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  2. Atmospheric optics - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_optics

    Cloud droplets tend to scatter light efficiently, so that the intensity of the solar radiation decreases with depth into the gases. As a result, the cloud base can vary from a very light to very dark grey depending on the cloud's thickness and how much light is being reflected or transmitted back to the observer.

  3. Starlight - Wikipedia

    en.wikipedia.org/wiki/Starlight

    One of the oldest stars yet identified - oldest but not most distant in this case - was identified in 2014: while "only" 6,000 light years away, the star SMSS J031300.36−670839.3 was determined to be 13.8 billion years old, or more or less the same age as the universe itself. [9] The starlight shining on Earth includes this star. [9]

  4. Rayleigh sky model - Wikipedia

    en.wikipedia.org/wiki/Rayleigh_sky_model

    From the polarization patterns, these species can orient themselves by determining the exact position of the Sun without the use of direct sunlight. Thus under cloudy skies, or even at night, animals can find their way. Using polarized light as a compass however is no easy task. The animal must be capable of detecting and analyzing polarized light.

  5. Cloudy skies? Social media reacts to upcoming total solar ...

    www.aol.com/cloudy-skies-social-media-reacts...

    A solar eclipse happens when the moon passes between the sun and Earth, either fully or partially blocking the sun's light and casting a temporary shadow on Earth, according to NASA.

  6. Solar flares vs. coronal mass ejections: Here's which once ...

    www.aol.com/solar-flares-vs-coronal-mass...

    Here's the possibility of seeing the northern lights. ... Coronal mass ejection vs. solar flare: 1 gives us the aurora borealis. Show comments. Advertisement. Advertisement.

  7. Orders of magnitude (illuminance) - Wikipedia

    en.wikipedia.org/wiki/Orders_of_magnitude...

    Cloudy night sky without moon [4] 400 μcd/m 2 "Darkest sky" [5] 1 mcd/m 2: Night sky [6] 1.4 mcd/m 2: Typical photographic scene lit by full moon [7] 10 −2: 5 mcd/m 2: Approximate scotopic/mesopic threshold [8] 10 −1: 10 0: cd/m 2: 2 cd/m 2: Floodlit buildings, monuments, and fountains [9] 10 1: 5 cd/m 2: Approximate mesopic/photopic ...

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