46° halo

A 46° halo is a rare member of the family of ice crystal halos, appearing as a large ring centred on the Sun at roughly twice the distance as the much more common 22° halo. At solar elevations of 15–27°, the 46° halo is often confused with the less rare and more colourful supralateral and infralateral arcs, which cross the parhelic circle at about 46° to the left and right of the sun.[1]

Sun dogs with a larger and fainter 46° halo and a 22° halo with an upper tangent arc

The 46° halo is similar to, but much larger and fainter than, the more common 22° halo. It forms when sunlight enters randomly oriented hexagonal ice crystals through a prism face and exits through a hexagonal base.[2] The 90° inclination between the two faces of the crystals causes the colours of the 46° halo to be more widely dispersed than those of the 22° halo. In addition, as many rays are deflected at larger angles than the angle of minimum deviation, the outer edge of the halo is more diffuse.[3]

To tell the difference between a 46° halo and the infralateral or supralateral arcs, one should carefully observe sun elevation and the fluctuating shapes and orientations of the arcs. The supralateral arc always touches the circumzenithal arc, while the 46° halo only achieves this when the sun is located 15–27° over the horizon, leaving a gap between the two at other elevations. In contrast, supralateral arcs cannot form when the Sun is over 32°, so a halo in the 46°-region is always a 46° halo at higher elevations. If the Sun is near the zenith, however, circumhorizontal or infralateral arcs are located 46° under the Sun and can be confused with the 46° halo. [4][5]

ReferencesEdit

  1. ^ The 46° halo was first explained as being caused by refractions through ice crystals in 1679 by the French physicist Edmé Mariotte (1620–1684). See: Mariotte, Quatrieme Essay. De la Nature des Couleur (Paris, France: Estienne Michallet, 1681). Sun dogs as well as the 22° and 46° halos are explained in terms of refractions from ice crystals on pages 466–524.
  2. ^ "46°-halo". Arbeitskreis Meteore e.V. Archived from the original on 31 March 2007. Retrieved 2007-04-16.
  3. ^ Les Cowley (?). "46° Halo Formation". Atmospheric Optics. Retrieved 2007-04-16. (including an illustration and an animation)
  4. ^ Les Cowley (?). "Is it a 46° halo or a supra/infralateral arc?". Atmospheric Optics. Retrieved 2007-04-16.
  5. ^ "Supralateral arc". Arbeitskreis Meteore e.V. Retrieved 2007-04-16.

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