Optics, electromagnetic theory Geometrical optics Theorem
Abbe sine condition
Builds on Refractive indexOptical aberration
Statement
Let a rotationally symmetric optical system image an axial object point onto an axial image point without spherical aberration. Let and be the refractive indices of the object and image media. Let a ray from make the angle with the axis. Let be the angle of the same ray with the axis at . Let be the paraxial lateral magnification. Consider a small object element in the plane through perpendicular to the axis. It is imaged sharply, to first order in its height, if and only if all rays from through the aperture satisfy
Remarks
The condition says that the ratio is the same for all rays, not only for paraxial ones. One proof compares the optical path lengths from a point near in the object plane to its ideal image, along different rays. To first order in the object height , the path length changes by , and sharp imaging requires this change to be the same for all rays, hence zero.
A system with no spherical aberration that satisfies the sine condition is called aplanatic; it is free of coma near the axis.
Example: a microscope objective of numerical aperture and magnification in air on the image side needs at the edge of the aperture.
Without the sine condition the image of an off-axis point is blurred into a comet-shaped spot, the aberration called coma.
Going deeper
For a student
The sine condition is a design criterion for aplanatic objectives and for wide-aperture systems. It is the large-angle replacement for the paraxial relation , which follows from the Lagrange invariant. For the axial direction, the analogous condition for sharp imaging along the axis is Herschel's condition, and in general the two cannot both hold.
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About this page
| Tag | 4WDZCHTAEZ |
|---|---|
| URI | m2://4WDZCHTAEZ |
| Kind | statement, theorem |
| Writing | W0 stub |
| MSC | 78A05 |
| Status | This copy of the site has no build data. Run m2 status 4WDZCHTAEZ. |
| About | Optical aberration |
| Uses | Refractive index, Optical aberration |
| Same as | |
| Changed | 3 November 2026 |
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