Corona (optical phenomenon)

File:Lunar-coronae.jpg

A lunar corona

File:Lunar corona.JPG

Lunar aureole as seen from Mumbai, India.

File:SolarDiffractionCorona.jpg

A solar corona soon after sunrise

In meteorology, a corona (plural coronae) is an optical phenomenon produced by the diffraction of light from the Sun or the Moon (or, occasionally, bright stars or planets) by individual small water droplets and sometimes tiny ice crystals of a cloud or on a foggy glass surface. In its full form, a corona consists of several concentric, pastel-colored rings around the celestial object and a central bright area called aureole. The aureole is often (especially in case of the Moon) the only visible part of the corona and has the appearance of a bluish-white disk which fades to reddish-brown towards the edge. The angular size of a corona depends on the diameters of the water droplets involved: Smaller droplets produce larger coronae. For the same reason, the corona is the most pronounced when the size of the droplets is most uniform. Coronae differ from halos in that the latter are formed by refraction (rather than diffraction) from comparatively large rather than small ice crystals.

See also

• Atmospheric diffraction
• Glory

External links

• Explanation and image gallery - Atmospheric Optics by Les Cowley
• Rings around the sun and moon: coronae and diffraction
• Corona from Fogged Eyeglasses
• Experimental simulations of pollen coronas
• The Corona

File:Janus24.jpg

Lunar corona with Altocumulus floccus

Gallery

• Coronae.jpg

  Forest Corona

• Solar coronae reflection.jpg

  Reflection of solar corona

• Coronae at GGB.jpg

  Solar Corona at Golden Gate Bridge

• Iridescent fog.jpg

  Partial Corona at Golden Gate Bridge

• Moon Marki 19032011 3.JPG

  Moon