213 lines
No EOL
6 KiB
GLSL
213 lines
No EOL
6 KiB
GLSL
#include "../math/const.glsl"
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#include "../math/saturate.glsl"
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// Stars deps
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#include "../math/mod2.glsl"
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#include "../math/rotate3dX.glsl"
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#include "../math/rotate3dZ.glsl"
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#include "../space/cart2polar.glsl"
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#include "../color/space/k2rgb.glsl"
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#include "../generative/random.glsl"
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#include "ray.glsl"
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#include "common/rayleigh.glsl"
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#include "common/henyeyGreenstein.glsl"
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/*
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contributor: Patricio Gonzalez Vivo
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description: |
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Rayleigh and Mie scattering atmosphere system.
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Based on:
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- ["Accurate Atmospheric Scattering" from GPU Gems2](https://developer.nvidia.com/gpugems/GPUGems2/gpugems2_chapter16.html)
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- [Alan Zucconi's Atmospheric Scattering articles](https://www.alanzucconi.com/2017/10/10/atmospheric-scattering-6/)
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- [Dimas Leenman atmosphere.glsl](https://github.com/Dimev/atmospheric-scattering-explained)
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- [Simulating the Colors of the Sky](https://www.scratchapixel.com/lessons/procedural-generation-virtual-worlds/simulating-sky/simulating-colors-of-the-sky.html)
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- [License CC0: Stars and galaxy by mrange](https://www.shadertoy.com/view/stBcW1)
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use: <vec3> atmosphere(<vec3> eye_dir, <vec3> sun_dir)
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OPTIONS:
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ATMOSPHERE_ORIGIN: Defualt vec3(0.0)
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ATMOSPHERE_SUN_POWER: sun power. Default 20.0
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ATMOSPHERE_LIGHT_SAMPLES: Defualt 8
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ATMOSPHERE_SAMPLES: Defualt 16
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ATMOSPHERE_GROUND: Example vec3( 0.37, 0.35, 0.34 )
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ATMOSPHERE_STARS_LAYERS: Example 3
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ATMOSPHERE_STARS_ELEVATION: Example u_time * 0.01
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ATMOSPHERE_STARS_AZIMUTH: Example u_time * 0.05
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examples:
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- /shaders/lighting_atmosphere.frag
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*/
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#ifndef ATMOSPHERE_ORIGIN
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#define ATMOSPHERE_ORIGIN vec3(0.0)
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#endif
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#ifndef ATMOSPHERE_SUN_POWER
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#define ATMOSPHERE_SUN_POWER 20.0
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#endif
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#ifndef ATMOSPHERE_RAY
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#define ATMOSPHERE_RAY vec3(55e-7, 13e-6, 22e-6)
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#endif
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#ifndef ATMOSPHERE_MIE
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#define ATMOSPHERE_MIE vec3(21e-6)
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#endif
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#ifndef ATMOSPHERE_LIGHT_SAMPLES
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#define ATMOSPHERE_LIGHT_SAMPLES 8
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#endif
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#ifndef ATMOSPHERE_SAMPLES
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#define ATMOSPHERE_SAMPLES 16
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#endif
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#ifndef FNC_ATMOSPHERE
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#define FNC_ATMOSPHERE
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bool atmosphere_intersect(Ray ray, inout float t0, inout float t1) {
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vec3 L = ATMOSPHERE_ORIGIN - ray.origin;
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float DT = dot(L, ray.direction);
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float D2 = dot(L, L) - DT * DT;
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const float R2 = 412164e8;
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if (D2 > R2)
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return false;
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float AT = sqrt(R2 - D2);
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t0 = DT - AT;
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t1 = DT + AT;
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return true;
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}
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vec3 atmosphere_pos(Ray ray, float dist, float ds) {
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return ray.origin + ray.direction * (dist + ds * 0.5);
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}
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float atmosphere_height(Ray ray, float dist, float ds, inout vec2 density) {
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vec3 p = atmosphere_pos(ray, dist, ds);
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float h = length(p) - 6371e3;
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#ifdef ATMOSPHERE_GROUND
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if (h <= 0.0)
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return 0.0;
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#endif
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density += exp(-h * vec2(125e-6, 833e-6)) * ds; // Rayleigh
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return h;
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}
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bool atmosphere_light(Ray ray, inout vec2 depth) {
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float t0 = 0.0; // Atmosphere entry point
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float t1 = 99999.0; // Atmosphere exit point
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#ifdef ATMOSPHERE_GROUND
