Raytracer

PPM

First line tells that each pixel is 3 units long Second line informs about the number of columns and rows Third line tells the max value each param can take Rest are pixel info

Vec3 Class

Contains three variables x,y,z

#include<iostream>

#include<cmath>

#define _VEC3 VEC3

class VEC3{

    public:

        VEC3(){}

        VEC3(float x1, float y1, float z1){x = x1; y=y1; z=z1;}

        float x,y,z;

        VEC3 operator-(){return VEC3(-x, -y, -z);}

        VEC3 operator+(){return *this;}

        VEC3& operator+=(VEC3& v2);

        VEC3& operator-=(VEC3& v2);

        VEC3& operator*=(VEC3& v2);

        VEC3& operator/=(VEC3& v2);

        VEC3& operator+=(const float f2);

        VEC3& operator-=(const float f2);

        VEC3& operator*=(const float f2);

        VEC3& operator/=(const float f2);

  

        float operator[](int i){

            if(i==0) return x;

            if(i==1) return y;

            if(i==2) return z;

        }

  

        void normalize();

        float magnitude();

};

  
  

float dot(VEC3& v1, VEC3& v2);

VEC3 cross(VEC3& v1, VEC3& v2);

  

std::ostream& operator<<(std::ostream& ost, VEC3 v);

  

std::istream& operator>>(std::istream& ist, VEC3 v);

  

VEC3 operator+(VEC3& v1, VEC3& v2);

VEC3 operator-(VEC3& v1, VEC3& v2);

VEC3 operator*(VEC3& v1, VEC3& v2);

VEC3 operator/(VEC3& v1, VEC3& v2);

VEC3 operator+(VEC3& v1, float& f2);

VEC3 operator-(VEC3& v1, float& f2);

VEC3 operator*(VEC3& v1, float& f2);

VEC3 operator/(VEC3& v1, float& f2);

**After we define vector class, we can utilize it in making ppm files

#ifndef _VEC3

    #include "vec3.h"

#endif

  

#include<fstream>

using namespace std;

int main(){

  

    fstream ppm;

    ppm.open("img.ppm", ios::out);

  

    ppm << "P3\n200 200\n 255\n";

    int row  = 200;

    int col = 200;

    float max = 255.0f;

    VEC3 color;

  

    for(int i=row-1; i>=0; i--){

        for(int j=0; j<col; j++){

            color = VEC3(float(j)/col, float(i)/row, 0.2f);

            color*=255.99f;

            ppm << color << "\n";

        }

    }

   return 0;  

}

Rays, a simple camera, and background

Computation of colors in a raytracer happens along the direction of a ray. Function of the ray, let p(t) = A + t*B, p is any 3D position along the ray. A is the starting point of the ray and B is the direction of the ray.

Every raytracer has a color(ray) function that interpolates the colors across the screen.

Adding DEM Spheres

Equation of a spehere centered at origin with radius R, is x*x + y*y + z*z = R*r Same sphere, if located at center (cx, cy, cz) (x-cx)(x-cx) + (y-cy)(y-cy)+ (z-cz)(z-cz)

The same thing in vector form becomes, Taking P = (x,y,z) C = (cx, cy, cz) and dot(P-C, P-C) has the value (x-cx)(x-cx) + (y-cy)(y-cy)+ (z-cz)(z-cz) which is equal to R*R

Therefore the equation of a sphere in Vector form is dot(P-C,P-C) = R*R

Instead of P, we use our ray as P(t) and check where and all the above equation becomes true

Expanding the above formula with P(t) = A + B*t

we get (A+B*t-C)(A+B*t-C) = (A-C)(A-C) + 2*(A-C)*B*t + (B*B)t*t - R*R = 0 which is a quadratic in t, therefore easily solvable

But you ask, what about DEM NORMALS??

Normal is a vector that is perpendicular to the surface and by convention points out. For spheres specifically normals point outwards from hitpoint, in the direction of center, so if P is point and C is the center then, P-C is the normal

rec.N = rec.P - this->center;
rec.N.normalize();

Anti Aliasing

It is the process of reducing the jaggedness around the edges of a color change, mostly done by averaging a bunch of samples inside a pixel and by putting the color of pixel equal to the average. For our general purpose raytracers stratification is not critical. We make use of a random number generator to average out the samples, with the number of samples per pixel as 100(say).

abhiraj2/raytracer

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