This phenomenon commonly affects lenses and curved mirrors, as these components are often shaped in a spherical manner for ease of manufacturing.
The effect of spherical aberration was first identified in the 11th century by Ibn al-Haytham who discussed it in his work Kitāb al-Manāẓir.
Lens systems with aberration correction are usually designed by numerical ray tracing.
Because of spherical aberration, telescopes with focal ratio less than f/10 are usually made with non-spherical mirrors or with correcting lenses.
[2] In 2018, Rafael G. González-Acuña and Héctor A. Chaparro-Romo, graduate students at the National Autonomous University of Mexico and the Monterrey Institute of Technology and Higher Education in Mexico, found a closed formula for a lens surface that eliminates spherical aberration.
Many ways to estimate the diameter of the focused spot due to spherical aberration are based on ray optics.
Therefore, the results can be wrong due to interference effects arisen from the wave nature of light.
A rather simple formalism based on ray optics, which holds for thin lenses only, is the Coddington notation.