Notes
This page calculates the times of sunrise and sunset on any date,
accurate to the minute within several centuries of the present. It
correctly describes what happens in the Arctic and Antarctic regions,
where the Sun may not rise or set on a given date. The program was
adapted from a BASIC program in Sky & Telescope magazine, August
1994, page 84,
Sunrise occurs when the rotation of the Earth causes the upper
limb of the Sun to move above the visible horizon as seen by an
observer on the Earth's surface. Sunset is similar, occurring when
the upper limb of the Sun moves below the visible horizon. The mathematical
model of the Sun's apparent motion in the sky gives the position
of the center of the Sun as it would be seen from the center of
the Earth. Because the Sun is very distant from the Earth, it is
not necessary to correct for parallax, the angular offset due observation
from the Earth's surface. However, it is necessary to account for
the visual radius of the Sun since the position of the upper limb
determines sunset and sunrise. Additionally, the Earth's atmosphere
refracts light noticeably for light source near the horizon. This
calculator includes corrections that account for both of these under
average conditions. Actual observations of sunset and sunrise may
differ from the predicted times due to variations in atmospheric
conditions and due to local topography.
The predicted times are given in local time, standard or daylight
saving, obtained from your computer's operating system. The azimuth
of sunrise and sunset is given, measured in degrees from true North.
You must determine your correct latitude and longitude to obtain
valid predictions for your location
Copyright © 2004, Stephen R. Schmitt
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