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/**
* Precomputed Atmospheric Scattering
* Copyright (c) 2008 INRIA
* All rights reserved.
*
* Redistribution and use in source and binary forms, with or without
* modification, are permitted provided that the following conditions
* are met:
* 1. Redistributions of source code must retain the above copyright
* notice, this list of conditions and the following disclaimer.
* 2. Redistributions in binary form must reproduce the above copyright
* notice, this list of conditions and the following disclaimer in the
* documentation and/or other materials provided with the distribution.
* 3. Neither the name of the copyright holders nor the names of its
* contributors may be used to endorse or promote products derived from
* this software without specific prior written permission.
*
* THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS "AS IS"
* AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE
* IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE
* ARE DISCLAIMED. IN NO EVENT SHALL THE COPYRIGHT OWNER OR CONTRIBUTORS BE
* LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR
* CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF
* SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS
* INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN
* CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE)
* ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF
* THE POSSIBILITY OF SUCH DAMAGE.
*/
/**
* Author: Eric Bruneton
*/
const float SUN_INTENSITY = 100.0;
const vec3 earthPos = vec3(0.0, 0.0, 6360010.0);
// ----------------------------------------------------------------------------
// PHYSICAL MODEL PARAMETERS
// ----------------------------------------------------------------------------
const float SCALE = 1000.0;
const float Rg = 6360.0 * SCALE;
const float Rt = 6420.0 * SCALE;
const float RL = 6421.0 * SCALE;
const float AVERAGE_GROUND_REFLECTANCE = 0.1;
// Rayleigh
const float HR = 8.0 * SCALE;
const vec3 betaR = vec3(5.8e-3, 1.35e-2, 3.31e-2) / SCALE;
// Mie
// DEFAULT
const float HM = 1.2 * SCALE;
const vec3 betaMSca = vec3(4e-3) / SCALE;
const vec3 betaMEx = betaMSca / 0.9;
const float mieG = 0.8;
// CLEAR SKY
/*const float HM = 1.2 * SCALE;
const vec3 betaMSca = vec3(20e-3) / SCALE;
const vec3 betaMEx = betaMSca / 0.9;
const float mieG = 0.76;*/
// PARTLY CLOUDY
/*const float HM = 3.0 * SCALE;
const vec3 betaMSca = vec3(3e-3) / SCALE;
const vec3 betaMEx = betaMSca / 0.9;
const float mieG = 0.65;*/
const float g = 9.81;
const float M_PI = 3.141592657;
// ----------------------------------------------------------------------------
// NUMERICAL INTEGRATION PARAMETERS
// ----------------------------------------------------------------------------
const int TRANSMITTANCE_INTEGRAL_SAMPLES = 500;
const int INSCATTER_INTEGRAL_SAMPLES = 50;
const int IRRADIANCE_INTEGRAL_SAMPLES = 32;
const int INSCATTER_SPHERICAL_INTEGRAL_SAMPLES = 16;
// ----------------------------------------------------------------------------
// PARAMETERIZATION OPTIONS
// ----------------------------------------------------------------------------
const int TRANSMITTANCE_W = 256;
const int TRANSMITTANCE_H = 64;
const int SKY_W = 64;
const int SKY_H = 16;
const int RES_R = 32;
const int RES_MU = 128;
