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#include <fstream>
#include "Vector.hpp"
#include "Renderer.hpp"
#include "Scene.hpp"
#include <optional>
inline float deg2rad(const float °)
{ return deg * M_PI/180.0; }
// Compute reflection direction
Vector3f reflect(const Vector3f &I, const Vector3f &N)
{
return I - 2 * dotProduct(I, N) * N;
}
// [comment]
// Compute refraction direction using Snell's law
//
// We need to handle with care the two possible situations:
//
// - When the ray is inside the object
//
// - When the ray is outside.
//
// If the ray is outside, you need to make cosi positive cosi = -N.I
//
// If the ray is inside, you need to invert the refractive indices and negate the normal N
// [/comment]
Vector3f refract(const Vector3f &I, const Vector3f &N, const float &ior)
{
float cosi = clamp(-1, 1, dotProduct(I, N));
float etai = 1, etat = ior;
Vector3f n = N;
if (cosi < 0) { cosi = -cosi; } else { std::swap(etai, etat); n= -N; }
float eta = etai / etat;
float k = 1 - eta * eta * (1 - cosi * cosi);
return k < 0 ? 0 : eta * I + (eta * cosi - sqrtf(k)) * n;
}
// [comment]
// Compute Fresnel equation
//
// \param I is the incident view direction
//
// \param N is the normal at the intersection point
//
// \param ior is the material refractive index
// [/comment]
float fresnel(const Vector3f &I, const Vector3f &N, const float &ior)
{
float cosi = clamp(-1, 1, dotProduct(I, N));
float etai = 1, etat = ior;
if (cosi > 0) { std::swap(etai, etat); }
// Compute sini using Snell's law
float sint = etai / etat * sqrtf(std::max(0.f, 1 - cosi * cosi));
// Total internal reflection
if (sint >= 1) {
return 1;
}
else {
float cost = sqrtf(std::max(0.f, 1 - sint * sint));
cosi = fabsf(cosi);
float Rs = ((etat * cosi) - (etai * cost)) / ((etat * cosi) + (etai * cost));
float Rp = ((etai * cosi) - (etat * cost)) / ((etai * cosi) + (etat * cost));
return (Rs * Rs + Rp * Rp) / 2;
}
// As a consequence of the conservation of energy, transmittance is given by:
// kt = 1 - kr;
}
// [comment]
// Returns true if the ray intersects an object, false otherwise.
//
// \param orig is the ray origin
// \param dir is the ray direction
// \param objects is the list of objects the scene contains
// \param[out] tNear contains the distance to the cloesest intersected object.
// \param[out] index stores the index of the intersect triangle if the interesected object is a mesh.
// \param[out] uv stores the u and v barycentric coordinates of the intersected point
// \param[out] *hitObject stores the pointer to the intersected object (used to retrieve material information, etc.)
// \param isShadowRay is it a shadow ray. We can return from the function sooner as soon as we have found a hit.
// [/comment]
std::optional<hit_payload> trace(
const Vector3f &orig, const Vector3f &dir,
const std::vector<std::unique_ptr<Object> > &objects)
{
float tNear = kInfinity; //用于判断和哪一个物体先相交。
std::optional<hit_payload> payload;
for (const auto & object : objects)//遍历场景中存在的所有物体
{
float tNearK = kInfinity;
uint32_t indexK;
Vector2f uvK;
if (object->intersect(orig, dir, tNearK, indexK, uvK) && tNearK < tNear)
{
payload.emplace();
payload->hit_obj = object.get();
payload->tNear = tNearK;
payload->index = indexK;
payload->uv = uvK;
tNear = tNearK;
}
}
return payload;
}
// [comment]
// Implementation of the Whitted-style light transport algorithm (E [S*] (D|G) L)
//
// This function is the function that compute the color at the intersection point
// of a ray defined by a position and a direction. Note that thus function is recursive (it calls itself).
//
// If the material of the intersected object is either reflective or reflective and refractive,
// then we compute the reflection/refraction direction and cast two new rays into the scene
// by calling the castRay() function recursively. When the surface is transparent, we mix
// the reflection and refraction color using the result of the fresnel equations (it computes
// the amount of reflection and refraction depending on the surface normal, incident view direction
// and surface refractive index).
//
// If the surface is diffuse/glossy we use the Phong illumation model to compute the color
// at the intersection point.
