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@ -25,6 +25,7 @@ |
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#include "renderer/passes/material-pass.hpp"
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#include "renderer/passes/material-pass.hpp"
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#include "utility/gamma.hpp"
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#include "utility/gamma.hpp"
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#include "resources/image.hpp"
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#include "resources/image.hpp"
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#include "game/astronomy/celestial-coordinates.hpp"
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#include <cmath>
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#include <cmath>
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#include <iostream>
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#include <iostream>
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@ -54,31 +55,30 @@ static double julian_day(int year, int month, int day, double time) |
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return std::floor(365.25 * y) + std::floor(30.6001 * (m + 1.0)) - 15.0 + 1720996.5 + d + time; |
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return std::floor(365.25 * y) + std::floor(30.6001 * (m + 1.0)) - 15.0 + 1720996.5 + d + time; |
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} |
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} |
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/// @see A Physically-Based Night Sky Model
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/// @see http://www.powerfromthesun.net/Book/chapter03/chapter03.html
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void find_sun_ecliptic(double jd, double* longitude, double* latitude, double* distance) |
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/**
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* Calculates the ecliptic rectangular geocentric coordinates of the sun, with distance in AU. |
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*/ |
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double3 calculate_sun_ecliptic(double jd) |
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{ |
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{ |
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const double t = (jd - 2451545.0) / 36525.0; |
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const double t = (jd - 2451545.0) / 36525.0; |
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const double m = 6.24 + 628.302 * t; |
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const double m = 6.24 + 628.302 * t; |
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*longitude = 4.895048 + 628.331951 * t + (0.033417 - 0.000084 * t) * std::sin(m) + 0.000351 * std::sin(m * 2.0); |
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*latitude = 0.0; |
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*distance = 1.000140 - (0.016708 - 0.000042 * t) * std::cos(m) - 0.000141 * std::cos(m * 2.0); |
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const double longitude = 4.895048 + 628.331951 * t + (0.033417 - 0.000084 * t) * std::sin(m) + 0.000351 * std::sin(m * 2.0); |
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const double latitude = 0.0; |
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const double distance = 1.000140 - (0.016708 - 0.000042 * t) * std::cos(m) - 0.000141 * std::cos(m * 2.0); |
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double3 ecliptic; |
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ecliptic.x = distance * std::cos(longitude) * std::cos(latitude); |
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ecliptic.y = distance * std::sin(longitude) * std::cos(latitude); |
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ecliptic.z = distance * std::sin(latitude); |
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return ecliptic; |
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} |
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} |
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/**
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/**
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* Calculates the ecliptic geocentric coordinates of the moon, given a Julian day. |
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* |
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* @param[in] jd Julian day. |
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* @param[out] longitude Ecliptic longitude of the moon, in radians. |
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* @param[out] latitude Ecliptic latitude of the moon, in radians. |
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* @param[out] distance Distance to the moon, in Earth radii. |
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* @return Array containing the ecliptic longitude and latitude of the moon, in radians. |
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* |
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* @see A Physically-Based Night Sky Model |
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* Calculates the ecliptic rectangular geocentric coordinates of the moon, with distance in Earth radii. |
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*/ |
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*/ |
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void find_moon_ecliptic(double jd, double* longitude, double* latitude, double* distance) |
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double3 calculate_moon_ecliptic(double jd) |
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{ |
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{ |
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const double t = (jd - 2451545.0) / 36525.0; |
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const double t = (jd - 2451545.0) / 36525.0; |
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const double l1 = 3.8104 + 8399.7091 * t; |
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const double l1 = 3.8104 + 8399.7091 * t; |
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@ -88,7 +88,7 @@ void find_moon_ecliptic(double jd, double* longitude, double* latitude, double* |
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const double d2 = d * 2.0; |
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const double d2 = d * 2.0; |
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const double f = 1.6280 + 8433.4663 * t; |
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const double f = 1.6280 + 8433.4663 * t; |
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*longitude = l1 |
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const double longitude = l1 |
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+ 0.1098 * std::sin(m1) |
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+ 0.1098 * std::sin(m1) |
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+ 0.0222 * std::sin(d2 - m1) |
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+ 0.0222 * std::sin(d2 - m1) |
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+ 0.0115 * std::sin(d2) |
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+ 0.0115 * std::sin(d2) |
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@ -103,7 +103,7 @@ void find_moon_ecliptic(double jd, double* longitude, double* latitude, double* |
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- 0.0006 * std::sin(d) |