const int RES_MU_S = 32;
const int RES_NU = 8;
#define TRANSMITTANCE_NON_LINEAR
#define INSCATTER_NON_LINEAR
// ----------------------------------------------------------------------------
// PARAMETERIZATION FUNCTIONS
// ----------------------------------------------------------------------------
#ifdef _FRAGMENT_
uniform sampler2D transmittanceSampler;
uniform sampler2D skyIrradianceSampler;
uniform sampler3D inscatterSampler;
vec2 getTransmittanceUV(float r, float mu) {
float uR, uMu;
#ifdef TRANSMITTANCE_NON_LINEAR
uR = sqrt((r - Rg) / (Rt - Rg));
uMu = atan((mu + 0.15) / (1.0 + 0.15) * tan(1.5)) / 1.5;
#else
uR = (r - Rg) / (Rt - Rg);
uMu = (mu + 0.15) / (1.0 + 0.15);
#endif
return vec2(uMu, uR);
}
void getTransmittanceRMu(out float r, out float muS) {
r = gl_FragCoord.y / float(TRANSMITTANCE_H);
muS = gl_FragCoord.x / float(TRANSMITTANCE_W);
#ifdef TRANSMITTANCE_NON_LINEAR
r = Rg + (r * r) * (Rt - Rg);
muS = -0.15 + tan(1.5 * muS) / tan(1.5) * (1.0 + 0.15);
#else
r = Rg + r * (Rt - Rg);
muS = -0.15 + muS * (1.0 + 0.15);
#endif
}
vec2 getIrradianceUV(float r, float muS) {
float uR = (r - Rg) / (Rt - Rg);
float uMuS = (muS + 0.2) / (1.0 + 0.2);
return vec2(uMuS, uR);
}
void getIrradianceRMuS(out float r, out float muS) {
r = Rg + (gl_FragCoord.y - 0.5) / (float(SKY_H) - 1.0) * (Rt - Rg);
muS = -0.2 + (gl_FragCoord.x - 0.5) / (float(SKY_W) - 1.0) * (1.0 + 0.2);
}
vec4 texture4D(sampler3D table, float r, float mu, float muS, float nu)
{
float H = sqrt(Rt * Rt - Rg * Rg);
float rho = sqrt(r * r - Rg * Rg);
#ifdef INSCATTER_NON_LINEAR
float rmu = r * mu;
float delta = rmu * rmu - r * r + Rg * Rg;
vec4 cst = rmu < 0.0 && delta > 0.0 ? vec4(1.0, 0.0, 0.0, 0.5 - 0.5 / float(RES_MU)) : vec4(-1.0, H * H, H, 0.5 + 0.5 / float(RES_MU));
float uR = 0.5 / float(RES_R) + rho / H * (1.0 - 1.0 / float(RES_R));
float uMu = cst.w + (rmu * cst.x + sqrt(delta + cst.y)) / (rho + cst.z) * (0.5 - 1.0 / float(RES_MU));
// paper formula
//float uMuS = 0.5 / float(RES_MU_S) + max((1.0 - exp(-3.0 * muS - 0.6)) / (1.0 - exp(-3.6)), 0.0) * (1.0 - 1.0 / float(RES_MU_S));
// better formula
float uMuS = 0.5 / float(RES_MU_S) + (atan(max(muS, -0.1975) * tan(1.26 * 1.1)) / 1.1 + (1.0 - 0.26)) * 0.5 * (1.0 - 1.0 / float(RES_MU_S));
#else
float uR = 0.5 / float(RES_R) + rho / H * (1.0 - 1.0 / float(RES_R));
float uMu = 0.5 / float(RES_MU) + (mu + 1.0) / 2.0 * (1.0 - 1.0 / float(RES_MU));
float uMuS = 0.5 / float(RES_MU_S) + max(muS + 0.2, 0.0) / 1.2 * (1.0 - 1.0 / float(RES_MU_S));
#endif
float lerp = (nu + 1.0) / 2.0 * (float(RES_NU) - 1.0);
float uNu = floor(lerp);
lerp = lerp - uNu;
return texture3D(table, vec3((uNu + uMuS) / float(RES_NU), uMu, uR)) * (1.0 - lerp) +
texture3D(table, vec3((uNu + uMuS + 1.0) / float(RES_NU), uMu, uR)) * lerp;
}
void getMuMuSNu(float r, vec4 dhdH, out float mu, out float muS, out float nu) {
float x = gl_FragCoord.x - 0.5;
float y = gl_FragCoord.y - 0.5;
#ifdef INSCATTER_NON_LINEAR
if (y < float(RES_MU) / 2.0) {
float d = 1.0 - y / (float(RES_MU) / 2.0 - 1.0);
d = min(max(dhdH.z, d * dhdH.w), dhdH.w * 0.999);
mu = (Rg * Rg - r * r - d * d) / (2.0 * r * d);
mu = min(mu, -sqrt(1.0 - (Rg / r) * (Rg / r)) - 0.001);
} else {
float d = (y - float(RES_MU) / 2.0) / (float(RES_MU) / 2.0 - 1.0);
d = min(max(dhdH.x, d * dhdH.y), dhdH.y * 0.999);
