Kern arc

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The Kern arc is the extremely rare atmospheric optical phenomenon related to the circumzenithal arc. It is a complete and faint circle around the zenith. In contrast, the related and much more common circumzenithal arc is only ever a partial circle.

The Kern arc is named after H. F. A. Kern in the Netherlands, who first reported it in 1895. Since then it has been reported on six occasions.[1]

It is formed by rays entering the top faces of horizontal plate crystals and leaving through a near vertical side face. Kern arc rays undergo an internal reflection off a side face inclined at 60 degrees to the exit face. Near triangular hexagonal crystals with three alternate side faces much shorter than the others allow Kern arc.

The first photographs of the Kern arc were taken by Marko Mikkilä close to Vuokatti Ski Resort Sotkamo, Finland on 17 November 2007.[2] The photographs were in natural sunlight taken from an artificial cloud created by snowguns.[1] At the Vuokatti Ski Resort about 100 snowguns may operate at one time. The temperature was −15 to −18 °C in clear sky and almost no wind. Nikon D70 and Nikon FM cameras were used with Sigma 8mm EX F4, Sigma 15mm EX F2.8 lenses. Some samples of ice crystals were also collected confirming their nearly triangular base.

Mikkiläs photographs were first published in Tähdet ja avaruus-magazine 1/2008. The magazine is published by URSA, the Finnish association of astronomy.

See also[edit]

References[edit]

  1. ^ a b Mikkilä, Marko (2008-01-27). "Kern arc photographed in Finland". Halo Reports (blog). URSA. Retrieved 2008-01-30.  (Mikkilä's description of the observation.)
  2. ^ Cowley, Les. "Kern Arc". Atmospheric Optics. Retrieved 2008-01-27.