07.03 Sunlight calculations
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Definitions
Definition | ||
Declination | The angle of the sun's rays to the equatorial plane, positive in summer. | |
Latitude | The angle from the equator to a position on Earth's surface. | |
Hour angle | The angle the Earth needs to rotate to bring the meridian to noon. Each hour of time is equivalent to 15 deg. | |
Altitude | The angle of the sun above the horizon plane. | |
Azimuth | The compass direction of the sun. May be measured in degrees clockwise from North, or degrees East or West of South. | |
Day Number | The day number, January 1st is 1. |
sin g = cos D x cos L x cos H + sin D x sin L
cos z = ( cos D x cos H x sin L - sin D x cos L ) / cos g
sin z = ( sin H x cos D ) / cos g
tan z = sin H / ( sin L x cos H - cos L x tan D )
cos Hg=0 = - tan D x tan L
Number of daylight hours = cos-1 ( - tan D x tan L ) x 2 /15 hours
Declination = 23.4 x sin [ 360 (284 + N ) / 365]
Using the convention, declination is positive in summer,
cos zg=0 = - sin D / cos L
gnoon = 90o - L + D
(see also this image)
gmidnight = L + D - 90o