# Archives

# Abbe-Method

Measuring method (named after Ernst Abbe) used to determine the focal length and the position of the principal planes of a lens singlet or a lens system (=objective) on the optical axis.

How to determine the **focal length**:

The position of the lens is fixed and the camera (or the screen ) is moved depending on the object position, that you get a foczussed image (in the image center). Different object positions result in different camera- or screen distances

How to determine the **focal length of an objective** (= (= lens system)):

The Position of a lens (and the lens singlets in it) are fixed and an *arbitrary* Point O on the optical axis is marked as reference point, for example the center of the lens or the center of the first lens element).

Now we measure the distance x from the reference point to the object, the distance x’ to the image and the image size B.

You get a list of Magnifications

,

and equations from refererence Point to object

and reference point to image:

Where h und h’ are the distances from object side resp. image side principal planw to the reference point.

# Abbe-number

(also known as v-number)

a measure of the materials dispersion (=variation of refractive index with wavelength),

with high values of V indicating low dispersion (low chromatic aberration).

The value Vd is given by

which defines the Abbe number with respect to the yellow Fraunhofer-Line d (or D3) helium line at 587.5618 nm wavelength.

It can also be defined using the green mercury E-line at 546.073 nm:

where F’ and C’ are the blue and red cadmium lines at 480.0 nm and 643.8 nm, respectively.

# Abbe’s Invariant

In paraxial optics each single refracting surface satisfies the Abbe’s Invariant Q in the paraxial Area, that relates the front focal distance s of an axial object point with the back focal distance s’ of it’s conjugated point behind the surface

# ABCD Matrix

ABCD Matrixes

are used in **paraxial ** optical design.

The angles are measured

**in radians**!

A beam is described by a distance r from the optical axis and a offset angle from the optical axis

An ABCD Matrix that describes the optical element is formed

The ABCD Matrix is multiplied by the input vector

The result is an output vector that describes the output beam with a new distance from the optical axis and a new angle off the optical axis

is a short for for the equation system

with

with

**Examples of ABCD matrices for simple optical elements :****Propagation in free space or in a medium of constant refractive index :**

Where d = reduced distance= thickness / refraction index

**Propagation through a series i=1..k of planparallel media with constant refraction indices :**

Where d_i = reduced distance_i= thickness_i / refraction index_i

**Refraction at a flat surface:**

Where:

= initial refractive index

= final refractive index

**Refraction at a curved surface:**

Where:

R = radius of curvature, for a convex surface (centre of curvature after interface)

= initial refractive index

= final refractive index

**Reflection vrom a flat mirror:**

Identity matrix

**Reflection from a curved mirror:**

Where:

effective radius of curvature in tangential plane (horizontal direction)

effective radius of curvature in the sagittal plane (vertical direction)

With for convex mirrors (centre of curvature after interface)

**Refraction at a thin lens **

Where:

f = focal length of the lens, where for convex/positive/converging lenses. Valid if if and only if the focal length is much bigger than the thickness of the lens

**Refraction at a thick lens **

Where:

= refractive index outside of the lens.

= refractive index of the lens itself (inside the lens).

= Radius of curvature of First surface.

= Radius of curvature of Second surface.

t = center thickness of lens.

# Airy-Disk

see: circle of confusion

# angular

# Aperture angle

Angle that the lens can see in the direction of a given sensor measure.

Actual aperture angles are influenced by the length of used extension rings,and even focus distances (because they are mostly achieved by simulating extension rings) max possible aperture angles aren’t

Changing the sensor size changes the actual aperture angle, max possible aperture angles aren’t

# aperture value

Number which characterizes the luminous sensitivity of a lens. Another term for aperture value is F-number.

The smaller the number, the more light a lens can collect, the brighter the image, the smaller the depth of field.

The larger the number, the darker the image, but in generally the greater depth of field. At the same time, we generally lose resolution, see Rayleigh Criterion.

The f-number is the ratio of the focal length divided by the apparent size of the aperture (= entry pupil diameter).

The inverse of the square of the f-number is a measure for the image brightness of a lens.

# back focal length

= BFL)

distance on the optical axis between last active optical surface and the sensor when the object is at infinity.

The value is only valid in paraxial optics, ie for objects close to the optical axis.

Further off the optical axis, the focal distance of distant objects is affected by the spherical aberration.

(back focal distance = Back Focal Length = BFL)

Note:

Not to be confused with the effective focal length EFL!