/* * Copyright (C) 2021 Christopher J. Howard * * This file is part of Antkeeper source code. * * Antkeeper source code is free software: you can redistribute it and/or modify * it under the terms of the GNU General Public License as published by * the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * Antkeeper source code is distributed in the hope that it will be useful, * but WITHOUT ANY WARRANTY; without even the implied warranty of * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * GNU General Public License for more details. * * You should have received a copy of the GNU General Public License * along with Antkeeper source code. If not, see . */ #include "entity/systems/astronomy.hpp" #include "astro/apparent-size.hpp" #include "entity/components/blackbody.hpp" #include "entity/components/transform.hpp" #include "geom/intersection.hpp" #include "color/color.hpp" #include "physics/orbit/orbit.hpp" #include "physics/time/ut1.hpp" #include "physics/light/photometry.hpp" #include "physics/light/luminosity.hpp" #include "physics/light/refraction.hpp" #include "physics/atmosphere.hpp" #include "geom/cartesian.hpp" #include namespace entity { namespace system { template math::vector3 transmittance(T depth_r, T depth_m, T depth_o, const math::vector3& beta_r, const math::vector3& beta_m) { math::vector3 transmittance_r = beta_r * depth_r; math::vector3 transmittance_m = beta_m * 1.1 * depth_m; math::vector3 transmittance_o = {0, 0, 0}; math::vector3 t = transmittance_r + transmittance_m + transmittance_o; t.x = std::exp(-t.x); t.y = std::exp(-t.y); t.z = std::exp(-t.z); return t; } astronomy::astronomy(entity::registry& registry): updatable(registry), universal_time(0.0), time_scale(1.0), reference_entity(entt::null), observer_location{0, 0, 0}, sun_light(nullptr), sky_pass(nullptr) { // Construct reference frame which transforms coordinates from SEZ to EZS sez_to_ezs = physics::frame { {0, 0, 0}, math::normalize ( math::quaternion::rotate_x(-math::half_pi) * math::quaternion::rotate_z(-math::half_pi) ) }; // Construct reference frame which transforms coordinates from EZS to SEZ ezs_to_sez = sez_to_ezs.inverse(); registry.on_construct().connect<&astronomy::on_celestial_body_construct>(this); registry.on_replace().connect<&astronomy::on_celestial_body_replace>(this); } void astronomy::update(double t, double dt) { // Add scaled timestep to current time set_universal_time(universal_time + dt * time_scale); // Abort if no reference body if (reference_entity == entt::null) return; // Abort if either reference body or orbit have not been set if (!registry.has(reference_entity) || !registry.has(reference_entity)) return; const entity::component::orbit& reference_orbit = registry.get(reference_entity); const entity::component::celestial_body& reference_body = registry.get(reference_entity); // Determine axial rotation at current time const double reference_axial_rotation = reference_body.axial_rotation + reference_body.angular_frequency * universal_time; // Construct reference frame which transforms coordinates from inertial space to reference body BCBF space inertial_to_bcbf = physics::orbit::inertial::to_bcbf ( reference_orbit.state.r, reference_orbit.elements.i, reference_body.axial_tilt, reference_axial_rotation ); // Construct reference frame which transforms coordinates from inertial space to reference body topocentric space inertial_to_topocentric = inertial_to_bcbf * bcbf_to_topocentric; // Set the transform component translations of orbiting bodies to their topocentric positions registry.view().each( [&](entity::id entity_id, const auto& celestial_body, const auto& orbit, auto& transform) { // Transform Cartesian position vector (r) from inertial space to topocentric space const math::vector3 r_topocentric = inertial_to_topocentric * orbit.state.r; // Update local transform transform.local.translation = math::type_cast(r_topocentric); }); // Update blackbody lighting registry.view().each( [&](entity::id entity_id, const auto& celestial_body, const auto& orbit, const auto& blackbody) { // Calculate blackbody inertial basis double3 blackbody_forward_inertial = math::normalize(reference_orbit.state.r - orbit.state.r); double3 blackbody_up_inertial = {0, 0, 1}; // Transform blackbody inertial position and basis into topocentric space double3 blackbody_position_topocentric = inertial_to_topocentric * orbit.state.r; double3 blackbody_forward_topocentric = inertial_to_topocentric.rotation * blackbody_forward_inertial; double3 blackbody_up_topocentric = inertial_to_topocentric.rotation * blackbody_up_inertial; // Calculate distance from observer to blackbody double blackbody_distance = math::length(blackbody_position_topocentric) - celestial_body.radius; // Calculate blackbody distance attenuation double distance_attenuation = 1.0 / (blackbody_distance * blackbody_distance); // Init atmospheric transmittance