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  2. Solar irradiance - Wikipedia

    en.wikipedia.org/wiki/Solar_irradiance

    Solar irradiance is the power per unit area ... Online insolation calculator This page was last edited on 9 December 2024, at 03:56 (UTC). Text is available ...

  3. Ultraviolet index - Wikipedia

    en.wikipedia.org/wiki/Ultraviolet_index

    When the UV index is presented on a daily basis, it represents UV intensity around the sun's highest point in the day, called solar noon, halfway between sunrise and sunset. This typically occurs between 11:30 and 12:30, or between 12:30 and 13:30 in areas where daylight saving time is being observed.

  4. Sun dog - Wikipedia

    en.wikipedia.org/wiki/Sun_dog

    Sun dogs typically appear as a pair of subtly colored patches of light, around 22° to the left and right of the Sun, and at the same altitude above the horizon as the Sun. They can be seen anywhere in the world during any season, but are not always obvious or bright. Sun dogs are best seen and most conspicuous when the Sun is near the horizon.

  5. Will your pets be safe during the solar eclipse? Here's what ...

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  6. Is it safe for dogs to be outside during a solar eclipse?

    www.aol.com/safe-dogs-outside-during-solar...

    Dog owners should be more worried about the festivities surrounding the eclipse than the event itself. “This is a big occasion. We’re going to turn this natural event into an unnatural event.

  7. Is it safe for pets to go outside during the solar eclipse?

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  8. Sunlight - Wikipedia

    en.wikipedia.org/wiki/Sunlight

    The solar constant is a measure of flux density, is the amount of incoming solar electromagnetic radiation per unit area that would be incident on a plane perpendicular to the rays, at a distance of one astronomical unit (AU) (roughly the mean distance from the Sun to Earth).

  9. Solar constant - Wikipedia

    en.wikipedia.org/wiki/Solar_constant

    The solar "constant" is not a physical constant in the modern CODATA scientific sense; that is, it is not like the Planck constant or the speed of light which are absolutely constant in physics. The solar constant is an average of a varying value. In the past 400 years it has varied less than 0.2 percent. [2]