mu = (Rt * Rt - r * r - d * d) / (2.0 * r * d);
}
muS = mod(x, float(RES_MU_S)) / (float(RES_MU_S) - 1.0);
// paper formula
//muS = -(0.6 + log(1.0 - muS * (1.0 - exp(-3.6)))) / 3.0;
// better formula
muS = tan((2.0 * muS - 1.0 + 0.26) * 1.1) / tan(1.26 * 1.1);
nu = -1.0 + floor(x / float(RES_MU_S)) / (float(RES_NU) - 1.0) * 2.0;
#else
mu = -1.0 + 2.0 * y / (float(RES_MU) - 1.0);
muS = mod(x, float(RES_MU_S)) / (float(RES_MU_S) - 1.0);
muS = -0.2 + muS * 1.2;
nu = -1.0 + floor(x / float(RES_MU_S)) / (float(RES_NU) - 1.0) * 2.0;
#endif
}
// ----------------------------------------------------------------------------
// UTILITY FUNCTIONS
// ----------------------------------------------------------------------------
// nearest intersection of ray r,mu with ground or top atmosphere boundary
// mu=cos(ray zenith angle at ray origin)
float limit(float r, float mu) {
float dout = -r * mu + sqrt(r * r * (mu * mu - 1.0) + RL * RL);
float delta2 = r * r * (mu * mu - 1.0) + Rg * Rg;
if (delta2 >= 0.0) {
float din = -r * mu - sqrt(delta2);
if (din >= 0.0) {
dout = min(dout, din);
}
}
return dout;
}
// optical depth for ray (r,mu) of length d, using analytic formula
// (mu=cos(view zenith angle)), intersections with ground ignored
// H=height scale of exponential density function
float opticalDepth(float H, float r, float mu, float d) {
float a = sqrt((0.5/H)*r);
vec2 a01 = a*vec2(mu, mu + d / r);
vec2 a01s = sign(a01);
vec2 a01sq = a01*a01;
float x = a01s.y > a01s.x ? exp(a01sq.x) : 0.0;
vec2 y = a01s / (2.3193*abs(a01) + sqrt(1.52*a01sq + 4.0)) * vec2(1.0, exp(-d/H*(d/(2.0*r)+mu)));
return sqrt((6.2831*H)*r) * exp((Rg-r)/H) * (x + dot(y, vec2(1.0, -1.0)));
}
// transmittance(=transparency) of atmosphere for infinite ray (r,mu)
// (mu=cos(view zenith angle)), intersections with ground ignored
vec3 transmittance(float r, float mu) {
vec2 uv = getTransmittanceUV(r, mu);
return texture2D(transmittanceSampler, uv).rgb;
}
// transmittance(=transparency) of atmosphere for ray (r,mu) of length d
// (mu=cos(view zenith angle)), intersections with ground ignored
// uses analytic formula instead of transmittance texture
vec3 analyticTransmittance(float r, float mu, float d) {
return exp(- betaR * opticalDepth(HR, r, mu, d) - betaMEx * opticalDepth(HM, r, mu, d));
}
// transmittance(=transparency) of atmosphere for infinite ray (r,mu)
// (mu=cos(view zenith angle)), or zero if ray intersects ground
vec3 transmittanceWithShadow(float r, float mu) {
return mu < -sqrt(1.0 - (Rg / r) * (Rg / r)) ? vec3(0.0) : transmittance(r, mu);
}
// transmittance(=transparency) of atmosphere between x and x0
// assume segment x,x0 not intersecting ground
// r=||x||, mu=cos(zenith angle of [x,x0) ray at x), v=unit direction vector of [x,x0) ray
vec3 transmittance(float r, float mu, vec3 v, vec3 x0) {
vec3 result;
float r1 = length(x0);
float mu1 = dot(x0, v) / r;
if (mu > 0.0) {
result = min(transmittance(r, mu) / transmittance(r1, mu1), 1.0);
} else {
result = min(transmittance(r1, -mu1) / transmittance(r, -mu), 1.0);
}
return result;
}
// transmittance(=transparency) of atmosphere between x and x0
// assume segment x,x0 not intersecting ground
// d = distance between x and x0, mu=cos(zenith angle of [x,x0) ray at x)
vec3 transmittance(float r, float mu, float d) {