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- 0.0006 * std::sin(d) |
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- 0.0005 * std::sin(m + m1); |
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- 0.0005 * std::sin(m + m1); |
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*latitude = 0.0895 * sin(f) |
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const double latitude = 0.0895 * sin(f) |
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+ 0.0049 * std::sin(m1 + f) |
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+ 0.0049 * std::sin(m1 + f) |
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+ 0.0048 * std::sin(m1 - f) |
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+ 0.0048 * std::sin(m1 - f) |
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+ 0.0030 * std::sin(d2 - f) |
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+ 0.0030 * std::sin(d2 - f) |
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@ -111,13 +111,54 @@ void find_moon_ecliptic(double jd, double* longitude, double* latitude, double* |
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+ 0.0008 * std::sin(d2 - f - m1) |
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+ 0.0008 * std::sin(d2 - f - m1) |
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+ 0.0006 * std::sin(d2 + f); |
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+ 0.0006 * std::sin(d2 + f); |
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*distance = 1.0 / (0.016593 |
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const double r = 1.0 / (0.016593 |
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+ 0.000904 * std::cos(m1) |
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+ 0.000904 * std::cos(m1) |
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+ 0.000166 * std::cos(d2 - m1) |
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+ 0.000166 * std::cos(d2 - m1) |
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+ 0.000137 * std::cos(d2) |
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+ 0.000137 * std::cos(d2) |
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+ 0.000049 * std::cos(m1 * 2.0) |
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+ 0.000049 * std::cos(m1 * 2.0) |
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+ 0.000015 * std::cos(d2 + m1) |
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+ 0.000015 * std::cos(d2 + m1) |
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+ 0.000009 * std::cos(d2 - m)); |
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+ 0.000009 * std::cos(d2 - m)); |
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double3 ecliptic; |
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ecliptic.x = r * std::cos(longitude) * std::cos(latitude); |
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ecliptic.y = r * std::sin(longitude) * std::cos(latitude); |
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ecliptic.z = r * std::sin(latitude); |
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return ecliptic; |
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} |
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double3x3 find_moon_ecliptic_rotation(double jd) |
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{ |
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const double t = (jd - 2451545.0) / 36525.0; |
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const double l1 = 3.8104 + 8399.7091 * t; |
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const double f = 1.6280 + 8433.4663 * t; |
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const double az0 = f + math::pi<double>; |
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const double ax = 0.026920; |
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const double az1 = l1 - f; |
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double3x3 rz0 = |
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{ |
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cos(az0), -sin(az0), 0, |
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sin(az0), cos(az0), 0, |
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0, 0, 1 |
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}; |
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double3x3 rx = |
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{ |
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1, 0, 0, |
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0, cos(ax), -sin(ax), |
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0, sin(ax), cos(ax) |
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}; |
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double3x3 rz1 = |
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{ |
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cos(az1), -sin(az1), 0, |
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sin(az1), cos(az1), 0, |
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0, 0, 1 |
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}; |
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return rz0 * rx * rz1; |
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} |
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} |
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/// @see http://www.stjarnhimlen.se/comp/ppcomp.html
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/// @see http://www.stjarnhimlen.se/comp/ppcomp.html
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@ -154,6 +195,17 @@ void equatorial_to_horizontal(double right_ascension, double declination, double |
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*elevation = math::wrap_radians<double>(std::atan2(horiz_z, std::sqrt(horiz_x * horiz_x + horiz_y * horiz_y))); |
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*elevation = math::wrap_radians<double>(std::atan2(horiz_z, std::sqrt(horiz_x * horiz_x + horiz_y * horiz_y))); |
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} |
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} |
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double3x3 horizontal_to_right_handed() |
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{ |
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return double3x3 |
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{ |
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0.0, 0.0, 1.0, |
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1.0, 0.0, 0.0, |
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0.0, -1.0, 0.0 |
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}; |
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} |
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/**
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/**
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* Calculates the Greenwich mean sidereal time (GMST) from a Julian day. |
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* Calculates the Greenwich mean sidereal time (GMST) from a Julian day. |
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* |
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* |
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@ -187,97 +239,72 @@ void weather_system::update(double t, double dt) |
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const float latitude = location[0]; |
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const float latitude = location[0]; |
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const float longitude = location[1]; |
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const float longitude = location[1]; |
