22-degree halo 2026-10-20
The common optical halo has a radius of approximately around the Sun or Moon. Refraction through a ice-crystal prism supplies a minimum-deviation edge. Nearby incident directions are concentrated near that edge, forming a caustic.[ref]
Optical halo 2026-10-20
An optical halo is a ring, arc or other light pattern formed by refraction or reflection in atmospheric ice crystals. It is distinct from a dark-matter halo.
Snell's law is , with angles measured from the interface normal. The Huygens-Fresnel principle explains it by constructing the transmitted wavefront from secondary wavelets: during the same time interval, distances travelled in the two media are proportional to and . The geometry of the advancing plane wavefront then gives .
For incidence from index into vacuum, the transmitted angle is . The ray bends away from the normal, so its positive deviation is
For ,
Thus the graph rises monotonically from zero to a finite endpoint with a vertical tangent:
At the endpoint the transmitted ray grazes the interface. Beyond the critical angle for total internal reflection, no propagating transmitted ray exists and total internal reflection occurs.
Inside a prism, the two ray angles with the face normals sum to its apex angle. For the equilateral cross-section, they are and . The entry deviation equals the corresponding exit deviation under ray reversal. Adding the two changes of direction therefore gives
This is symmetric about . Symmetry alone gives a stationary point; to establish that it is a minimum, differentiate once more:
within the transmitted-ray interval. The sum is therefore strictly convex, and
These expressions require for a non-grazing path through both faces; is a grazing limit, and admits no such two-face transmitted path. More explicitly, both internal angles must be at most , which is possible only if .
Figure 1.
Single-interface deviation and the symmetric minimum of an equilateral prism, illustrated for index 1.5
. Details.
Atmospheric hexagonal ice crystals can present pairs of faces with a angle, acting as small prisms. Their orientations turn the minimum-deviation cone around the Moon into an optical halo. No transmitted ray of this family is deflected less than the minimum deviation of a prism. Moreover, near the minimum, is quadratic in the departure from the symmetric ray, so a range of incident directions is compressed into a small outgoing angular range. This caustic makes the inner rim sharp and bright, with the ray density decreasing farther outside. The common 22-degree halo has an angular radius near about either the Sun or Moon, hence a diameter near .[ref]