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Transcript
Optics
Spring 2016
ELEC E-5730
lectures: Toni Laurila, [email protected],
office I431, Tel. 050-458 2460
excercises: Aigar Vaigu [email protected], office I427
Course web site on Aalto MyCourses
• Exercise I question sheet and course schedule available
• Course book chapters 1 and 2 available for downloading
• course includes 6 compulsory laboratory works which will accomplished
during two laboratory exercise sessions
Last lecture – the Fundamentals
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•
Light as electromagnetic radiation
Light can treated both as photons and waves
Huygens’ principle
Fermat’s principle (”principle of least time”)
1) In homogenous medium light travels in a linear fashion
2) Law of reflection: 1 = 2
3) Law of refraction or Snell’s law: n1 sin( 1) = n2 sin( 2)
•
Total internal reflection
Today – Powerful set of tools for optical design
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Derivation of the lens maker’s formula and thin lens equation
Basics of ray tracing in optical systems
Different types of lenses, magnification, numerical aperture, f-number
Non-ideal lenses - aberrations
Matrix formalism for ray tracing
Why imaging optics is needed?
optical
elements
Optics is required ”to collect” light scattered from the object to
form a sharp, focused image
Refractive power of a spherical surface
optical path length
According to the Fermat’s principle the variation of the path equals zero, that is,
dL/d = 0.
Refractive power of a spherical surface
law of cosines applied to triangles SAC and ACP
SAC:
ACP:
dL/d = 0
Here we do so called ’paraxial approximation’:
Refractive power of a spherical surface
All rays will refract through point P at si which is independent on the angle .
Derivation of the lens maker’s formula and
thin lens equation
Lens maker’s formula
1
f
1
n 1
R1
1
R2
Thin lens equation
1
s
1
s'
1
f
(s=so and s’=si)
Assumptions used during the derivation:
and cos
1. paraksial approximation (sin
2. lens is thin
1; 1st terms in the series expansions)
Basics of lenses – positive lens
Refraction of a ray is proportional to the
distance from the optical axis.
Basics of lenses – negative lens
Refraction of a ray is proportional to the
distance from the optical axis.
Sign rules for lenses
Ri is > 0 if the centre point of curvature is
to the right of the surface
Also the terms ”positive” ja ”negative”
lens are used.
Principal rays of a lens (3 rays)
1. Ray propagates through the centre of the lens
without changing its direction.
2. Collimated ray travels through the focal point
behind the lens (virtual focal point in
front of a negative lens)
3. Ray going through the front focal point will be
collimated after the lens (back virtual focal for a
negative lens).
Magnification M of a lens
M
yi/yo
From equivivalent triangles S1S2O ja P1P2O it follows:
M = yi/yo = si/so
Magnification M
M = yi/yo = si/so
1
so
1
si
1
f
When the magnification is equal to 1?
Or where the object should be placed
to get an image having the original size?
f-number and numerical aperture N.A.
f-number (also known as f/#) = f/D
For example, f-number = 2 is the same as f/2
numerical aperture characterises the
light gathering power of a lens
N.A. = n sin
D
n D/(2f) = n / (2 x f/#)
f
Ideal lens
Validity of the paraxial approximation
Further away from the optical axis the paraxial approximation
is not good enough anymore.
Aberrations or imperfections of lenses
Ignoring the third and higher order terms in the series expansion of the sine and
cosine functions causes aberrations. Typical aberrations for a monochromatic
system are:
• spherical aberration
• astigmatism
• coma
• field curvature
• distortion.
For light containing several colours there are additional aberrations:
• chromatic aberration
• lateral colour
Spherical aberration
Ideal lens shape for imaging is not a spherical surface. However, a spherical
surface is the easiest and most affordable to manufacture. In a bi-convex
lens, for example, the rays of light propagating far away from the optical
distance will refract closer to the lens than paraxial rays.
With modern manufacturing systems aspherical lenses can already be
manufactured at a reasonable cost by pressing lenses out of melt glass or
plastic using a mold. Aspheric surface can compensate for the spherical
aberration.
Astigmatism
Means lens imperfecton where a non-paraxial ray has different focal points
in the horizontal and vertical directions.
Field distortion
Lens can distort the image in many ways even though the image is sharp or
the focusing properties are good.
Field curvature
Non-paraksial rays do not focus on a place surface.
Chromatic aberration
Is caused by the fact that the refractive index n is actually not a constant but
depends on the wavelength/frequency of light = material dispersion.
n = n( ) = n( )
Chromatic aberration in a bi-convex lens
Compensation of chromatic aberration
achromatic doublet lens
Lateral colour
Matrix formalism for ray tracing
Matrix formalism for ray tracing
T1
R1
1 d1
0
1
1
1
r1
T2
0
1
nL
T3
1 d2
0
1 d3
0 1
1
R2
1
1
r2
0
nL
1
Typical transformation matrices
Principal planes of an optical system
Principal planes of an optical system
Principal planes of an optical system
Principal planes of an optical system
Principal planes of an optical system
Summary
We have discussed the fundamental concepts of geometrical optics:
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lens maker’s formula for a thin lens
thin lens equation
ray tracing:
• principal rays of lenses
• sign convention
concepts: magnification, numerical aperture, f-number
lens aberrations
matrix formalism for optical systems
reduction of an optical system into a thin lens: principal planes