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daylight.cpp
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daylight.cpp
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/*
* Copyright (c)2018 dresden elektronik ingenieurtechnik gmbh.
* All rights reserved.
*
* The software in this package is published under the terms of the BSD
* style license a copy of which has been included with this distribution in
* the LICENSE.txt file.
*
*/
#include <QtMath>
#include <QVariantMap>
#include "daylight.h"
// Qt/C++ port of:
// https://github.com/mourner/suncalc/blob/master/suncalc.js
static const qreal dayMs = 1000 * 60 * 60 * 24;
static const qreal J1970 = 2440588;
static const qreal J2000 = 2451545;
static const double rad = M_PI / 180;
static const double e = rad * 23.4397; // obliquity of the Earth
static double toJulian(double msecSinceEpoch) { return msecSinceEpoch / dayMs - 0.5 + J1970; }
static double fromJulian(double j) { return (j + 0.5 - J1970) * dayMs; }
static double toDays(double msecSinceEpoch) { return toJulian(msecSinceEpoch) - J2000; }
static double declination(double l, double b) { return asin(sin(b) * cos(e) + cos(b) * sin(e) * sin(l)); }
// general sun calculations
static double solarMeanAnomaly(double d) { return rad * (357.5291 + 0.98560028 * d); }
static double eclipticLongitude(double M) {
double C = rad * (1.9148 * sin(M) + 0.02 * sin(2 * M) + 0.0003 * sin(3 * M)); // equation of center
double P = rad * 102.9372; // perihelion of the Earth
return M + C + P + M_PI;
}
// calculations for sun times
static const double J0 = 0.0009;
static double julianCycle(double d, double lw) { return round(d - J0 - lw / (2 * M_PI)); }
static double approxTransit(double Ht, double lw, double n) { return J0 + (Ht + lw) / (2 * M_PI) + n; }
static double solarTransitJ(double ds, double M, double L) { return J2000 + ds + 0.0053 * sin(M) - 0.0069 * sin(2 * L); }
static double hourAngle(double h, double phi, double d) { return acos((sin(h) - sin(phi) * sin(d)) / (cos(phi) * cos(d))); }
// returns set time for the given sun altitude
static double getSetJ(double h, double lw, double phi, double dec, double n, double M, double L) {
double w = hourAngle(h, phi, dec);
double a = approxTransit(w, lw, n);
return solarTransitJ(a, M, L);
}
struct TimePin {
double offset;
const char *first;
int firstWeight;
const char *second;
int secondWeight;
};
// calculates sun times for a given date and latitude/longitude
void getDaylightTimes(quint64 msecSinceEpoch, double lat, double lng, std::vector<DL_Result> &result)
{
std::vector<TimePin> times;
// sun times configuration (angle, morning name, evening name)
times.push_back({-0.833, "sunriseStart", DL_SUNRISE_START, "sunsetEnd", DL_SUNSET_END});
times.push_back({-0.3, "sunriseEnd", DL_SUNRISE_END, "sunsetStart", DL_SUNSET_START});
times.push_back({-6, "dawn", DL_DAWN, "dusk", DL_DUSK});
times.push_back({-12, "nauticalDawn", DL_NAUTICAL_DAWN, "nauticalDusk", DL_NAUTICAL_DUSK});
times.push_back({-18, "nightEnd", DL_NIGHT_END, "nightStart", DL_NIGHT_START});
times.push_back({6, "goldenHour1", DL_GOLDENHOUR1, "goldenHour2", DL_GOLDENHOUR2});
double lw = rad * -lng,
phi = rad * lat,
d = toDays(msecSinceEpoch),
n = julianCycle(d, lw),
ds = approxTransit(0, lw, n),
M = solarMeanAnomaly(ds),
L = eclipticLongitude(M),
dec = declination(L, 0),
Jnoon = solarTransitJ(ds, M, L),
Jset, Jrise;
result.push_back({"solarNoon", DL_SOLAR_NOON, (quint64)fromJulian(Jnoon)});
result.push_back({"nadir", DL_NADIR, (quint64)fromJulian(Jnoon - 0.5)});
for (const TimePin &time : times)
{
Jset = getSetJ(time.offset * rad, lw, phi, dec, n, M, L);
Jrise = Jnoon - (Jset - Jnoon);
result.push_back({time.first, time.firstWeight, (quint64)fromJulian(Jrise)});
result.push_back({time.second, time.secondWeight, (quint64)fromJulian(Jset)});
}
std::sort(result.begin(), result.end(),
[](const DL_Result &a, const DL_Result &b)
{ return a.msecsSinceEpoch < b.msecsSinceEpoch; });
}