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// Time correction
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double tc = longitude / (math::two_pi<double> / 24.0); |
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//double pst_tc = -7.0;
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double local_jd = jd + tc / 24.0 - 0.5; |
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// Calculate local mean sidereal time (LMST)
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double time_correction = longitude / (math::two_pi<double> / 24.0); |
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double local_jd = jd + time_correction / 24.0 - 0.5; |
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double local_time = (local_jd - std::floor(local_jd)) * 24.0; |
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double local_time = (local_jd - std::floor(local_jd)) * 24.0; |
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double hour = local_time; |
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double hour = local_time; |
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// Calculate equation of time
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//float eot_b = (360.0f / 365.0f) * (day_of_year - 81.0f);
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//float eot = 9.87f * std::sin(eot_b * 2.0f) - 7.53f * std::cos(eot_b) - 1.5f * std::sin(eot_b);
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// Calculate local mean sidereal time (LST)
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//double tc = longitude / (math::two_pi<double> / 24.0); // Time correction
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//double ut = local_time + tc; // Universal time
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double gmst = jd_to_gmst(jd); |
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double gmst = jd_to_gmst(jd); |
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double lmst = gmst + longitude; |
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double lmst = gmst + longitude; |
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// Calculate sun position
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//float local_solar_time = local_time;// + eot / 60.0f;
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/*
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float sun_declination = math::radians(23.45f) * std::sin((math::two_pi<float> / 365.0f) * (284.0f + day_of_year)); |
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float sun_hour_angle = math::radians(15.0f) * (local_solar_time - 12.0f); |
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sun_elevation = std::asin(std::sin(sun_declination) * std::sin(latitude) + std::cos(sun_declination) * std::cos(sun_hour_angle) * std::cos(latitude)); |
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sun_azimuth = std::acos((std::sin(sun_declination) * std::cos(latitude) - std::cos(sun_declination) * std::cos(sun_hour_angle) * std::sin(latitude)) / std::cos(sun_elevation)); |
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if (sun_hour_angle > 0.0f) |
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sun_azimuth = math::two_pi<float> - sun_azimuth; |
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*/ |
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// J2000 day
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double d = jd - 2451545.0; |
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// Obliquity of the ecliptic
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// Obliquity of the ecliptic
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double ecl = math::radians<double>(23.4393 - 3.563e-7 * d); |
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// Calculation sun coordinates
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double sun_longitude; |
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double sun_latitude; |
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double sun_distance; |
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double sun_right_ascension; |
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double sun_declination; |
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double sun_azimuth; |
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double sun_elevation; |
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find_sun_ecliptic(jd, &sun_longitude, &sun_latitude, &sun_distance); |
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ecliptic_to_equatorial(sun_longitude, sun_latitude, ecl, &sun_right_ascension, &sun_declination); |
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equatorial_to_horizontal(sun_right_ascension, sun_declination, lmst, latitude, &sun_azimuth, &sun_elevation); |
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// Calculate moon coordinates
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double moon_longitude; |
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double moon_latitude; |
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double moon_distance; |
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double moon_right_ascension; |
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double moon_declination; |
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double moon_azimuth; |
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double moon_elevation; |
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find_moon_ecliptic(jd, &moon_longitude, &moon_latitude, &moon_distance); |
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ecliptic_to_equatorial(moon_longitude, moon_latitude, ecl, &moon_right_ascension, &moon_declination); |
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equatorial_to_horizontal(moon_right_ascension, moon_declination, lmst, latitude, &moon_azimuth, &moon_elevation); |
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float2 sun_az_el = float2{static_cast<float>(sun_azimuth), static_cast<float>(sun_elevation)}; |
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math::quaternion<float> sun_azimuth_rotation = math::angle_axis(sun_az_el[0], float3{0, 1, 0}); |
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math::quaternion<float> sun_elevation_rotation = math::angle_axis(sun_az_el[1], float3{-1, 0, 0}); |
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math::quaternion<float> sun_rotation = math::normalize(sun_azimuth_rotation * sun_elevation_rotation); |
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float3 sun_position = math::normalize(sun_rotation * float3{0, 0, -1}); |
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float2 moon_az_el = float2{static_cast<float>(moon_azimuth), static_cast<float>(moon_elevation)}; |
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math::quaternion<float> moon_azimuth_rotation = math::angle_axis(moon_az_el[0], float3{0, 1, 0}); |
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math::quaternion<float> moon_elevation_rotation = math::angle_axis(moon_az_el[1], float3{-1, 0, 0}); |
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math::quaternion<float> moon_rotation = math::normalize(moon_azimuth_rotation * moon_elevation_rotation); |
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float3 moon_position = math::normalize(moon_rotation * float3{0, 0, -1}); |
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double ecl = math::radians<double>(23.4393 - 3.563e-7 * (jd - 2451545.0)); |
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// Solar distance in AU
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//double sr = ...