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if (!atmosphere_intersect(ray, t0, t1))
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return false;
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#endif
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float dist = 0.;
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float dstep = t1 / float(ATMOSPHERE_LIGHT_SAMPLES);
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for (int i = 0; i < ATMOSPHERE_LIGHT_SAMPLES; i++) {
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if (atmosphere_height(ray, dist, dstep, depth) <= 0.0)
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return false;
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dist += dstep;
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}
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return true;
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}
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vec3 atmosphere(Ray ray, vec3 sun_dir) {
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float t0 = 0.0;
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float t1 = 99999.0;
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#ifdef ATMOSPHERE_GROUND
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if (!atmosphere_intersect(ray, t0, t1))
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return vec3(0.0);
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#endif
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float dstep = t1 / float(ATMOSPHERE_SAMPLES);
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vec2 depth = vec2(0.0);
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vec3 sumR = vec3(0.0, 0.0, 0.0);
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vec3 sumM = vec3(0.0, 0.0, 0.0);
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float dist = 0.0;
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for (int i = 0; i < ATMOSPHERE_SAMPLES; i++) {
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vec2 density = vec2(0.);
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#ifdef ATMOSPHERE_GROUND
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if (atmosphere_height(ray, dist, dstep, density) <= 0.0)
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return ATMOSPHERE_GROUND * sun_dir.y;
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#else
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atmosphere_height(ray, dist, dstep, density);
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#endif
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depth += density;
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vec2 light = vec2(0.);
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if ( atmosphere_light(Ray(atmosphere_pos(ray, dist, dstep), sun_dir), light) ) {
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vec3 attn = exp(-ATMOSPHERE_RAY * (depth.x + light.x)
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-ATMOSPHERE_MIE * (depth.y + light.y));
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sumR += density.x * attn;
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sumM += density.y * attn;
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}
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dist += dstep;
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}
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float mu = dot(ray.direction, sun_dir);
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sumR *= rayleigh(mu) * ATMOSPHERE_RAY;
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sumM *= henyeyGreenstein(mu) * ATMOSPHERE_MIE;
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vec3 color = ATMOSPHERE_SUN_POWER * (sumR + sumM);
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// Draw stars
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#ifdef ATMOSPHERE_STARS_LAYERS
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const float m = float(ATMOSPHERE_STARS_LAYERS);
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float hh = 1.0-saturate(sun_dir.y);
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hh *= hh;
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hh *= hh * hh * hh;
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vec3 dir = ray.direction;
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#ifdef ATMOSPHERE_GROUND
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hh *= step(0.0, dir.y);
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#endif
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#ifdef ATMOSPHERE_STARS_ELEVATION
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dir = rotate3dX(ATMOSPHERE_STARS_ELEVATION) * dir;
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#endif
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#ifdef ATMOSPHERE_STARS_AZIMUTH
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dir = rotate3dZ(ATMOSPHERE_STARS_AZIMUTH) * dir;
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#endif
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vec2 sp = cart2polar(dir.xzy).yz;
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for (float i = 0.0; i < m; ++i) {
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vec2 pp = sp + 0.5 * i;
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float s = i / (m-1.0);
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float dim = mix(0.05, 0.003, s) * PI;
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vec2 np = mod2(pp, dim);
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vec2 h = random2(np + 127.0 + i);
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vec2 o = -1.0+2.0*h;
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float y = sin(sp.x);
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pp += o * dim * 0.5;
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pp.y *= y;
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float l = length(pp);
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float h1 = fract(h.x * 1667.0);
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float h2 = fract(h.x * 1887.0);
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float h3 = fract(h.x * 2997.0);
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vec3 scol = mix(8.0 * h2, 0.25 * h2 * h2, s) * k2rgb(mix(3000.0, 22000.0, h1 * h1));
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vec3 ccol = color + exp(-(mix(6000.0, 2000.0, hh) / mix(2.0, 0.25, s)) * max(l-0.001, 0.0)) * scol * hh;
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color = h3 < y ? ccol : color;
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}
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#endif
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return color;
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}
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vec3 atmosphere(vec3 eye_dir, vec3 sun_dir) {
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Ray ray = Ray(vec3(0., 6371e3 + 1.0, 0.), eye_dir);
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return atmosphere(ray, sun_dir);
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}
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#endif |