Alpenglow
Alpenglow (from Template:Langx; Template:Langx) is an optical phenomenon that appears as a horizontal reddish glow near the horizon opposite to the Sun when the solar disk is just below the horizon.<ref name=LynchLivingston2001>Template:Cite book</ref>
DescriptionEdit
Strictly speaking, alpenglow refers to indirect sunlight reflected or diffracted by the atmosphere after sunset or before sunrise. This diffuse illumination creates soft shadows in addition to the reddish color. The term is also used informally to include direct illumination by the reddish light of the rising or setting sun, with sharply defined shadows.
Reflected sunlightEdit
When the Sun is below the horizon, sunlight has no direct path to reach a mountain. Unlike the direct sunlight around sunrise or sunset, the light that causes alpenglow is reflected off airborne precipitation, ice crystals, or particulates in the lower atmosphere. These conditions differentiate between direct sunlight around sunrise or sunset and alpenglow.<ref name="CD-20091228">Template:Cite news</ref>
The term is generally confused to be any sunrise or sunset light reflected off the mountains or clouds, but alpenglow in the strict sense of the word is not direct sunlight and is only visible after sunset or before sunrise.<ref name=LynchLivingston2001/>
After sunset, if mountains are absent, aerosols in the eastern sky can be illuminated in a similar way by the remaining scattered reddish light above the fringe of Earth's shadow. This backscattered light produces a pinkish band opposite of the Sun's direction, called the Belt of Venus.<ref name="Powell 2018 pp. 105–130">Template:Cite book</ref>
Direct sunlightEdit
Alpenglow in a looser sense may refer to any illumination by the rosy or reddish light of the setting or rising Sun.<ref name=DigitalPhotographySchool>Template:Cite news</ref><ref>Template:Cite dictionary</ref>