Parhelic circle

File:Halo and sun dog - NOAA.jpg

A crisp parhelic circle (horizontal line) over South Pole Station.
Photo: John Bortniak, NOAA, January 1979.

A halo phenomenon observed over the South Pole. Featured in the photo are several distinct phenomena: A parhelic circle (horizontal line), a 22° halo (circle) with two sundogs (bright spots), and an upper tangent arc.
Photo: Cindy McFee, NOAA, December 1980.

A parhelic circle is a halo, an optical phenomenon appearing as a horizontal white line on the same altitude as the sun, or occasionally the Moon. If complete, it stretches all around the sky, but more commonly it only appears in sections.

Even fractions of parhelic circles are less common than sun dogs and 22° halos. While parhelic circles are generally white in colour because they are produced by reflection, they can however show a bluish or greenish tone near the 120° parhelia and be reddish or deep violet along the fringes.

Parhelic circles form as beams of sunlight are reflected by vertical or almost vertical hexagonal ice crystals. The reflection can be either external (e.g. without the light passing through the crystal) which contributes to the parhelic circle near the sun, or internal (one or more reflections inside the crystal) which creates much of the circle away from the sun. Because an increasing number of reflections makes refraction asymmetric some colour separation occurs away from the sun. Sun dogs are always aligned to the parhelic circle (but not always to the 22° halo).

The intensity distribution of the parhelic circle is largely dominated by 1-3-2 and 1-3-8-2 rays (cf. the nomenclature by W. Tape, i.e. 1 denotes the top hexagonal face, 2 the bottom face, and 3-8 enumerate the side faces in counter-clockwise fashion. A ray is notated by the sequence in which it encounters the prism faces). The former ray-path is responsible for the blue spot halo which occurs at an azimuth

$\theta_{\mathfrak{1}\mathfrak{3}\mathfrak{2}}=2\arcsin\left(n\cos\left(\arcsin\left(1/n\right)\right)/\cos\left(e\right)\right)$,

with $n$ being the material's index of refraction (not the Bravais index of refraction for inclined rays). However, many more features give a structure to the intensity pattern of the parhelic circle. Among the features of the parhelic circle are the Liljequist parhelia, the 90° parhelia (likely unobservable), the second order 90° parhelia (unobservable), the 22° parhelia and more.

See also

• Lower tangent arc
• Upper tangent arc
• Circumzenithal arc
• Liljequist parhelion

External links

• Atmospheric Optics - Ice Halos