// Encoding: UTF-8 #include "calendar.h" #include #include #include /*以下为"calendar.h规定之量*/ double day = 86400; double delta = 1e-11; Julian julian; parameter p; pair getSunPos(time_t time) { double t = julian.getJulianKiloYear(time); pair sun = p.sun_longitude(t); radToDMS("Sun longitude:\t\t", 0, 360, sun.first); radToDMS("Sun latitude:\t\t", -90, 90, sun.second); double alpha, delta; // 太阳赤经赤纬 double lambda = sun.first, beta = sun.second; // 太阳黄经黄纬 // 黄赤交角epsilon double epsilon = p.get_epsilon(t); radToDMS("Ecliptic Obliquity:\t\t", 0, 90, epsilon); delta = asin(sin(epsilon) * sin(lambda) * cos(beta) + cos(epsilon) * sin(beta)); alpha = atan2( (cos(epsilon) * sin(lambda) * cos(beta) - sin(epsilon) * sin(beta)), (cos(lambda) * cos(beta))); radToDMS("Sun right ascension:\t\t", 0, 360, alpha); radToDMS("Sun declination:\t\t", -90, 90, delta); // 时角 double H = p.getHourAngle(t, LONGITUDE, LATITUDE, alpha); double A, h; //方位角和高度角 h = asin(sin(LATITUDE) * sin(delta) + cos(LATITUDE) * cos(delta) * cos(H)); A = atan2(-cos(delta) * sin(H), cos(LATITUDE) * sin(delta) - sin(LATITUDE) * cos(delta) * cos(H)); A += M_PI; // 转换为角度制输出 radToDMS("Hour angle:\t\t", 0, 360, H); radToDMS("Azimuth:\t\t", 0, 360, A); radToDMS("Elevation:\t\t", -90, 90, h); } int main(int argc, char *argv[]) { Date date; if (argc != 2) { printf("Input the time you want to calculate in " "format:\t\t"); scanf("%d-%d-%d,%d:%d:%d", &date.tm_year, &date.tm_mon, &date.tm_mday, &date.tm_hour, &date.tm_min, &date.tm_sec); } else { sscanf(argv[1], "%d-%d-%d,%d:%d:%d", &date.tm_year, &date.tm_mon, &date.tm_mday, &date.tm_hour, &date.tm_min, &date.tm_sec); } date.tm_year -= 1900; date.tm_mon -= 1; date.tm_isdst = -1; time_t time = mktime(&date); getSunPos(time); return 0; }