// [/comment]
Vector3f castRay(
const Vector3f &orig, const Vector3f &dir, const Scene& scene,
int depth)
{
if (depth > scene.maxDepth) {
return Vector3f(0.0,0.0,0.0);
}
Vector3f hitColor = scene.backgroundColor;
if (auto payload = trace(orig, dir, scene.get_objects()); payload)
{
Vector3f hitPoint = orig + dir * payload->tNear;
Vector3f N; // normal
Vector2f st; // st coordinates
payload->hit_obj->getSurfaceProperties(hitPoint, dir, payload->index, payload->uv, N, st);
switch (payload->hit_obj->materialType) {
case REFLECTION_AND_REFRACTION:
{
Vector3f reflectionDirection = normalize(reflect(dir, N));
Vector3f refractionDirection = normalize(refract(dir, N, payload->hit_obj->ior));
Vector3f reflectionRayOrig = (dotProduct(reflectionDirection, N) < 0) ?
hitPoint - N * scene.epsilon :
hitPoint + N * scene.epsilon;
Vector3f refractionRayOrig = (dotProduct(refractionDirection, N) < 0) ?
hitPoint - N * scene.epsilon :
hitPoint + N * scene.epsilon;
Vector3f reflectionColor = castRay(reflectionRayOrig, reflectionDirection, scene, depth + 1);
Vector3f refractionColor = castRay(refractionRayOrig, refractionDirection, scene, depth + 1);
float kr = fresnel(dir, N, payload->hit_obj->ior);
hitColor = reflectionColor * kr + refractionColor * (1 - kr);
break;
}
case REFLECTION:
{
float kr = fresnel(dir, N, payload->hit_obj->ior);
Vector3f reflectionDirection = reflect(dir, N);
Vector3f reflectionRayOrig = (dotProduct(reflectionDirection, N) < 0) ?
hitPoint + N * scene.epsilon :
hitPoint - N * scene.epsilon;
hitColor = castRay(reflectionRayOrig, reflectionDirection, scene, depth + 1) * kr;
break;
}
default:
{
// [comment]
// We use the Phong illumation model int the default case. The phong model
// is composed of a diffuse and a specular reflection component.
// [/comment]
Vector3f lightAmt = 0, specularColor = 0;
//?????????????这个是干什么的
Vector3f shadowPointOrig = (dotProduct(dir, N) < 0) ?
hitPoint + N * scene.epsilon :
hitPoint - N * scene.epsilon;
// [comment]
// Loop over all lights in the scene and sum their contribution up
// We also apply the lambert cosine law
// [/comment]
for (auto& light : scene.get_lights()) {
Vector3f lightDir = light->position - hitPoint;
// square of the distance between hitPoint and the light
float lightDistance2 = dotProduct(lightDir, lightDir);
lightDir = normalize(lightDir);
float LdotN = std::max(0.f, dotProduct(lightDir, N));
// is the point in shadow, and is the nearest occluding object closer to the object than the light itself?
auto shadow_res = trace(shadowPointOrig, lightDir, scene.get_objects());
bool inShadow = shadow_res && (shadow_res->tNear * shadow_res->tNear < lightDistance2);
lightAmt += inShadow ? 0 : light->intensity * LdotN;
Vector3f reflectionDirection = reflect(-lightDir, N);
specularColor += powf(std::max(0.f, -dotProduct(reflectionDirection, dir)),
payload->hit_obj->specularExponent) * light->intensity;
}
hitColor = lightAmt * payload->hit_obj->evalDiffuseColor(st) * payload->hit_obj->Kd + specularColor * payload->hit_obj->Ks;
break;
}
}
}
return hitColor;
}
// [comment]
// The main render function. This where we iterate over all pixels in the image, generate
// primary rays and cast these rays into the scene. The content of the framebuffer is
// saved to a file.
// [/comment]
void Renderer::Render(const Scene& scene)
{
std::vector<Vector3f> framebuffer(scene.width * scene.height);
float scale = std::tan(deg2rad(scene.fov * 0.5f));
float imageAspectRatio = scene.width / (float)scene.height;
// Use this variable as the eye position to start your rays.
Vector3f eye_pos(0);
int m = 0;
for (int j = 0; j < scene.height; ++j)
{
for (int i = 0; i < scene.width; ++i)
{
// generate primary ray direction
float x;
float y;
// TODO: Find the x and y positions of the current pixel to get the direction
// vector that passes through it.
// Also, don't forget to multiply both of them with the variable *scale*, and
// x (horizontal) variable with the *imageAspectRatio*
x = (2 * ((float)i + 0.5f) / (float)scene.width - 1) * imageAspectRatio * scale;
y = (1 - 2 * ((float)j + 0.5f) / (float)scene.height) * scale;
Vector3f dir = Vector3f(x, y, -1); // Don't forget to normalize this direction!
dir = normalize(dir);
framebuffer[m++] = castRay(eye_pos, dir, scene, 0);
}
UpdateProgress(j / (float)scene.height);
}
// save framebuffer to file
FILE* fp = fopen("binary.ppm", "wb");
(void)fprintf(fp, "P6\n%d %d\n255\n", scene.width, scene.height);
for (auto i = 0; i < scene.height * scene.width; ++i) {
static unsigned char color[3];
color[0] = (char)(255 * clamp(0, 1, framebuffer[i].x));
color[1] = (char)(255 * clamp(0, 1, framebuffer[i].y));
color[2] = (char)(255 * clamp(0, 1, framebuffer[i].z));
fwrite(color, 1, 3, fp);
}
fclose(fp);
}
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