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fgdata/Shaders/HDR/atmos-include.frag

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#version 330 core
const float PI = 3.14159265358979323846;
const float INV_PI = 0.31830988618379067154;
const float INV_4PI = 0.25 * INV_PI;
const float PHASE_ISOTROPIC = INV_4PI;
const float RAYLEIGH_PHASE_SCALE = (3.0 / 16.0) * INV_PI;
const float g = 0.8;
const float gg = g*g;
const float ATMOSPHERE_RADIUS = 6471e3;
// Rayleigh scattering coefficient at sea level, units m^-1
// "Rayleigh-scattering calculations for the terrestrial atmosphere"
// by Anthony Bucholtz (1995).
const vec4 molecular_scattering_coefficient_base =
vec4(6.605e-6, 1.067e-5, 1.842e-5, 3.156e-5);
// Ozone absorption cross section, units m^2 / molecules
// "High spectral resolution ozone absorption cross-sections"
// by V. Gorshelev et al. (2014).
const vec4 ozone_cross_section =
vec4(3.472e-21, 3.914e-21, 1.349e-21, 11.03e-23) * 1e-4f;
const float ozone_mean_monthly_dobson[] = float[](
347.0, // January
370.0, // February
381.0, // March
384.0, // April
372.0, // May
352.0, // June
333.0, // July
317.0, // August
298.0, // September
285.0, // October
290.0, // November
315.0 // December
);
const float ozone_height_distribution[] = float[](
9.0 / 210.0,
14.0 / 210.0,
111.0 / 210.0,
64.0 / 210.0,
6.0 / 210.0,
6.0 / 210.0,
0.0
);
/*
* Every aerosol type expects 5 parameters:
* - Scattering cross section
* - Absorption cross section
* - Base density (km^-3)
* - Background density (km^-3)
* - Height scaling parameter
* These parameters can be sent as uniforms.
*
* This model for aerosols and their corresponding parameters come from
* "A Physically-Based Spatio-Temporal Sky Model"
* by Guimera et al. (2018).
*/
// Urban
uniform vec4 aerosol_absorption_cross_section =
vec4(2.8722e-24, 4.6168e-24, 7.9706e-24, 1.3578e-23);
uniform vec4 aerosol_scattering_cross_section =
vec4(1.5908e-22, 1.7711e-22, 2.0942e-22, 2.4033e-22);
uniform float aerosol_base_density = 1.3681e20;
uniform float aerosol_relative_background_density = 2e6 / 1.3681e20;
uniform float aerosol_height_scale = 0.73;
uniform float aerosol_turbidity = 1.0;
uniform int month_of_the_year = 0;
uniform vec4 ground_albedo = vec4(0.3);
uniform float fg_EarthRadius;
//------------------------------------------------------------------------------
/*
* Helper function to obtain the transmittance to the top of the atmosphere
* from Buffer A.
*/
vec4 transmittance_from_lut(sampler2D lut, float cos_theta, float normalized_altitude)
{
float u = clamp(cos_theta * 0.5 + 0.5, 0.0, 1.0);
float v = clamp(normalized_altitude, 0.0, 1.0);
return texture(lut, vec2(u, v));
}
/*
* Returns the distance between ro and the first intersection with the sphere
* or -1.0 if there is no intersection. The sphere's origin is (0,0,0).
* -1.0 is also returned if the ray is pointing away from the sphere.
*/
float ray_sphere_intersection(vec3 ro, vec3 rd, float radius)
{
float b = dot(ro, rd);
float c = dot(ro, ro) - radius*radius;
if (c > 0.0 && b > 0.0) return -1.0;
float d = b*b - c;
if (d < 0.0) return -1.0;
if (d > b*b) return (-b+sqrt(d));
return (-b-sqrt(d));
}
/*
* Rayleigh phase function.
*/
float molecular_phase_function(float cos_theta)
{
return RAYLEIGH_PHASE_SCALE * (1.0 + cos_theta*cos_theta);
}
/*
* Henyey-Greenstrein phase function.
*/
float aerosol_phase_function(float cos_theta)
{
float den = 1.0 + gg + 2.0 * g * cos_theta;
return INV_4PI * (1.0 - gg) / (den * sqrt(den));
}
/*
* Get the approximated multiple scattering contribution for a given point
* within the atmosphere.
*/
vec4 get_multiple_scattering(sampler2D transmittance_lut,
float cos_theta,
float normalized_height,
float d)
{
// Solid angle subtended by the planet from a point at d distance
// from the planet center.
float omega = 2.0 * PI * (1.0 - sqrt(d*d - fg_EarthRadius*fg_EarthRadius) / d);
omega = max(0.0, omega);
vec4 T_to_ground = transmittance_from_lut(transmittance_lut, cos_theta, 0.0);
vec4 T_ground_to_sample =
transmittance_from_lut(transmittance_lut, 1.0, 0.0) /
transmittance_from_lut(transmittance_lut, 1.0, normalized_height);
// 2nd order scattering from the ground
vec4 L_ground = PHASE_ISOTROPIC * omega * (ground_albedo * INV_PI)
* T_to_ground * T_ground_to_sample * max(0.0, cos_theta);
// Fit of Earth's multiple scattering coming from other points in the atmosphere
vec4 L_ms = 0.02 * vec4(0.217, 0.347, 0.594, 1.0)
* (1.0 / (1.0 + 5.0 * exp(-17.92 * cos_theta)));
return L_ms + L_ground;
}
/*
* Return the molecular volume scattering coefficient (m^-1) for a given altitude
* in kilometers.
