/* * Copyright 2011-2020 Blender Foundation * * Licensed under the Apache License, Version 2.0 (the "License"); * you may not use this file except in compliance with the License. * You may obtain a copy of the License at * * http://www.apache.org/licenses/LICENSE-2.0 * * Unless required by applicable law or agreed to in writing, software * distributed under the License is distributed on an "AS IS" BASIS, * WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied. * See the License for the specific language governing permissions and * limitations under the License. */ #include "sky_float3.h" #include "sky_model.h" /* Constants */ static const float rayleigh_scale = 8e3f; // Rayleigh scale height (m) static const float mie_scale = 1.2e3f; // Mie scale height (m) static const float mie_coeff = 2e-5f; // Mie scattering coefficient (m^-1) static const float mie_G = 0.76f; // aerosols anisotropy static const float sqr_G = mie_G * mie_G; // squared aerosols anisotropy static const float earth_radius = 6360e3f; // radius of Earth (m) static const float atmosphere_radius = 6420e3f; // radius of atmosphere (m) static const int steps = 32; // segments of primary ray static const int steps_light = 16; // segments of sun connection ray static const int num_wavelengths = 21; // number of wavelengths static const int min_wavelength = 380; // lowest sampled wavelength (nm) static const int max_wavelength = 780; // highest sampled wavelength (nm) // step between each sampled wavelength (nm) static const float step_lambda = (max_wavelength - min_wavelength) / (num_wavelengths - 1); /* Sun irradiance on top of the atmosphere (W*m^-2*nm^-1) */ static const float irradiance[] = { 1.45756829855592995315f, 1.56596305559738380175f, 1.65148449067670455293f, 1.71496242737209314555f, 1.75797983805020541226f, 1.78256407885924539336f, 1.79095108475838560302f, 1.78541550133410664714f, 1.76815554864306845317f, 1.74122069647250410362f, 1.70647127164943679389f, 1.66556087452739887134f, 1.61993437242451854274f, 1.57083597368892080581f, 1.51932335059305478886f, 1.46628494965214395407f, 1.41245852740172450623f, 1.35844961970384092709f, 1.30474913844739281998f, 1.25174963272610817455f, 1.19975998755420620867f}; /* Rayleigh scattering coefficient (m^-1) */ static const float rayleigh_coeff[] = { 0.00005424820087636473f, 0.00004418549866505454f, 0.00003635151910165377f, 0.00003017929012024763f, 0.00002526320226989157f, 0.00002130859310621843f, 0.00001809838025320633f, 0.00001547057129129042f, 0.00001330284977336850f, 0.00001150184784075764f, 0.00000999557429990163f, 0.00000872799973630707f, 0.00000765513700977967f, 0.00000674217203751443f, 0.00000596134125832052f, 0.00000529034598065810f, 0.00000471115687557433f, 0.00000420910481110487f, 0.00000377218381260133f, 0.00000339051255477280f, 0.00000305591531679811f}; /* Ozone absorption coefficient (m^-1) */ static const float ozone_coeff[] = { 0.00000000325126849861f, 0.00000000585395365047f, 0.00000001977191155085f, 0.00000007309568762914f, 0.00000020084561514287f, 0.00000040383958096161f, 0.00000063551335912363f, 0.00000096707041180970f, 0.00000154797400424410f, 0.00000209038647223331f, 0.00000246128056164565f, 0.00000273551299461512f, 0.00000215125863128643f, 0.00000159051840791988f, 0.00000112356197979857f, 0.00000073527551487574f, 0.00000046450130357806f, 0.00000033096079921048f, 0.00000022512612292678f, 0.00000014879129266490f, 0.00000016828623364192f}; /* CIE XYZ color matching functions */ static const float cmf_xyz[][3] = {{0.00136800000f, 0.00003900000f, 0.00645000100f}, {0.01431000000f, 0.00039600000f, 0.06785001000f}, {0.13438000000f, 0.00400000000f, 0.64560000000f}, {0.34828000000f, 0.02300000000f, 1.74706000000f}, {0.29080000000f, 0.06000000000f, 1.66920000000f}, {0.09564000000f, 0.13902000000f, 0.81295010000f}, {0.00490000000f, 0.32300000000f, 0.27200000000f}, {0.06327000000f, 0.71000000000f, 0.07824999000f}, {0.29040000000f, 0.95400000000f, 0.02030000000f}, {0.59450000000f, 0.99500000000f, 0.00390000000f}, {0.91630000000f, 0.87000000000f, 0.00165000100f}, {1.06220000000f, 0.63100000000f, 0.00080000000f}, {0.85444990000f, 0.38100000000f, 0.00019000000f}, {0.44790000000f, 0.17500000000f, 0.00002000000f}, {0.16490000000f, 0.06100000000f, 0.00000000000f}, {0.04677000000f, 0.01700000000f, 0.00000000000f}, {0.01135916000f, 0.00410200000f, 0.00000000000f}, {0.00289932700f, 0.00104700000f, 0.00000000000f}, {0.00069007860f, 0.00024920000f, 0.00000000000f}, {0.00016615050f, 0.00006000000f, 0.00000000000f}, {0.00004150994f, 0.00001499000f, 0.00000000000f}}; static float3 geographical_to_direction(float