This page is devoted to atmospheric effects. All photographs presented in this section have been taken by the authors with digital DSLR, mirrorless, compact and analog cameras. For some sunrise or sunset images, relatively long focal lengths have been required, like telescopes.
WARNING : Never view the sun through optical instruments like telescopes or binoculars without reducing light intensity with appropriate filters. Irreversible eye damage may result!
· Sunrise on the Bernese Alps observed from Prêles, Switzerland on January 5, 2020.
© Michel Willemin
· Collection of images taken during the same sunrise.
Exp 1/1000, 1/4000, 1/4000, 1/4000s, f/11, 11, 11, 18, ISO 400, UTC 7:24, 7:26, 7:27, 7:27, respectively. © Michel Willemin
· Sunset observed from the Croatian island of Lošinj and offering a tiny Green Flash!
July 19, 2019, from Otok Lošinj direction Otok Unije (Croatia). © Michel Willemin
· Rainbow, sundog and sunrise observed from Prêles, Switzerland
Images taken on July 25, 2017, on October 10, 2017 and on January 5, 2018 respectively. © Michel Willemin
Respective publications in Journal du Jura on July 27, 2017, on October 14, 2017 and on January 6, 2018.
· Eruptive sunrise over the Schreckhorn (4078m) observed from Prêles, Switzerland
Images taken on December 25, 2015 @ 7:25 UTC. © Michel Willemin
Image taken from Affoltern am Albis (Switzerland), September 2001. © M. Willemin
Parhelia or sundogs are the brightest and most common halo that originates in an oriented crystal. They are found on either side of the sun at the same altitude and tend to show bright colors. They are red on their sunward side and fainter and more bluish away from the sun. At low altitudes parhelia are found 22° from the sun but at higher altitudes they separate from it.
· Rainbows images
© M. Willemin
The second photograph has been taken just before the sunset, which explains the red dominent.
· Rainbows "theory"
This very interesting, natural and nice effect is due to the refraction and dispersion of the light through the water drops. Sun and rain together is the condition for rainbows. The primary rainbow is easy to observe. It results from a single internal reflexion and two refraction of the light of the sun in water drops. The index of refraction of water depends on the wavelength (dispersion), which produces a decomposition of the light during the two refraction processes, like a prism. Under good conditions, a secondary rainbow can also be observed (see second photograph). In this case, two internal reflexions of light within the water drops occur. The intensity of the secondary rainbow is much lower than for the primary or main rainbow.
For calculating your own rainbow online, click HERE !
|Wavelength (nm)||Index n||Primary angle (°)||Secondary angle (°)|
· Collection of sunsets
© M. Willemin
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