightSample *ccl_restrict ls)
{
const ccl_global KernelLight *klight = &kernel_data_fetch(lights, lamp);
const int shader = klight->shader_id;
const LightType type = (LightType)klight->type;
if (type != LIGHT_DISTANT) {
return false;
}
if (!(shader & SHADER_USE_MIS)) {
return false;
}
if (klight->distant.angle == 0.0f) {
return false;
}
/* Workaround to prevent a hang in the classroom scene with AMD HIP drivers 22.10,
* Remove when a compiler fix is available. */
#ifdef __HIP__
ls->shader = klight->shader_id;
#endif
if (vector_angle(-klight->co, ray_D) > klight->distant.angle) {
return false;
}
ls->type = type;
#ifndef __HIP__
ls->shader = klight->shader_id;
#endif
ls->object = klight->object_id;
ls->prim = lamp;
ls->t = FLT_MAX;
ls->P = -ray_D;
ls->Ng = -ray_D;
ls->D = ray_D;
ls->group = object_lightgroup(kg, ls->object);
ls->pdf = klight->distant.pdf;
ls->eval_fac = klight->distant.eval_fac;
distant_light_uv(kg, klight, ray_D, &ls->u, &ls->v);
return true;
}
template<bool in_volume_segment>
ccl_device_forceinline bool distant_light_tree_parameters(const float3 centroid,
const float theta_e,
const float t,
ccl_private float &cos_theta_u,
ccl_private float2 &distance,
ccl_private float3 &point_to_centroid,
ccl_private float &theta_d)
{
if (in_volume_segment) {
if (t == FLT_MAX) {
/* In world volumes, distant lights can contribute to the lighting of the volume with
* specific configurations of procedurally generated volumes. Use a ray length of 1.0 in this
* case to give the distant light some weight, but one that isn't too high for a typical
* world volume use case. */
theta_d = 1.0f;
}
else {
theta_d = t;
}
}
/* Treating it as a disk light 1 unit away */
cos_theta_u = fast_cosf(theta_e);
distance = make_float2(1.0f / cos_theta_u, 1.0f);
point_to_centroid = -centroid;
return true;
}
CCL_NAMESPACE_END