lenses and imaging (part i)

48
Lenses and Imaging (Part I) Why is imaging necessary: Huygen’s prin ciple – Spherical & parallel ray bundles, po ints at infinity Refraction at spherical surfaces (parax ial approximation) Optical power and imaging condition Matrix formulation of geometrical optic s The thin lens Surfaces of positive/negative power Real and virtual images MIT 2.71/2.710 09/15/04 wk2- b-1

Upload: evette

Post on 22-Jan-2016

40 views

Category:

Documents


0 download

DESCRIPTION

Lenses and Imaging (Part I). • Why is imaging necessary: Huygen’s principle – Spherical & parallel ray bundles, points at infinity • Refraction at spherical surfaces (paraxial approximation) • Optical power and imaging condition • Matrix formulation of geometrical optics - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: Lenses and Imaging (Part I)

Lenses and Imaging (Part I)

• Why is imaging necessary: Huygen’s principle – Spherical & parallel ray bundles, points at infinity• Refraction at spherical surfaces (paraxial approximation)• Optical power and imaging condition• Matrix formulation of geometrical optics• The thin lens• Surfaces of positive/negative power• Real and virtual images

MIT 2.71/2.71009/15/04 wk2-b-1

Page 2: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-2

Parabloid mirror: perfect focusing(e.g. satellite dish)

f: focal length

Page 3: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-3

Lens: main instrument for imageformation

air

opticalaxis

airglass

Point source(object)

Point image

The curved surface makes the rays bend proportionally to their distancefrom the “optical axis”, according to Snell’s law. Therefore, the divergent

wavefront becomes convergent at the right-hand (output) side.

Page 4: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-4

Why are focusing instrumentsnecessary?

• Ray bundles: spherical waves and plane waves• Point sources and point images• Huygens principle and why we can see around us• The role of classical imaging systems

Page 5: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-5

Ray bundles

pointsource

sphericalwave

(diverging)wave-front

⊥ rays

wave-front ⊥ rays

pointsource

very-veryfar away plane

wave

Page 6: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-6

Huygens principle

Each point on the wavefrontacts as a secondary light sourceemitting a spherical wave

The wavefront after a shortpropagation distance is theresult of superimposing allthese spherical wavelets

opticalwavefronts

Page 7: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-7

Why are focusing instrumentsnecessary?

incident light

...is scattered by

the object

object

Page 8: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-8

Why are focusing instrumentsnecessary?

incident light

...is scattered by

the object

objectimage

⇒need optics to “undo”the effects of scattering,i.e. focus the light

Page 9: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-9

Ideal lens

air

opticalaxis

airglass

Point source(object)

Point image

Each point source from the object plane focuses onto a pointimage at the image plane; NOTE the image inversion

Page 10: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-10

Summary:Why are imaging systems

needed?• Each point in an object scatters the incident illumination into a spherical wave, according to the Huygens principle.• A few microns away from the object surface, the rays emanating from all object points become entangled, delocalizing object details.• To relocalize object details, a method must be found to reassign (“focus”) all the rays that emanated from a single point object into another point in space (the “image.”)• The latter function is the topic of the discipline of Optical Imaging.

Page 11: Lenses and Imaging (Part I)

The ideal optical imaging system

opticalelements

object image

MIT 2.71/2.71009/15/04 wk2-b-11

Ideal imaging system:each point in the object is mapped

onto a single point in the image

Real imaging systems introduce blur ...

Page 12: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-12

Focus, defocus and blur

Perfect focus Defocus

Page 13: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-13

Focus, defocus and blur

Perfect focus Imperfect focus

“sphericalaberration”

Page 14: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-14

Why optical systems do not focusperfectly

• Diffraction• Aberrations

• However, in the paraxial approximation to Geometrical Optics that we are about to embark upon, optical systems do focus perfectly

• To deal with aberrations, we need non-paraxial Geometrical Optics (higher order approximations)• To deal with diffraction, we need Wave Optics

Page 15: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-15

Ideal lens

air

opticalaxis

airglass

Point source(object)

Point image

Each point source from the object plane focuses onto a pointimage at the image plane

