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A contour plot of the hours of daylight as a function of latitude and day of the year, using the most accurate models described in this article. It can be seen that the area of constant day and constant night reach up to the polar circles (here labeled "Anta. c." and "Arct. c."), which is a consequence of the earth's inclination.
English: Blue (#0072B2) indicates regions that change clocks between daylight saving time in summer and standard time in winter (48 states, the District of Columbia, and the Navajo Nation). Orange (#E69F00) indicates regions that observe permanent standard time (Hawaii, all five inhabited U.S. territories, and all of Arizona outside of the ...
The graph is nonscientific; roughly adopted from Image:Daylight.png, in addition the graph form (yearly average) and the additional shadow area was assumed from Daylight Time Map, DaylightMap png and ConstructAfrique. Author: Melancholie: Permission (Reusing this file) GNU-FDL and CC-BY-SA: Other versions
World map showing the areas of Earth receiving daylight around 13:00 UTC in April. Daylight is the combination of all direct and indirect sunlight during the daytime.This includes direct sunlight, diffuse sky radiation, and (often) both of these reflected by Earth and terrestrial objects, like landforms and buildings.
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The United States Naval Observatory states "the Equation of Time is the difference apparent solar time minus mean solar time", i.e. if the sun is ahead of the clock the sign is positive, and if the clock is ahead of the sun the sign is negative. [6] [7] The equation of time is shown in the upper graph above for a period of slightly more than a ...
Earth daylight on the June solstice Earth daylight on the December solstice Daytime length or daytime duration is the time elapsed between beginning and end of the daytime period. Given that Earth's own axis of rotation is tilted 23.44° to the line perpendicular to its orbital plane , called the ecliptic , the length of daytime varies with the ...
A 2021 publication [8] about solar geometry first calculates the x-, y-, and z-component of the solar vector, which is a unit vector with its tail fixed at the observer's location and its head kept pointing toward the Sun, and then uses the components to calculate the solar zenith angle and solar azimuth angle. The calculated solar vector at 1 ...
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