vec3 result;
float r1 = sqrt(r * r + d * d + 2.0 * r * mu * d);
float mu1 = (r * mu + d) / r1;
if (mu > 0.0) {
result = min(transmittance(r, mu) / transmittance(r1, mu1), 1.0);
} else {
result = min(transmittance(r1, -mu1) / transmittance(r, -mu), 1.0);
}
return result;
}
vec3 irradiance(sampler2D sampler, float r, float muS) {
vec2 uv = getIrradianceUV(r, muS);
return texture2D(sampler, uv).rgb;
}
// Rayleigh phase function
float phaseFunctionR(float mu) {
return (3.0 / (16.0 * M_PI)) * (1.0 + mu * mu);
}
// Mie phase function
float phaseFunctionM(float mu) {
return 1.5 * 1.0 / (4.0 * M_PI) * (1.0 - mieG*mieG) * pow(1.0 + (mieG*mieG) - 2.0*mieG*mu, -3.0/2.0) * (1.0 + mu * mu) / (2.0 + mieG*mieG);
}
// approximated single Mie scattering (cf. approximate Cm in paragraph "Angular precision")
vec3 getMie(vec4 rayMie) { // rayMie.rgb=C*, rayMie.w=Cm,r
return rayMie.rgb * rayMie.w / max(rayMie.r, 1e-4) * (betaR.r / betaR);
}
// ----------------------------------------------------------------------------
// PUBLIC FUNCTIONS
// ----------------------------------------------------------------------------
// incident sun light at given position (radiance)
// r=length(x)
// muS=dot(x,s) / r
vec3 sunRadiance(float r, float muS) {
return transmittanceWithShadow(r, muS) * SUN_INTENSITY;
}
// incident sky light at given position, integrated over the hemisphere (irradiance)
// r=length(x)
// muS=dot(x,s) / r
vec3 skyIrradiance(float r, float muS) {
return irradiance(skyIrradianceSampler, r, muS) * SUN_INTENSITY;
}
// scattered sunlight between two points
// camera=observer
// viewdir=unit vector towards observed point
// sundir=unit vector towards the sun
// return scattered light and extinction coefficient
vec3 skyRadiance(vec3 camera, vec3 viewdir, vec3 sundir, out vec3 extinction)
{
vec3 result;
float r = length(camera);
float rMu = dot(camera, viewdir);
float mu = rMu / r;
float r0 = r;
float mu0 = mu;
float deltaSq = sqrt(rMu * rMu - r * r + Rt*Rt);
float din = max(-rMu - deltaSq, 0.0);
if (din > 0.0) {
camera += din * viewdir;
rMu += din;
mu = rMu / Rt;
r = Rt;
}
if (r <= Rt) {
float nu = dot(viewdir, sundir);
float muS = dot(camera, sundir) / r;
vec4 inScatter = texture4D(inscatterSampler, r, rMu / r, muS, nu);
extinction = transmittance(r, mu);
vec3 inScatterM = getMie(inScatter);
float phase = phaseFunctionR(nu);
float phaseM = phaseFunctionM(nu);
result = inScatter.rgb * phase + inScatterM * phaseM;
} else {
result = vec3(0.0);
extinction = vec3(1.0);
}
return result * SUN_INTENSITY;
}
// scattered sunlight between two points
// camera=observer
// point=point on the ground
// sundir=unit vector towards the sun
// return scattered light and extinction coefficient
vec3 inScattering(vec3 camera, vec3 point, vec3 sundir, out vec3 extinction) {
vec3 result;
vec3 viewdir = point - camera;
float d = length(viewdir);
viewdir = viewdir / d;
float r = length(camera);
float rMu = dot(camera, viewdir);
float mu = rMu / r;
float r0 = r;
float mu0 = mu;
float deltaSq = sqrt(rMu * rMu - r * r + Rt*Rt);
float din = max(-rMu - deltaSq, 0.0);
if (din > 0.0) {
camera += din * viewdir;
rMu += din;
mu = rMu / Rt;
r = Rt;
d -= din;
}
if (r <= Rt) {
float nu = dot(viewdir, sundir);
float muS = dot(camera, sundir) / r;
vec4 inScatter;
if (r < Rg + 600.0) {