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// Apparent radius in degrees
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//double sradius = 0.2666 / sr;
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double3x3 ecliptic_to_horizontal = ast::ecliptic_to_horizontal(ecl, latitude, lmst); |
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double3 sun_ecliptic = calculate_sun_ecliptic(jd); |
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double3 sun_horizontal = ecliptic_to_horizontal * sun_ecliptic; |
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double3 sun_spherical = ast::rectangular_to_spherical(sun_horizontal); |
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double3 sun_positiond = horizontal_to_right_handed() * sun_horizontal; |
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float2 sun_az_el = {static_cast<float>(sun_spherical.z) - math::pi<float>, static_cast<float>(sun_spherical.y)}; |
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float3 sun_position = math::normalize(float3{static_cast<float>(sun_positiond.x), static_cast<float>(sun_positiond.y), static_cast<float>(sun_positiond.z)}); |
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double3 moon_ecliptic = calculate_moon_ecliptic(jd); |
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double3 moon_horizontal = ecliptic_to_horizontal * moon_ecliptic; |
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moon_horizontal.z -= 1.0; // Subtract one earth radius, for position of observer
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double3 moon_spherical = ast::rectangular_to_spherical(moon_horizontal); |
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double3 moon_positiond = horizontal_to_right_handed() * moon_horizontal; |
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float2 moon_az_el = {static_cast<float>(moon_spherical.z) - math::pi<float>, static_cast<float>(moon_spherical.y)}; |
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float3 moon_position = math::normalize(float3{static_cast<float>(moon_positiond.x), static_cast<float>(moon_positiond.y), static_cast<float>(moon_positiond.z)}); |
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//std::cout << "new moon: " << math::degrees(moon_az_el[0]) << ", " << math::degrees(moon_az_el[1]) << std::endl;
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double3x3 moon_rotation_matrix = horizontal_to_right_handed() * ecliptic_to_horizontal; |
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math::quaternion<double> moon_rotationd = math::normalize(math::quaternion_cast(moon_rotation_matrix) * math::angle_axis(math::half_pi<double>, double3{0, 1, 0}) * math::angle_axis(-math::half_pi<double>, double3{0, 0, -1})); |
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math::quaternion<float> moon_rotation = |
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{ |
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static_cast<float>(moon_rotationd.w), |
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static_cast<float>(moon_rotationd.x), |
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static_cast<float>(moon_rotationd.y), |
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static_cast<float>(moon_rotationd.z) |
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}; |
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if (sun_light) |
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if (sun_light) |
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{ |
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{ |
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sun_light->set_rotation(sun_rotation); |
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math::quaternion<float> sun_azimuth_rotation = math::angle_axis(sun_az_el[0], float3{0, 1, 0}); |
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math::quaternion<float> sun_elevation_rotation = math::angle_axis(sun_az_el[1], float3{-1, 0, 0}); |
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math::quaternion<float> sun_az_el_rotation = math::normalize(sun_azimuth_rotation * sun_elevation_rotation); |
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sun_light->set_rotation(sun_az_el_rotation); |
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} |
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} |
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if (moon_light) |
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if (moon_light) |
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{ |
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{ |
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moon_light->set_rotation(moon_rotation); |
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math::quaternion<float> moon_azimuth_rotation = math::angle_axis(moon_az_el[0], float3{0, 1, 0}); |
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math::quaternion<float> moon_elevation_rotation = math::angle_axis(moon_az_el[1], float3{-1, 0, 0}); |
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math::quaternion<float> moon_az_el_rotation = math::normalize(moon_azimuth_rotation * moon_elevation_rotation); |
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moon_light->set_rotation(moon_az_el_rotation); |
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} |
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} |
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std::size_t hour_index = static_cast<std::size_t>(hour); |
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std::size_t hour_index = static_cast<std::size_t>(hour); |
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float lerp_factor = hour - std::floor(hour); |
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float lerp_factor = hour - std::floor(hour); |
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float sun_gradient_position = static_cast<float>(std::max<double>(0.0, ((sun_elevation + math::half_pi<double>) / math::pi<double>))); |
