SUMMARY
Spherical lenses and mirrors exhibit spherical aberration due to the varying convergence points of marginal and axial rays of light. This phenomenon arises from the geometric shape of the lens or mirror, where rays incident at the edges focus closer than those near the center. For spherical mirrors, rays from infinity intersect the axis at a distance of l = (r/2)cos(θ), where r is the radius and θ is the angle of incidence. When θ is small, cos(θ) approximates to 1, leading to a focus at r/2, which contributes to spherical aberration when the approximation fails.
PREREQUISITES
- Understanding of ray optics and light propagation
- Familiarity with spherical geometry and its properties
- Knowledge of lens and mirror equations
- Basic trigonometry, particularly cosine functions
NEXT STEPS
- Study the effects of lens shape on optical performance
- Explore methods to correct spherical aberration in optical systems
- Learn about parabolic mirrors and their advantages over spherical mirrors
- Investigate the role of ray tracing software in analyzing optical aberrations
USEFUL FOR
Optical engineers, physicists, and students studying optics who are interested in understanding and mitigating spherical aberration in lenses and mirrors.