A.
-

Latitude of the city of your choice (31.75N for Jerusalem) = a, (minus sign for Southern Latitudes.)
Declination of the sun (any value between +23.5 and -23.5. Use the declination curve vs. the day # of the year. ) = delta

The length of the day from sunrise to sunset is hours, and minutes. Note that when you do not get a numerical value, the day length is 24 hours.

The length of the day was calculated by doubling the equation for the Hour Angle H between a transit of the sun and sunset:

H (of sunset) = arccos ( - tan(a)*tan(delta) ) .

B.
-

Latitude of the city of your choice = a, (minus sign for Southern Latitudes.)
Declination of the sun (any value between +23.5 and -23.5) = delta

The length of the day from the apparent sunrise to the apparent sunset becomes hours, and minutes.

The length of the day was calculated by doubling the equation for the Hour Angle H between a transit of the sun and the apparent sunset (or sunrise):

H (of sunset) = arccos (( cos (z) - sin(a)*sin(delta)) / (cos(a)*cos(delta)) ) .

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C.
-

Latitude of the city of your choice = a, (minus sign for Southern Latitudes.)
Type 4 digits for the year : ,
type 1 or 2 digits for the month : ,
and type 1 or 2 digits for the day of the month : .

The length of the day from the apparent sunrise to the apparent sunset becomes hours, and minutes.


Other Cities
CITY LATITUDE (N) LONGITUDE (E)
London 51 0
Tel Aviv 32 35
Cairo 30 31
Wien 48 16
New York 41 -74 (74W)
Tokyo 35 140
Singapore 1 104
Manila 14 121
Bangkok 13 100
Anchorage (ALASKA) 61.2 -150
Tucson 32.25 -110.95
Addis Ababa 9 39
Phoenix 33.5 -112.05

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Prepared by A.C. from the


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