lat, float lon) { return make_float3(cosf(lat) * cosf(lon), cosf(lat) * sinf(lon), sinf(lat)); } static float3 spec_to_xyz(const float *spectrum) { float3 xyz = make_float3(0.0f, 0.0f, 0.0f); for (int i = 0; i < num_wavelengths; i++) { xyz.x += cmf_xyz[i][0] * spectrum[i]; xyz.y += cmf_xyz[i][1] * spectrum[i]; xyz.z += cmf_xyz[i][2] * spectrum[i]; } return xyz * step_lambda; } /* Atmosphere volume models */ static float density_rayleigh(float height) { return expf(-height / rayleigh_scale); } static float density_mie(float height) { return expf(-height / mie_scale); } static float density_ozone(float height) { float den = 0.0f; if (height >= 10000.0f && height < 25000.0f) { den = 1.0f / 15000.0f * height - 2.0f / 3.0f; } else if (height >= 25000 && height < 40000) { den = -(1.0f / 15000.0f * height - 8.0f / 3.0f); } return den; } static float phase_rayleigh(float mu) { return 3.0f / (16.0f * M_PI_F) * (1.0f + sqr(mu)); } static float phase_mie(float mu) { return (3.0f * (1.0f - sqr_G) * (1.0f + sqr(mu))) / (8.0f * M_PI_F * (2.0f + sqr_G) * powf((1.0f + sqr_G - 2.0f * mie_G * mu), 1.5)); } /* Intersection helpers */ static bool surface_intersection(float3 pos, float3 dir) { if (dir.z >= 0) { return false; } float b = -2.0f * dot(dir, -pos); float c = len_squared(pos) - sqr(earth_radius); float t = b * b - 4.0f * c; if (t >= 0.0f) { return true; } return false; } static float3 atmosphere_intersection(float3 pos, float3 dir) { float b = -2.0f * dot(dir, -pos); float c = len_squared(pos) - sqr(atmosphere_radius); float t = (-b + sqrtf(b * b - 4.0f * c)) / 2.0f; return make_float3(pos.x + dir.x * t, pos.y + dir.y * t, pos.z + dir.z * t); } static float3 ray_optical_depth(float3 ray_origin, float3 ray_dir) { /* this code computes the optical depth along a ray through the atmosphere */ float3 ray_end = atmosphere_intersection(ray_origin, ray_dir); float ray_length = distance(ray_origin, ray_end); /* to compute the optical depth, we step along the ray in segments and * accumulate the optical depth along each segment */ float segment_length = ray_length / steps_light; float3 segment = segment_length * ray_dir; /* instead of tracking the transmission spectrum across all wavelengths directly, * we use the fact that the density always has the same spectrum for each type of * scattering, so we split the density into a constant spectrum and a factor and * only track the factors */ float3 optical_depth = make_float3(0.0f, 0.0f, 0.0f); /* the density of each segment is evaluated at its middle */ float3 P = ray_origin + 0.5f * segment; for (int i = 0; i < steps_light; i++) { /* height above sea level */ float height = len(P) - earth_radius; /* accumulate optical depth of this segment (density is assumed to be constant along it) */ float3 density = make_float3( density_rayleigh(height), density_mie(height), density_ozone(height)); optical_depth += density; /* advance along ray */ P += segment; } return optical_depth * segment_length; } static void single_scattering(float3 ray_dir, float3 sun_dir, float3 ray_origin, float air_density, float dust_density, float ozone_density, float *r_spectrum) { /* this code computes single-inscattering along a ray through the atmosphere */ float3 ray_end = atmosphere_intersection(ray_origin, ray_dir); float ray_length = distance(ray_origin, ray_end); /* to compute the inscattering, we step along the ray in segments and accumulate * the inscattering as well as the optical depth along each segment */ float segment_length = ray_length / steps; float3 segment = segment_length * ray_dir; /* instead of tracking the transmission spectrum across all wavelengths directly, * we use the fact that the density always has the same spectrum for each type of * scattering, so we split the density into a constant spectrum and a factor and * only track the factors */ float3 optical_depth = make_float3(0.0f, 0.0f, 0.0f); /* zero out light accumulation */ for (int wl = 0; wl < num_wavelengths; wl++) { r_spectrum[wl] = 0.0f; } /* phase function for scattering and the density scale factor */ float mu = dot(ray_dir, sun_dir); float3 phase_function = make_float3(phase_rayleigh(mu), phase_mie(mu), 0.0f); float3 density_scale = make_float3(air_density, dust_density, ozone_density); /* the density and in-scattering of each segment is evaluated at its middle */ float3 P = ray_origin + 0.5f * segment; for (int i = 0; i < steps; i++) { /* height above sea level */ float height = len(P) - earth_radius; /* evaluate and accumulate optical depth along the ray */ float3 density = density_scale * make_float3(density_rayleigh(height), density_mie(height), density_ozone(height)); optical_depth += segment_length * density; /* if the Earth isn't in the way, evaluate inscattering from the sun */ if (!surface_intersection(P, sun_dir)) { float3 light_optical_depth = density_scale * ray_optical_depth(P, sun_dir); float3 total_optical_depth = optical_depth + light_optical_depth; /* attenuation of light */ for (int wl = 0; wl < num_wavelengths; wl++) { float3 extinction_density = total_optical_depth * make_float3(rayleigh_coeff[wl], 1.11f * mie_coeff, ozone_coeff[wl]); float attenuation = expf(-reduce_add(extinction_density)); float3 scattering_density = density * make_float3(rayleigh_coeff[wl], mie_coeff, 0.0f); /* the total inscattered radiance from one segment is: * Tr(A<->B) * Tr(B<->C) * sigma_s * phase * L * segment_length * * These terms are: * Tr(A<->B): Transmission from start to scattering position (tracked in optical_depth) * Tr(B<->C): Transmission from scattering position to light (computed in * ray_optical_depth) sigma_s: Scattering density phase: Phase function of the scattering * type (Rayleigh or Mie) L: Radiance coming from the light source segment_length: The * length of the segment * * The code here is just that, with a bit of additional optimization to not store full * spectra for the optical depth */ r_spectrum[wl] += attenuation * reduce_add(phase_function * scattering_density) * irradiance[wl] * segment_length; } } /* advance along ray */ P += segment; } } void SKY_nishita_skymodel_precompute_texture(float *pixels, int stride, int start_y, int end_y, int width, int height, float sun_elevation, float altitude, float air_density, float dust_density, float ozone_density) { /* calculate texture pixels */ float spectrum[num_wavelengths]; int half_width = width / 2; float3 cam_pos = make_float3(0, 0, earth_radius + altitude); float3 sun_dir = geographical_to_direction(sun_elevation, 0.0f); float latitude_step = M_PI_2_F / height; float longitude_step = M_2PI_F / width; float half_lat_step = latitude_step / 2.0f; for (int y = start_y; y < end_y; y++) { /* sample more pixels toward the horizon */ float latitude = (M_PI_2_F + half_lat_step) * sqr((float)y / height); float *pixel_row = pixels + (y * width * stride); for (int x = 0; x < half_width; x++) { float longitude = longitude_step * x - M_PI_F; float3 dir = geographical_to_direction(latitude, longitude); single_scattering(dir, sun_dir, cam_pos, air_density, dust_density, ozone_density, spectrum); float3 xyz = spec_to_xyz(spectrum); /* store pixels */ int pos_x = x * stride; pixel_row[pos_x] = xyz.x; pixel_row[pos_x + 1] = xyz.y; pixel_row[pos_x + 2] = xyz.z; /* mirror sky */ int mirror_x = (width - x - 1) * stride; pixel_row[mirror_x] = xyz.x; pixel_row[mirror_x + 1] = xyz.y; pixel_row[mirror_x + 2] = xyz.z; } } } /*********** Sun ***********/ static void sun_radiation(float3 cam_dir, float altitude, float air_density, float dust_density, float solid_angle, float *r_spectrum) { float3 cam_pos = make_float3(0, 0, earth_radius + altitude); float3 optical_depth = ray_optical_depth(cam_pos, cam_dir); /* compute final spectrum */ for (int i = 0; i < num_wavelengths; i++) { /* combine spectra and the optical depth into transmittance */ float transmittance = rayleigh_coeff[i] * optical_depth.x * air_density + 1.11f * mie_coeff * optical_depth.y * dust_density; r_spectrum[i] = irradiance[i] * expf(-transmittance) / solid_angle; } } void SKY_nishita_skymodel_precompute_sun(float sun_elevation, float angular_diameter, float altitude, float air_density, float dust_density, float *r_pixel_bottom, float *r_pixel_top) { /* definitions */ float half_angular = angular_diameter / 2.0f; float solid_angle = M_2PI_F * (1.0f - cosf(half_angular)); float spectrum[num_wavelengths]; float bottom = sun_elevation - half_angular; float top = sun_elevation + half_angular; float elevation_bottom, elevation_top; float3 pix_bottom, pix_top, sun_dir; /* compute 2 pixels for sun disc */ elevation_bottom = (bottom > 0.0f) ? bottom : 0.0f; elevation_top = (top > 0.0f) ? top : 0.0f; sun_dir = geographical_to_direction(elevation_bottom, 0.0f); sun_radiation(sun_dir, altitude, air_density, dust_density, solid_angle, spectrum); pix_bottom = spec_to_xyz(spectrum); sun_dir = geographical_to_direction(elevation_top, 0.0f); sun_radiation(sun_dir, altitude, air_density, dust_density, solid_angle, spectrum); pix_top = spec_to_xyz(spectrum); /* store pixels */ r_pixel_bottom[0] = pix_bottom.x; r_pixel_bottom[1] = pix_bottom.y; r_pixel_bottom[2] = pix_bottom.z; r_pixel_top[0] = pix_top.x; r_pixel_top[1] = pix_top.y; r_pixel_top[2] = pix_top.z; }