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float moon_gradient_position = static_cast<float>(std::max<double>(0.0, ((moon_elevation + math::half_pi<double>) / math::pi<double>))); |
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float sun_gradient_position = static_cast<float>(std::max<double>(0.0, ((sun_az_el[1] + math::half_pi<double>) / math::pi<double>))); |
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float moon_gradient_position = static_cast<float>(std::max<double>(0.0, ((moon_az_el[1] + math::half_pi<double>) / math::pi<double>))); |
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float sky_gradient_position = sun_gradient_position; |
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float sky_gradient_position = sun_gradient_position; |
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float ambient_gradient_position = sun_gradient_position; |
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float ambient_gradient_position = sun_gradient_position; |
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@ -290,9 +317,11 @@ void weather_system::update(double t, double dt) |
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float3 ambient_color = interpolate_gradient(ambient_colors, ambient_gradient_position); |
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float3 ambient_color = interpolate_gradient(ambient_colors, ambient_gradient_position); |
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sun_light->set_color(sun_color); |
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sun_light->set_color(sun_color); |
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sun_light->set_intensity(1.0f); |
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moon_light->set_color(moon_color); |
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moon_light->set_color(moon_color); |
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moon_light->set_intensity(1.0f); |
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moon_light->set_intensity(1.0f); |
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ambient_light->set_color(ambient_color); |
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ambient_light->set_color(ambient_color); |
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ambient_light->set_intensity(0.5f); |
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sky_pass->set_horizon_color(horizon_color); |
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sky_pass->set_horizon_color(horizon_color); |
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sky_pass->set_zenith_color(zenith_color); |
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sky_pass->set_zenith_color(zenith_color); |
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@ -301,12 +330,13 @@ void weather_system::update(double t, double dt) |
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sky_pass->set_sun_coordinates(sun_position, sun_az_el); |
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sky_pass->set_sun_coordinates(sun_position, sun_az_el); |
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sky_pass->set_moon_coordinates(moon_position, moon_az_el); |
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sky_pass->set_moon_coordinates(moon_position, moon_az_el); |
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sky_pass->set_julian_day(static_cast<float>(jd)); |
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sky_pass->set_julian_day(static_cast<float>(jd)); |
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sky_pass->set_moon_rotation(moon_rotation); |
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} |
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} |
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shadow_light = sun_light; |
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shadow_light = sun_light; |
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if (shadow_map_pass) |
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if (shadow_map_pass) |
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{ |
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{ |
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if (sun_elevation < 0.0f) |
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if (sun_az_el[1] < 0.0f) |
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{ |
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{ |
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shadow_map_pass->set_light(moon_light); |
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shadow_map_pass->set_light(moon_light); |
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} |
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} |
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@ -367,11 +397,6 @@ void weather_system::set_shadow_map_pass(::shadow_map_pass* pass) |
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void weather_system::set_material_pass(::material_pass* pass) |
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void weather_system::set_material_pass(::material_pass* pass) |
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{ |
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{ |
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material_pass = pass; |
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material_pass = pass; |
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if (material_pass) |
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{ |
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material_pass->set_shadow_strength(0.75f); |
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} |
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} |
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} |
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void weather_system::set_time(int year, int month, int day, int hour, int minute, int second, double tc) |
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void weather_system::set_time(int year, int month, int day, int hour, int minute, int second, double tc) |
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