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Daylight
Applet
/
Tageslicht-Applet
The
graphic lines for sunrise, sunset and twilight times don't take into
account daylight saving time.
During Daylight Savings the lines shift up by 1 hour, except for the
Sun position marker.
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Select
your
location
from
the
menu
list, |
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in the location database (Heavens Above): 2 million towns and villages world-wide, or in my small database here Enter latitude in decimal degrees and press return key,
enter longitude in decimal degrees and press return key. |
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Find the time zone (and Coordinates) of cities worldwide: The World Clock Interactive time zone map of countries around the world. |
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you
may
use
the
keys "h", "d", "m" to increase
the hour, date, or month, |
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you may enter your home location and change the horizon view image |
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can be written to a data window |
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Select from the menu to see the horizon at the selected location and time, or the word map showing day and night regions, or the sunshine hours per month. |
Compare:
Night
Hours Applet
Compare: Solstice Daylight Applet
Select
"Month" or "Year" from the "Write..." menu to open the data
window
showing sunrise, sunset and twilight times:


Select "Summary Year" from the "Write..." menu:

The
longest
day
(sommer
solstice)
is
not
the day of
earliest surise and/or latest sunset,
the shortest
day (winter
solstice) is not the day of latest
surise and/or earliest
sunset !
Select "Seasons" from the "Write..." menu:

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Daylight
hours
2005
Berlin
(52.51°
N):
mean of 12.29 hours per day, total 4485.56 hours.

Daily
difference
of
daylight
2005
Berlin
(52.51° N):
near the equinoxes the
absulute difference is a maximum (4 minutes).

Select "Duration of Sunlight" from the
"View" menu (calculating for 1 or 2 minutes):
Duration of
Sunlight depending on the Date and the Latitude
Computed using the diurnal arc of the Sun (arc
described by the Sun while
above the horizon):
α = arcos((cos(z)-sin(latitude)*sin(declination)/(cos(latitude)*cos(declination))
z=distance from the zenith (90.833° at rise/set)
duration of daylight:
T=2*(α/360°)*24h

Difference
of
daylight
per
week
2005
Berlin (52.51° N):
near the equinoxes the
absulute difference is a maximum (30 minutes).
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Due to the excentricity of the Earth's path, the percentage of daylight hours over a year is greater than 50 % for all latitudes ! (semidiameter of the Sun and atmospheric refraction taken into account).
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The latest sunrise and the earliest sunset do not occur on the day of winter solstice. The dates are different and depend on the geographical latitude.
The sunrise/sunset diagram is for Berlin (52.51° N, 13.41° E): Latest
sunrise
(2002): Earliest
sunset
(2002): For higher northern latitudes the date of latest sunrise will be earlier, and the date of earliest sunset will be later. |
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Shortest
day:
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Longest
day
2004: |
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Earliest
sunrise
2004: |
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Latest
sunset
2004: |
Look for details and explanations:
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civil twilight: nautical twilight: astronomical twilight: |
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twilight diagram
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Twilight duration at 0° N (minutes before rise):
Twilight duration at 30° N (minutes before rise):
Twilight duration at 60° N (minutes before rise): |
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the elevation (above horizon) and azimuth angle of the sun 0º = N, 90º = E
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enter latitude, and press
return key |
- degrees latitude as |
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enter longitude, and press
return key |
- degrees longitude as a |
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Look up your coordinates: |
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The coordinates of the user location are stored (during applet lifetime) and can be recalled by the location menu item "User Input". |
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Change the parameter values of "location", "latitude" and "longitude" parameters:
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<APPLET CODE="daylightxxx.class"
archive="Applet/JavaClasses.jar" <PARAM name="email" value="replace"> </APPLET> |
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time difference between zone time and Greenwich Time (GMT ) e.g. -5 h is the value computed from the longitude, which may differ from the actual time zone offset. If necessary, select the correct time zone offset from the menu. |
Central European Daylight Time = GMT + 2 hours |
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the declination and Greenwich-Hour-Angle (GHA) are the coordinates (latitude and longitude) of the sun's Geographical Position (GP), where the line from the sun to the centre of the earth intersects it's surface.
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The Equation of time is the difference between the time determined by a sundial and the clock time. It is due to the obliquity and the unequal motion of the sun (ellipse). |
For detailed information: |
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The total of daylight hours per month and per year is written to the diagram. |
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Length of Day (Herbert
Glarner) Comparative Lengths of
Days and Nights Frühester Sonnenuntergang, kürzester Tag, spätester Sonnenaufgang - ein Rätsel? |
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Last
Modified:
2010,
Jan 02