*/
vec4 get_molecular_scattering_coefficient(float h)
{
return molecular_scattering_coefficient_base
* exp(-0.07771971 * pow(h, 1.16364243));
}
/*
* Return the molecular volume absorption coefficient (km^-1) for a given altitude
* in kilometers.
*/
vec4 get_molecular_absorption_coefficient(float h)
{
int i = int(clamp(h / 9.0, 0.0, 6.0));
float density = ozone_height_distribution[i] *
ozone_mean_monthly_dobson[month_of_the_year] * 2.6867e20f; // molecules / m^2
density /= 9e3; // m^-3
return ozone_cross_section * density; // m^-1
}
/*
* Return the aerosol density for a given altitude in kilometers.
*/
float get_aerosol_density(float h)
{
return aerosol_base_density * (exp(-h / aerosol_height_scale)
+ aerosol_relative_background_density);
}
/*
* Get the collision coefficients (scattering and absorption) of the
* atmospheric medium for a given point at an altitude h.
*/
void get_atmosphere_collision_coefficients(in float h,
out vec4 aerosol_absorption,
out vec4 aerosol_scattering,
out vec4 molecular_absorption,
out vec4 molecular_scattering,
out vec4 extinction)
{
h = max(h, 0.0); // In case height is negative
float aerosol_density = get_aerosol_density(h * 1e-3) * aerosol_turbidity;
aerosol_absorption = aerosol_absorption_cross_section * aerosol_density * 1e-3;
aerosol_scattering = aerosol_scattering_cross_section * aerosol_density * 1e-3;
molecular_absorption = get_molecular_absorption_coefficient(h * 1e-3);
molecular_scattering = get_molecular_scattering_coefficient(h * 1e-3);
extinction =
aerosol_absorption + aerosol_scattering +
molecular_absorption + molecular_scattering;
}
/*
* Compute the in-scattering integral of the volume rendering equation (VRE)
*
* The integral is solved numerically by ray marching. The final in-scattering
* returned by this function is a 4D vector of the spectral radiance sampled for
* the 4 wavelengths at the top of this file. To obtain an RGB triplet, the
* spectral radiance must be multiplied by the spectral irradiance of the Sun
* and converted to sRGB.
*/
vec4 compute_inscattering(in vec3 ray_origin,
in vec3 ray_dir,
in float t_max,
in vec3 sun_dir,
in int steps,
in sampler2D transmittance_lut,
out vec4 transmittance)
{
// Any given ray inside the atmospheric medium can end in one of 3 places:
// 1. The Earth's surface.
// 2. Outer space. We define the boundary between space and the atmosphere
// at the Kármán line.
// 3. Any object within the atmosphere.
float ray_altitude = length(ray_origin);
// Handle the camera being underground
float earth_radius = min(ray_altitude, fg_EarthRadius);
float atmos_dist = ray_sphere_intersection(ray_origin, ray_dir, ATMOSPHERE_RADIUS);
float ground_dist = ray_sphere_intersection(ray_origin, ray_dir, earth_radius);
float t_d;
if (ray_altitude < ATMOSPHERE_RADIUS) {
// We are inside the atmosphere
if (ground_dist < 0.0) {
// No ground collision, use the distance to the outer atmosphere
t_d = atmos_dist;
} else {
// We have a collision with the ground, use the distance to it
t_d = ground_dist;
}
} else {
// We are in outer space
// XXX: For now this is a flight simulator, not a space simulator
transmittance = vec4(1.0);
return vec4(0.0);
}
// Clip by the maximum distance
t_d = min(t_d, t_max);
float cos_theta = dot(-ray_dir, sun_dir);
float molecular_phase = molecular_phase_function(cos_theta);
float aerosol_phase = aerosol_phase_function(cos_theta);
float dt = t_d / float(steps);
vec4 L_inscattering = vec4(0.0);
transmittance = vec4(1.0);
for (int i = 0; i < steps; ++i) {
float t = (float(i) + 0.5) * dt;
vec3 x_t = ray_origin + ray_dir * t;
float distance_to_earth_center = length(x_t);
vec3 zenith_dir = x_t / distance_to_earth_center;
float altitude = distance_to_earth_center - fg_EarthRadius;
float normalized_altitude = altitude / (ATMOSPHERE_RADIUS - fg_EarthRadius);
float sample_cos_theta = dot(zenith_dir, sun_dir);
vec4 aerosol_absorption, aerosol_scattering;
vec4 molecular_absorption, molecular_scattering;
vec4 extinction;
get_atmosphere_collision_coefficients(
altitude,
aerosol_absorption, aerosol_scattering,
molecular_absorption, molecular_scattering,
extinction);
vec4 transmittance_to_sun = transmittance_from_lut(
transmittance_lut, sample_cos_theta, normalized_altitude);
vec4 ms = get_multiple_scattering(
transmittance_lut, sample_cos_theta, normalized_altitude,
distance_to_earth_center);
vec4 S =
molecular_scattering * (molecular_phase * transmittance_to_sun + ms) +
aerosol_scattering * (aerosol_phase * transmittance_to_sun + ms);
vec4 step_transmittance = exp(-dt * extinction);
// Energy-conserving analytical integration
// "Physically Based Sky, Atmosphere and Cloud Rendering in Frostbite"
// by Sébastien Hillaire
vec4 S_int = (S - S * step_transmittance) / max(extinction, 1e-7);
L_inscattering += transmittance * S_int;
transmittance *= step_transmittance;
}
return L_inscattering;
}