// avoids imprecision problems in aerial perspective near ground
float f = (Rg + 600.0) / r;
r = r * f;
rMu = rMu * f;
point = point * f;
}
float r1 = length(point);
float rMu1 = dot(point, viewdir);
float mu1 = rMu1 / r1;
float muS1 = dot(point, sundir) / r1;
if (mu > 0.0) {
extinction = min(transmittance(r, mu) / transmittance(r1, mu1), 1.0);
} else {
extinction = min(transmittance(r1, -mu1) / transmittance(r, -mu), 1.0);
}
vec4 inScatter0 = texture4D(inscatterSampler, r, mu, muS, nu);
vec4 inScatter1 = texture4D(inscatterSampler, r1, mu1, muS1, nu);
inScatter = max(inScatter0 - inScatter1 * extinction.rgbr, 0.0);
// avoids imprecision problems in Mie scattering when sun is below horizon
inScatter.w *= smoothstep(0.00, 0.02, muS);
vec3 inScatterM = getMie(inScatter);
float phase = phaseFunctionR(nu);
float phaseM = phaseFunctionM(nu);
result = inScatter.rgb * phase + inScatterM * phaseM;
} else {
result = vec3(0.0);
extinction = vec3(1.0);
}
return result * SUN_INTENSITY;
}
void sunRadianceAndSkyIrradiance(vec3 worldP, vec3 worldS, out vec3 sunL, out vec3 skyE)
{
vec3 worldV = normalize(worldP); // vertical vector
float r = length(worldP);
float muS = dot(worldV, worldS);
sunL = sunRadiance(r, muS);
skyE = skyIrradiance(r, muS);
}
// ----------------------------------------------------------------------------
// SKYMAP AND HDR
// ----------------------------------------------------------------------------
uniform sampler2D skySampler;
uniform float hdrExposure;
vec4 skyRadiance(vec2 u) {
return texture2DLod(skySampler, (u * (0.5 / 1.1) + 0.5), 0.0);
}
vec3 hdr(vec3 L) {
L = L * hdrExposure;
L.r = L.r < 1.413 ? pow(L.r * 0.38317, 1.0 / 2.2) : 1.0 - exp(-L.r);
L.g = L.g < 1.413 ? pow(L.g * 0.38317, 1.0 / 2.2) : 1.0 - exp(-L.g);
L.b = L.b < 1.413 ? pow(L.b * 0.38317, 1.0 / 2.2) : 1.0 - exp(-L.b);
return L;
}
// ----------------------------------------------------------------------------
// CLOUDS
// ----------------------------------------------------------------------------
uniform sampler2D noiseSampler;
uniform float octaves;
uniform float lacunarity;
uniform float gain;
uniform float norm;
uniform float clamp1;
uniform float clamp2;
uniform vec4 cloudsColor;
vec4 cloudColor(vec3 worldP, vec3 worldCamera, vec3 worldSunDir) {
const float a = 23.0 / 180.0 * M_PI;
mat2 m = mat2(cos(a), sin(a), -sin(a), cos(a));
vec2 st = worldP.xy / 1000000.0;
float g = 1.0;
float r = 0.0;
for (float i = 0.0; i < octaves; i += 1.0) {
r -= g * (2.0 * texture2D(noiseSampler, st).r - 1.0);
st = (m * st) * lacunarity;
g *= gain;
}
float v = clamp((r * norm - clamp1) / (clamp2 - clamp1), 0.0, 1.0);
float t = clamp((r * norm * 3.0 - clamp1) / (clamp2 - clamp1), 0.0, 1.0);
vec3 PP = worldP + earthPos;
vec3 Lsun;
vec3 Esky;
vec3 extinction;
sunRadianceAndSkyIrradiance(PP, worldSunDir, Lsun, Esky);
vec3 cloudL = v * (Lsun * max(worldSunDir.z, 0.0) + Esky / 10.0) / M_PI;
vec3 inscatter = inScattering(worldCamera + earthPos, PP, worldSunDir, extinction);
cloudL = cloudL * extinction + inscatter;
return vec4(cloudL, t) * cloudsColor;
}
vec4 cloudColorV(vec3 worldCamera, vec3 V, vec3 worldSunDir) {
vec3 P = worldCamera + V * (3000.0 - worldCamera.z) / V.z;
return cloudColor(P, worldCamera, worldSunDir);
}
#endif
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