double3 atmospheric_transmittance = {1.0, 1.0, 1.0}; // Get atmosphere component of reference body (if any) if (this->registry.has(reference_entity)) { const entity::component::atmosphere& reference_atmosphere = registry.get(reference_entity); // Altitude of observer in meters geom::ray sample_ray; sample_ray.origin = {0, reference_body.radius + observer_location[0], 0}; sample_ray.direction = math::normalize(blackbody_position_topocentric); geom::sphere exosphere; exosphere.center = {0, 0, 0}; exosphere.radius = reference_body.radius + reference_atmosphere.exosphere_altitude; auto intersection_result = geom::ray_sphere_intersection(sample_ray, exosphere); if (std::get<0>(intersection_result)) { double3 sample_start = sample_ray.origin; double3 sample_end = sample_ray.extrapolate(std::get<2>(intersection_result)); double optical_depth_r = physics::atmosphere::optical_depth(sample_start, sample_end, reference_body.radius, reference_atmosphere.rayleigh_scale_height, 32); double optical_depth_k = physics::atmosphere::optical_depth(sample_start, sample_end, reference_body.radius, reference_atmosphere.mie_scale_height, 32); double optical_depth_o = 0.0; atmospheric_transmittance = transmittance(optical_depth_r, optical_depth_k, optical_depth_o, reference_atmosphere.rayleigh_scattering, reference_atmosphere.mie_scattering); } } if (sun_light != nullptr) { // Update blackbody light transform sun_light->set_translation(math::normalize(math::type_cast(blackbody_position_topocentric))); sun_light->set_rotation ( math::look_rotation ( math::type_cast(blackbody_forward_topocentric), math::type_cast(blackbody_up_topocentric) ) ); // Sun color at the outer atmosphere float3 sun_color_outer = math::type_cast(blackbody.luminous_intensity * distance_attenuation); // Sun color at sea level float3 sun_color_inner = math::type_cast(blackbody.luminous_intensity * distance_attenuation * atmospheric_transmittance); // Update blackbody light color and intensity sun_light->set_color(sun_color_inner); sun_light->set_intensity(1.0f); // Upload blackbody params to sky pass if (this->sky_pass) { this->sky_pass->set_sun_position(math::type_cast(blackbody_position_topocentric)); this->sky_pass->set_sun_color(sun_color_outer, sun_color_inner); double blackbody_angular_radius = std::asin((celestial_body.radius * 2.0) / (blackbody_distance * 2.0)); this->sky_pass->set_sun_angular_radius(static_cast(blackbody_angular_radius)); } } }); // Update sky pass topocentric frame if (sky_pass != nullptr) { // Upload topocentric frame to sky pass sky_pass->set_topocentric_frame ( physics::frame { math::type_cast(inertial_to_topocentric.translation), math::type_cast(inertial_to_topocentric.rotation) } ); // Upload observer altitude to sky pass sky_pass->set_observer_altitude(observer_location[0]); // Upload atmosphere params to sky pass if (registry.has(reference_entity)) { const entity::component::atmosphere& reference_atmosphere = registry.get(reference_entity); sky_pass->set_scale_heights(reference_atmosphere.rayleigh_scale_height, reference_atmosphere.mie_scale_height); sky_pass->set_scattering_coefficients(math::type_cast(reference_atmosphere.rayleigh_scattering), math::type_cast(reference_atmosphere.mie_scattering)); sky_pass->set_mie_anisotropy(reference_atmosphere.mie_anisotropy); sky_pass->set_atmosphere_radii(reference_body.radius, reference_body.radius + reference_atmosphere.exosphere_altitude); } } } void astronomy::set_universal_time(double time) { universal_time = time; } void astronomy::set_time_scale(double scale) { time_scale = scale; } void astronomy::set_reference_body(entity::id entity_id) { reference_entity = entity_id; update_bcbf_to_topocentric(); } void astronomy::set_observer_location(const double3& location) { observer_location = location; update_bcbf_to_topocentric(); } void astronomy::set_sun_light(scene::directional_light* light) { sun_light = light; } void astronomy::set_sky_pass(::render::sky_pass* pass) { this->sky_pass = pass; } void astronomy::on_celestial_body_construct(entity::registry& registry, entity::id entity_id, entity::component::celestial_body& celestial_body) { if (entity_id == reference_entity) update_bcbf_to_topocentric(); } void astronomy::on_celestial_body_replace(entity::registry& registry, entity::id entity_id, entity::component::celestial_body& celestial_body) { if (entity_id == reference_entity) update_bcbf_to_topocentric(); } void astronomy::update_bcbf_to_topocentric() { double radial_distance = observer_location[0]; if (reference_entity) { if (registry.has(reference_entity)) radial_distance += registry.get(reference_entity).radius; } // Construct reference frame which transforms coordinates from BCBF space to topocentric space bcbf_to_topocentric = physics::orbit::bcbf::to_topocentric ( radial_distance, observer_location[1], observer_location[2] ) * sez_to_ezs; } } // namespace system } // namespace entity