Ramsden's Eyepiece And its Applications

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This ppt covers all topics of Ramsden's Eyepiece -construction,working,calculations,applications


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RAMSDEN EYEPIECE AND ITS
APPLICATION

CONTENT
What is an eyepiece
Ramsden eyepiece
Spherical aberration
Cromatic aberration
Construction of ramsden eyepiece
Working of ramsden eyepiece
Condition for spherical and cromatic aberration
Mean Focal length
Positive eyepiece
Position of Cross-wire
Cardinal points of Ramsden eyepiece
Merits and Demerits
Difference between huygen's and ramsden's eyepiece
Application of Ramsden's eyepiece
References

EYEPIECE
Why we need eyepiece ?
The image obtained from
microscopes and telescopes
are not free from optical
defects like cromatic
aberration and spherical
aberration .
We required an instrument
which produce minimum
aberrated image of an object
,and eyepiece is the best for it.
The eyepiece is a magnifier , which is formed by the co-axial system of lenses and are used to
see the minimum abberrated image formed by the objective of optical instrument .

HUYGEN EYEPIECE
Ramsden eyepiece
There are two major types of eyepieces that
are grouped according to lens and
diaphragm arrangement:

JESSE
RAMSDEN
Ramsden was acknowledged to be the most
skillful and capable instrument maker of the
eighteenth century he developed dividing engine
which is the greatest contribution to the
technology of the era By 1789 he had also
produced theodolites, micrometers, balances,
barometers, and the many philosophical
instruments required by the physicists of that
period.
1735 -1800

RAMSDEN
EYEPIECE
A Ramsden eyepiece is the simplest
example of an eyepiece for a high
quality optical instrument,
containing two identical plano-
convex lenses. The Ramsden
eyepiece is one of several
eyepiece options when a single
simple magnifying lens is
inadequate due to aberrations. It
is particularly common in
instruments which have a scale or
micrometer wires. It is quite
effective in reducing spherical
aberration , distortion and removes
the problem of coma.

SPHERICAL
ABERRATION
Spherical Aberration is an optical problem that occurs when all incoming light
rays end up focusing at different points after passing through a spherical
surface

Chromatic aberration is the phenoma in which the lens fails to focus all colours
at the same point which result in multicoloured image of a white object.
CHROMATIC
ABERRATION

Ramsden's eyepiece consists of two plano-
convex lenses each of focal length f
separated by a distance equal to (2/3).
The field lens is a little larger than the
intermediate image and is placed close to
this image to allow as much light as
possible to pass through it. The eye lens has
a smaller diameter but carries out the
actual magnification.The objective forms
the real inverted image I1 of a distant
object of eye lens. This serves as an object
for the field lens, which gives rise to a
virtual image I2. in turn serves as an object
for the eye lens. which gives the final image
at infinity, because is made to lie at its
Principal focus.
CONSTRUCTION
OF RAMSDEN
EYEPIECE

Image of eye lens is at
Infinity it means object is at focus

WORKING

SPHERICAL
ABERRATION
CONDITION:
d= f1-f2
In Ramsden eyepiece
f1=f
f2=f
therefore d=f-f =0
So ,spherical abrerration
is present in ramsden eyepiece

CONDITION:
therefore,
CHROMATIC
ABERRATION
f1=f2=f

So, chromatic aberration is
present in ramsden eyepiece

CHECK ONLINE SHOP
EQUIVALENT
FOCAL
LENGTH (F)

POSITIVE
EYEPIECE
In this eyepiece
magnification of the
real image of the
objective lens is done
so this eyepiece is
positive eyepiece.

If a cross wire is placed at the I1
position then its magnification is
done by both field lens and eye
lens and their final images obtain
at the same plane.
POSITION OF
CROSS WIRE

CARDINAL POINTS
OF RAMSDEN
EYEPIECE
FIRST PRINCIPLE
POINT(P1)

SECOND PRINCIPAL
POINT (P2)
CARDINAL POINTS
OF RAMSDEN
EYEPIECE

FIRST FOCUS
POINT (F1)

SECOND FOCUS
POINT (F2)

MERITS AND
DEMERITS
The field of view of the eyepiece is fairly wide.
It is not entirely free from chromatic aberration since the
distance between the two lenses is not equal to half the sum of
their focal lengths. However, chromatic aberration is
minimized by using an achromatic combination both for the
field lens and the eye lens.
Spherical aberration is minimized by using two plano-convex
lenses. Ramsden’s eyepiece is used practically in all
instruments where measurements of the size of the final
image are to be made. The eyepiece is sometimes referred to as
positive eyepiece because a real image is formed by the
objective in front of the field lens, which further acts as a real
object for the eye lens.

IT SATISFIES THE CONDITION FOR
ACHROMATISM.
IT IS ACHROMATIC FOR ONLY TWO
CHOSEN COLOURS.
IT IS ACHROMATIC FOR ALL COLOUR
THE OTHER TYPES OF ABERRATIONS
ARE BETTER ELIMINATED. COMA IS
ABSENT AND DISTORTION IS 5%
HIGHER.
THE OTHER TYPES OF ABERRATIONS
LIKE PINCUSHION DISTORTION ARE
NOT ELIMINATED
THE EYE CLEARANCE IS 5% HIGHER
THE EYE CLEARANCE IS TOO SMALL
AND LESS COMFORTABLE.
RAMSDEN HUYGENS
RAMSDEN EYEPIECE IS POSITIVE
EYEPIECE. THE IMAGE FORMED BY
THE OBJECTIVE LIES IN FRONT OF
FIELD LENS. THEREFORE, CROSS-WIRE
CAN BE USED.
HUYGENS EYEPIECE IS NEGATIVE
EYEPIECE. THE IMAGE FORMED BY
THE OBJECTIVE LIES IN BETWEEN THE
TWO LENSES. THEREFORE, CROSS-WIRE
CANNOT BE USED.
THE CONDITION FOR MINIMUM
SPHERICAL ABERRATION IS NOT
SATISFIED. BUT BY SPREADING THE
DEVIATIONS OVER FOUR SURFACES ,
SPHERICAL ABERRATION IS
MINIMIZED.
THE CONDITION FOR MINIMUM
SPHERICAL ABERRATION IS SATISFIED.
IT DOES NOT SATISFY THE CONDITION
FOR ACHROMATISM BUT CAN BE
MADE ACHROMATIC BY USING AN
ACHROMATIC DOUBLET AS THE EYE
LENS.

APPLICATIONS
It remains highly suitable for use with
instruments operating using near-
monochromatic light sources e.g.
polarimeters.
The Ramsden eyepiece is still in use today in
astronomical telescopes
Due to the presence of cross wires this
eyepiece is used for taking measurements in
physical science laboratories
Can be used as a simple magnifying glass
Ramsden eyepieces is used in a spectrometer

REFERENCES
V. A description of a new construction of eye-glasses for such telescopes as may be
applied to mathematical instruments (royalsocietypublishing.org)
Choosing and Using Astronomical Eyepieces by William Paolini (auth.)
Optics and optical instruments - B.K Johnson
Fundamentals and basic optical lnstruments ; Advanced optical instruments and
techniques by Malacara & Daniel & Thompson & Brian J
Eyepieces (gsu.edu)
Eyepieces - an overview | ScienceDirect Topics
Chromatic Aberration of Eyepieces in Early Telescopes (unl.edu)
Jesse Ramsden - Wikipedia
Eyepiece - Wikipedia

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