I thought it might be interesting to derive a formula to find the amount of daylight throughout the year. In what follows θ and φ indicate the latitude and longitude of the Sun and a location on the Earth's surface. The subscripts, S and L are used to distinguish the two sets of coordinates. Z indicates a location and its zenith direction. P is the pole of the Earth's rotation, M a point on the Equator through which the location's meridian passes and M' is another meridian which is 90° to the east of M.
Using these quantities we can specify both the position of some location and the relative position of the Sun. The Sun is above the horizon when the projection of the two directions onto each other is positive. This condition gives in an equation involving three angles.

The times of sunrise and sunset depend on the latitudes of Sun, θ_S, and the location, θ_L, and the difference between these times, Δt, is known if Δφ is known. For the day with longest daylight the Sun is over the Tropic of Cancer and its latitude is 23.44°. At the latitude of Rhodes, 36°, this gives the maximum amount of daylight as being 14.4 hours which is in good agreement with Ptolemy's value. One can also reverse the procedure and estimate the latitude if the maximum amount of daylight is known.
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