Summary

1911 Encyclopædia Britannica, Volume 12… (1911)

Reflection from an excess of horizontal prisms gives rise to a vertical circle passing through the sun.
The parhelia (p) were explained by Mariotte as due to refraction through a pair of alternate faces of a vertical prism. When the sun is near the horizon the rays fall upon the principal section of the prisms; the minimum deviation for such rays is 22°, and consequently the parhelia are not only on the inner halo, but also on the parhelic circle. As the sun rises, the rays enter the prisms more and more obliquely, and the angle of minimum deviation increases
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