Optics And Photonics Codexery

Optical aberration

Deviation from ideal image formation in optical systems.

Optical aberration

Optical aberration is a property of optical systems, such as lenses and mirrors, that causes the image created by the system to not be a faithful reproduction of the object being observed. Aberrations cause the image formed by a lens to be blurred, distorted in shape, or have color fringing or other effects not seen in the object, with the nature of the distortion depending on the type of aberration. Aberration can be defined as a departure of the performance of an optical system from the predictions of paraxial optics.

field
Optics
known_for
Departure of optical system performance from paraxial optics predictions, causing image blur, distortion, or color fringing
types
Monochromatic and chromatic aberrations
common_monochromatic_aberrations
Defocus, spherical aberration, coma, astigmatism, field curvature, image distortion
chromatic_aberration_types
Axial (longitudinal) and lateral (transverse) chromatic aberration

Lore & Background

In optics, aberration occurs when light from one point of an object does not converge into (or does not diverge from) a single point after transmission through the system. Aberrations occur because the simple paraxial theory is not a completely accurate model of the effect of an optical system on light, rather than due to flaws in the optical elements. An image-forming optical system with aberration will produce an image which is not sharp, and makers of optical instruments need to correct optical systems to compensate for aberration.

Reader's Guide

Optical aberration is a fundamental concept in optics, describing the failure of lenses and mirrors to produce perfect images. It is divided into two classes: monochromatic aberrations, caused by the geometry of the lens or mirror and occurring even with monochromatic light, and chromatic aberrations, caused by dispersion (the variation of a lens's refractive index with wavelength). The most common monochromatic aberrations include defocus, spherical aberration, coma, astigmatism, field curvature, and image distortion. Chromatic aberrations are axial (longitudinal) and lateral (transverse). The Gaussian theory of optics provides a convenient approximation but is only true for infinitely small angles; realistic systems always exhibit aberrations. The sine condition, as noted by Abbe, is required to avoid certain aberrations for points off the axis, and a system fulfilling this condition and free from spherical aberration is called aplanatic. Aberration increases with lens diameter and aperture, and can be minimized by reducing the aperture, though this also reduces light gathering.

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