aboutsummaryrefslogtreecommitdiff
path: root/src/sun.c
diff options
context:
space:
mode:
authoraxtloss <axtlos@disroot.org>2024-05-28 13:01:13 +0200
committeraxtloss <axtlos@disroot.org>2024-05-28 13:01:13 +0200
commitb666cb3b757b408c9515b4749c7e8a05971ec451 (patch)
tree67f313f43f73205f987943a9e2cb6b367d0eb913 /src/sun.c
downloadautodarkmode-b666cb3b757b408c9515b4749c7e8a05971ec451.tar.gz
autodarkmode-b666cb3b757b408c9515b4749c7e8a05971ec451.tar.bz2
add files
Diffstat (limited to 'src/sun.c')
-rw-r--r--src/sun.c156
1 files changed, 156 insertions, 0 deletions
diff --git a/src/sun.c b/src/sun.c
new file mode 100644
index 0000000..f08dfd8
--- /dev/null
+++ b/src/sun.c
@@ -0,0 +1,156 @@
+#include <math.h>
+#include <glib.h>
+#define PI 3.1415926
+#define ZENITH -.83
+
+float calculateSunrise(int year,int month,int day,float lat, float lng,int localOffset) {
+ /*
+ localOffset will be <0 for western hemisphere and >0 for eastern hemisphere
+ daylightSavings should be 1 if it is in effect during the summer otherwise it should be 0
+ */
+ //1. first calculate the day of the year
+ float N1 = floor(275 * month / 9);
+ float N2 = floor((month + 9) / 12);
+ float N3 = (1 + floor((year - 4 * floor(year / 4) + 2) / 3));
+ float N = N1 - (N2 * N3) + day - 30;
+
+ //2. convert the longitude to hour value and calculate an approximate time
+ float lngHour = lng / 15.0;
+ float t = N + ((6 - lngHour) / 24);
+
+ //3. calculate the Sun's mean anomaly
+ float M = (0.9856 * t) - 3.289;
+
+ //4. calculate the Sun's true longitude
+ float L = fmod(M + (1.916 * sin((PI/180)*M)) + (0.020 * sin(2 *(PI/180) * M)) + 282.634,360.0);
+
+ if ( L < 0 )
+ L = L+360;
+ else if ( L > 360)
+ L = L-360;
+
+ //5a. calculate the Sun's right ascension
+ float RA = fmod(180/PI*atan(0.91764 * tan((PI/180)*L)),360.0);
+
+ if ( RA < 0 )
+ RA = RA+360;
+ else if ( RA > 360)
+ RA = RA-360;
+
+ //5b. right ascension value needs to be in the same quadrant as L
+ float Lquadrant = floor( L/90) * 90;
+ float RAquadrant = floor(RA/90) * 90;
+ RA = RA + (Lquadrant - RAquadrant);
+
+ //5c. right ascension value needs to be converted into hours
+ RA = RA / 15;
+
+ //6. calculate the Sun's declination
+ float sinDec = 0.39782 * sin((PI/180)*L);
+ float cosDec = cos(asin(sinDec));
+
+ //7a. calculate the Sun's local hour angle
+ float cosH = (sin((PI/180)*ZENITH) - (sinDec * sin((PI/180)*lat))) / (cosDec * cos((PI/180)*lat));
+
+ if (cosH > 1)
+ g_print("Never rising\n");
+ else if (cosH < -1)
+ g_print("Never setting\n");
+
+ //7b. finish calculating H and convert into hours
+ float H = 360 - (180/PI)*acos(cosH); // if if rising time is desired:
+
+ H = H / 15;
+
+ //8. calculate local mean time of rising/setting
+ float T = H + RA - (0.06571 * t) - 6.622;
+
+ //9. adjust back to UTC
+ float UT = fmod(T - lngHour,24.0);
+
+ if ( UT < 0 )
+ UT = UT+24;
+ else if (UT > 24)
+ UT = UT-24;
+
+ //10. convert UT value to local time zone of latitude/longitude
+ return UT + localOffset;
+
+ }
+
+float calculateSunset(int year,int month,int day,float lat, float lng,int localOffset) {
+ /*
+ localOffset will be <0 for western hemisphere and >0 for eastern hemisphere
+ daylightSavings should be 1 if it is in effect during the summer otherwise it should be 0
+ */
+ //1. first calculate the day of the year
+ float N1 = floor(275 * month / 9);
+ float N2 = floor((month + 9) / 12);
+ float N3 = (1 + floor((year - 4 * floor(year / 4) + 2) / 3));
+ float N = N1 - (N2 * N3) + day - 30;
+
+ //2. convert the longitude to hour value and calculate an approximate time
+ float lngHour = lng / 15.0;
+
+ float t = N + ((18 - lngHour) / 24); //if setting time is desired:
+
+ //3. calculate the Sun's mean anomaly
+ float M = (0.9856 * t) - 3.289;
+
+ //4. calculate the Sun's true longitude
+ float L = fmod(M + (1.916 * sin((PI/180)*M)) + (0.020 * sin(2 *(PI/180) * M)) + 282.634,360.0);
+
+ if ( L < 0 )
+ L = L+360;
+ else if ( L > 360)
+ L = L-360;
+
+ //5a. calculate the Sun's right ascension
+ float RA = fmod(180/PI*atan(0.91764 * tan((PI/180)*L)),360.0);
+
+ if ( RA < 0 )
+ RA = RA+360;
+ else if ( RA > 360)
+ RA = RA-360;
+
+ //5b. right ascension value needs to be in the same quadrant as L
+ float Lquadrant = floor( L/90) * 90;
+ float RAquadrant = floor(RA/90) * 90;
+ RA = RA + (Lquadrant - RAquadrant);
+
+ //5c. right ascension value needs to be converted into hours
+ RA = RA / 15;
+
+ //6. calculate the Sun's declination
+ float sinDec = 0.39782 * sin((PI/180)*L);
+ float cosDec = cos(asin(sinDec));
+
+ //7a. calculate the Sun's local hour angle
+ float cosH = (sin((PI/180)*ZENITH) - (sinDec * sin((PI/180)*lat))) / (cosDec * cos((PI/180)*lat));
+
+ if (cosH > 1)
+ g_print("Never rising\n");
+ else if (cosH < -1)
+ g_print("Never setting\n");
+
+
+ //7b. finish calculating H and convert into hours
+
+ float H = (180/PI)*acos(cosH); // if setting time is desired:
+ H = H / 15;
+
+ //8. calculate local mean time of rising/setting
+ float T = H + RA - (0.06571 * t) - 6.622;
+
+ //9. adjust back to UTC
+ float UT = fmod(T - lngHour,24.0);
+
+ if ( UT < 0 )
+ UT = UT+24;
+ else if (UT > 24)
+ UT = UT-24;
+
+ //10. convert UT value to local time zone of latitude/longitude
+ return UT + localOffset;
+
+}