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   » Wiki: Sunlight
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Sunlight is the portion of the electromagnetic radiation which is emitted by the (i.e. solar radiation) and received by the , in particular the light perceptible to the as well as invisible (typically perceived by humans as warmth) and (which can have physiological effects such as ) lights. However, according to the American Meteorological Society, there are "conflicting conventions as to whether all three ... are referred to as light, or whether that term should only be applied to the visible portion of the spectrum". Upon reaching the Earth, sunlight is scattered and through the Earth's atmosphere as when the Sun is above the . When direct is not blocked by , it is experienced as sunshine, a combination of bright and (atmospheric). When or reflected off other objects, sunlight is diffused. Sources estimate a global average of between 164 watts to 340 watts per square meter over a 24-hour day; this figure is estimated by NASA to be about a quarter of Earth's average total solar irradiance.

The ultraviolet radiation in sunlight has both positive and negative health effects, as it is both a requisite for vitamin D3 synthesis and a .

Sunlight takes about 8.3 minutes to reach Earth from the surface of the Sun.

(2025). 9780521546225, Cambridge University Press. .
Extract of page 56 A photon starting at the center of the Sun and changing direction every time it encounters a would take between 10,000 and 170,000 years to get to the surface.

Sunlight is a key factor in , the process used by plants and other organisms to convert , normally from the Sun, into that can be used to synthesize carbohydrates and fuel the organisms' activities.

Daylighting is the natural lighting of interior spaces by admitting sunlight. is the rate of solar energy received by a unit area from sunlight.


Measurement
Researchers can measure the intensity of sunlight using a sunshine recorder, , or . To calculate the amount of sunlight reaching the ground, both the eccentricity of Earth's and the attenuation by Earth's atmosphere have to be taken into account. The extraterrestrial solar illuminance (), corrected for the elliptic orbit by using the day number of the year (dn), is given to a good approximation by
E_{\rm ext}= E_{\rm sc} \cdot \left(1+0.033412 \cdot \cos\left(2\pi\frac

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