diff options
Diffstat (limited to 'src/calendar.cpp')
-rw-r--r-- | src/calendar.cpp | 77 |
1 files changed, 30 insertions, 47 deletions
diff --git a/src/calendar.cpp b/src/calendar.cpp index 8af1851..6731692 100644 --- a/src/calendar.cpp +++ b/src/calendar.cpp | |||
@@ -7,36 +7,47 @@ | |||
7 | /*以下为"calendar.h规定之量*/ | 7 | /*以下为"calendar.h规定之量*/ |
8 | double day = 86400; | 8 | double day = 86400; |
9 | double delta = 1e-11; | 9 | double delta = 1e-11; |
10 | |||
11 | /*计算需要用的类的实例化*/ | ||
12 | Julian julian; | 10 | Julian julian; |
13 | parameter p; | 11 | parameter p; |
14 | 12 | ||
15 | void radToDMS(const char *message, int lowerBound, int upperBound, | 13 | pair<double, double> getSunPos(time_t time) { |
16 | double radians) { | 14 | double t = julian.getJulianKiloYear(time); |
17 | // Convert radians to degrees | ||
18 | double degrees = radians * 180.0 / M_PI; | ||
19 | 15 | ||
20 | while (degrees < lowerBound) | 16 | pair<double, double> sun = p.sun_longitude(t); |
21 | degrees += (upperBound - lowerBound); | 17 | radToDMS("Sun longitude:\t\t", 0, 360, sun.first); |
22 | while (degrees >= upperBound) | 18 | radToDMS("Sun latitude:\t\t", -90, 90, sun.second); |
23 | degrees -= (upperBound - lowerBound); | ||
24 | 19 | ||
25 | // Calculate degrees, minutes, and seconds | 20 | double alpha, delta; // 太阳赤经赤纬 |
26 | int deg = static_cast<int>(degrees); | 21 | double lambda = sun.first, beta = sun.second; // 太阳黄经黄纬 |
27 | double min_sec = (degrees - deg) * 60.0; | 22 | // 黄赤交角epsilon |
28 | int min = static_cast<int>(min_sec); | 23 | double epsilon = p.get_epsilon(t); |
29 | double sec = (min_sec - min) * 60.0; | 24 | radToDMS("Ecliptic Obliquity:\t\t", 0, 90, epsilon); |
30 | 25 | ||
31 | // Output the result | 26 | delta = |
32 | printf("%s: %d°%d'%06.3f''\n", message, deg, min, sec); | 27 | asin(sin(epsilon) * sin(lambda) * cos(beta) + cos(epsilon) * sin(beta)); |
28 | alpha = atan2( | ||
29 | (cos(epsilon) * sin(lambda) * cos(beta) - sin(epsilon) * sin(beta)), | ||
30 | (cos(lambda) * cos(beta))); | ||
31 | radToDMS("Sun right ascension:\t\t", 0, 360, alpha); | ||
32 | radToDMS("Sun declination:\t\t", -90, 90, delta); | ||
33 | // 时角 | ||
34 | double H = p.getHourAngle(t, LONGITUDE, LATITUDE, alpha); | ||
35 | double A, h; //方位角和高度角 | ||
36 | h = asin(sin(LATITUDE) * sin(delta) + cos(LATITUDE) * cos(delta) * cos(H)); | ||
37 | A = atan2(-cos(delta) * sin(H), | ||
38 | cos(LATITUDE) * sin(delta) - sin(LATITUDE) * cos(delta) * cos(H)); | ||
39 | A += M_PI; | ||
40 | // 转换为角度制输出 | ||
41 | radToDMS("Hour angle:\t\t", 0, 360, H); | ||
42 | radToDMS("Azimuth:\t\t", 0, 360, A); | ||
43 | radToDMS("Elevation:\t\t", -90, 90, h); | ||
33 | } | 44 | } |
34 | 45 | ||
35 | int main(int argc, char *argv[]) { | 46 | int main(int argc, char *argv[]) { |
36 | Date date; | 47 | Date date; |
37 | if (argc != 2) { | 48 | if (argc != 2) { |
38 | printf("Input the time you want to calculate in <YYYY-MM-DD,HH:MM:SS> " | 49 | printf("Input the time you want to calculate in <YYYY-MM-DD,HH:MM:SS> " |
39 | "format: "); | 50 | "format:\t\t"); |
40 | scanf("%d-%d-%d,%d:%d:%d", &date.tm_year, &date.tm_mon, &date.tm_mday, | 51 | scanf("%d-%d-%d,%d:%d:%d", &date.tm_year, &date.tm_mon, &date.tm_mday, |
41 | &date.tm_hour, &date.tm_min, &date.tm_sec); | 52 | &date.tm_hour, &date.tm_min, &date.tm_sec); |
42 | } else { | 53 | } else { |
@@ -48,34 +59,6 @@ int main(int argc, char *argv[]) { | |||
48 | date.tm_isdst = -1; | 59 | date.tm_isdst = -1; |
49 | 60 | ||
50 | time_t time = mktime(&date); | 61 | time_t time = mktime(&date); |
51 | double t = julian.getJulianKiloYear(time); | 62 | getSunPos(time); |
52 | |||
53 | pair<double, double> sun = p.sun_longitude(t); | ||
54 | radToDMS("Sun longitude: ", 0, 360, sun.first); | ||
55 | radToDMS("Sun latitude: ", -90, 90, sun.second); | ||
56 | |||
57 | double alpha, delta; // 太阳赤经赤纬 | ||
58 | double lambda = sun.first, beta = sun.second; // 太阳黄经黄纬 | ||
59 | // 黄赤交角epsilon,23°26'21.448''转换为弧度 | ||
60 | double epsilon = (23.0 + 26.0 / 60.0 + 21.448 / 3600.0) * M_PI / 180.0; | ||
61 | |||
62 | delta = | ||
63 | asin(sin(epsilon) * sin(lambda) * cos(beta) + cos(epsilon) * sin(beta)); | ||
64 | alpha = atan2( | ||
65 | (cos(epsilon) * sin(lambda) * cos(beta) - sin(epsilon) * sin(beta)), | ||
66 | (cos(epsilon) * cos(beta))); | ||
67 | radToDMS("Sun right ascension: ", 0, 360, alpha); | ||
68 | radToDMS("Sun declination: ", -90, 90, delta); | ||
69 | // 时角 | ||
70 | double H = p.getHourAngle(t, LONGITUDE, LATITUDE, alpha); | ||
71 | double A, h; //方位角和高度角 | ||
72 | h = asin(sin(LATITUDE) * sin(delta) + cos(LATITUDE) * cos(delta) * cos(H)); | ||
73 | A = atan2(-cos(delta) * sin(H), | ||
74 | cos(LATITUDE) * sin(delta) - sin(LATITUDE) * cos(delta) * cos(H)); | ||
75 | A += M_PI; | ||
76 | // 转换为角度制输出 | ||
77 | radToDMS("Hour angle: ", 0, 360, H); | ||
78 | radToDMS("Azimuth: ", 0, 360, A); | ||
79 | radToDMS("Elevation: ", 0, 90, h); | ||
80 | return 0; | 63 | return 0; |
81 | } | 64 | } |