Lecture 5: Geometrical aberrations

Optical Image Formation

Perfect optical image:
All rays coming from one object point intersect in one image point

Real system with aberrations

transverse aberration in the image plane

longitudinal aberrations from the image plane

wave aberration in the exit pupil
perfect spherical wave surface as reference

Representation of Geometrical Aberrations

Longitudinal aberrations delta(s)

Transverse aberrations delta(y)

Angle aberrations delta(u)

Wave aberrations delta(W)
wavefront: function of pupil coordinate

Angle aberrations for a ray bundle: deviation from common direction of the collimated ray bundle
in mrad/°

Representation as a conventional spot diagram

Strong relation to spot diagram

Usually only linear sampling along the x-,y-axis
No information in the quadrant of the aperture

Typical low order polynomial contribution for

Defocus: linear

Coma: quadratic

Spherical: Cubic

Lateral color: offset

Spot diagram

All rays start in one point in the object plane
Entrance pupil is sampled equidistant
In exit pupil, the transferred grid may be distorted
In image plane a spreaded spot diagram is generated.
Symmetry on x comes from sampling on the y-axis.

Polynomial Expansion of the Aberrations
Aberrations occur for larger angle values

Taylor expansion of the deviation:
Transverse aberration: Image height; Pupil height; Pupil azimuth angle

Symmetry invariance

Type of aberration based on field y and aperture r.
Image location: defocus, tilt
Primary aberrations: Spherical, Coma, Astig./Curva., Distortion
Secondary aberrations.

Primary Aberrations

Three types of definition:
1.Only for chief ray
2.small neighborhood around chief ray
3.finite aperture
Coupling relation between Transverse aberration and wave aberration

Transverse Aberrations of Seidel

Surface Contributions

Expansion of the transverse aberration delta(y) on image height y and pupil height r

Abbreviations

Seidel aberrations expression

height ratio of marginal rays

height ratio of chief rays

Surface invariant of Abbe

Abbe invariant of the pupil imaging

Surface contributions of chromatical aberrations

Axial

transverse

total chromatical errors of a system

In height ratio and Abbe invariant

In n', n, R, s', p'

Lens contribution of Seidel

Spherical aberration

On axis, circular symmetry
Real marginal rays, shorter intersection length

Optimal image plane: circle of least rms value

lens bending
spherical aberration and focal spot diameter as a function of the lens bending

Optimal bending for incidence averaged incidence angles

Minimum larger than zero: usually no complete correction possible

Aplanatic surfaces: zero spherical aberration

ns = n's'

condition for aplanatic surface

Virtual image location

Applications:
Microscopic objective lens;
Interferometer objective lens

Aplanatic lenses: combination of one concentric and one aplanatic surface

zero contribution of the whole lens to spherical aberration

A-A: parallel offset
A-C: convergence enhanced
C-A: convergence reduced
C-C: no effect

Astigmatism

Reason:
Chief ray: oblique angle
different refractive power for tangential and sagittal section

Different focal line for tangential and sagittal
tangential rays meet closer
In between: circle of least confusion

Imaging with astigmatism

Tangential and sagittal image shell depending on the azimuth

Field curvature and image shell

Law of Petzval
No effect of bending on curvature, but distribution of lens powers and indices

Sharpe imaged zone changes from centre to margin of the image field

Astigmastism corrected:
remains a curved image shell
Bended field--> Petzval curvature(not an optimal surface with godd imaging resolution)

Coma

Tangential ray fan for coma: caustic
sagittal: groove-like surface

Coma aberration: for oblique bundles and finite aperture due to asymmetry

Relation of spot circles and pupil zones

Distortion

Purely geometrical deviations without any blur

Distortion correspond to spherical aberration of the chief ray
the location of the stop defines the chief ray path

Definition of local magnification changes
D = (y'_real - y'_ideal) / y'_ideal

D<0: barrel, front stop

D>0: pincushion, rear stop

Chromatical aberrations (1st order)

Axial chromatical aberration:
dispersion of marginal ray
different image locations

Transverse chromatical aberration
dispersion of chief ray
different image sizes

higher n -->shorter intersection length

definition of error: change in image location/intersection length

correction by glasses with different dispersion

equal intersection length for outer wavelength(blue, red), residual deviation for middle wavelength.

Secondary spectrum: Residual errors in image location

Apochromat

coincidence of the image location for at least 3 wavelengths

3 glasses necessary, only with anomal partial dispersion

Corresponds to a change of magnification with wavelength

Impression in real images

typical colored fringes/edges

color sequence depends on sigh of CHV ?

color rings isotropic around circle object
color rings uniform over FoV