Page 16: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-16

Refraction at single spherical surface

for each ray, must calculate• point of intersection with sphere• angle between ray and normal tosurface• apply Snell’s law to find direction ofpropagation of refracted ray

R: radius ofsphericalsurface

center ofsphericalsurface

medium 1index n,

e.g. air n=1

Page 17: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-17

Paraxial approximation /1

• In paraxial optics, we make heavy use of the following approximate (1st order Taylor) expressions:

where ε is the angle between a ray and the optical axis, and is a smallnumber (ε «1 rad). The range of validity of this approximationtypically extends up to ~10-30 degrees, depending on the desireddegree of accuracy. This regime is also known as “Gaussian optics” or“paraxial optics.”

Note the assumption of existence of an optical axis (i.e., perfectalignment!)

Page 18: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-18

Paraxial approximation /2

Ignore the distancebetween the location

of the axial rayintersection and theactual off-axis ray

intersection

Apply Snell’s law as ifray bending occurred at

the intersection of theaxial ray with the lens Valid for small curvatures

& thin optical elements

axial ray

off-axis r

ay

Page 19: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-19

Refraction at spherical surface

Refraction at positive spherical surface:

Power x: ray heightα: ray direction

R: radiusof curvature

optical axis

off-axis r

ay

Page 20: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-20

Propagation in uniform space

Propagation through distance D:

x: ray heightα: ray direction

optical axis

off-axis ray

Page 21: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-21

Paraxial ray-tracing

air airglass

Free-spacepropagation

Refraction atair-glassinterface

Free-spacepropagation

Free-spacepropagation

Refraction atglass-airinterface

Page 22: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-22

Example: one spherical surface,translation + refraction + translation

Non-paraxial ray(approximation

gives large error) medium 1index n,

e.g. air n=1

center ofsphericalsurface

Paraxial rays(approximation

valid)

R: radius ofsphericalsurface

Page 23: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-23

Translation + refraction + translation /1

Starting ray: location x0 directionα0

Translation through distance D01 (+ direction):

Refraction at positive spherical surface:

Page 24: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-24

Translation + refraction + translation /2

Translation through distance D12 (+ direction):

Put together:

Page 25: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-25

Translation + refraction + translation /3

Page 26: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-26

Sign conventions for refraction

• Light travels from left to right• A radius of curvature is positive if the surface is convex towards the left• Longitudinal distances are positive if pointing to the right• Lateral distances are positive if pointing up• Ray angles are positive if the ray direction is obtained by rotating the +z axis counterclockwise through an acute angle

optical axis +z

Page 27: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-27

On-axis image formation

Pointobject

Pointimage

Page 28: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-28

On-axis image formation

All rays emanating at arrive at x2

irrespective of departure angleα0

Page 29: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-29

On-axis image formation

All rays emanating at arrive at x2

irrespective of departure angleα0

“Power” of the sphericalsurface [units: diopters, 1D=1 m - 1 ]

Page 30: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-30

Off-axis image formation

Pointobject

(off-axis)

Pointimage

opticalaxis

Page 31: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-31

Magnification: lateral (off-axis), angle

Lateral

Angle

Page 32: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-32

Object-image transformation

Ray-tracing transformation(paraxial) between

object and image points

Page 33: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-33

Image of point object at infinity

Pointimage

Page 34: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-34

Image of point object at infinity

objectat ∞

image

: image focal length

Note:

ambient refractive indexat space of point image

1/Power

Page 35: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-35

Point object imaged at infinity

Pointobject

Page 36: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-36

Point object imaged at infinity

object

Imageat ∞

: object focal length

Note:

ambient refractive indexat space of point image

1/Power

Page 37: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-37

Image / object focal lengths

Pointobject

Imageat ∞

objectat ∞

Pointimage

Power Power

Page 38: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-38

Matrix formulation /1

translation byDistance D 01

refraction bysurface with radius

of curvature R

ray-tracingobject-image

transformationform common to all

Page 39: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-39

Matrix formulation /2

Refraction by spherical surface Power

Translation through uniform medium

Page 40: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-40

Translation + refraction + translation

translation by D12

Refraction by r.curv. R

translation by D01

result…

Page 41: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-41

Thin lens in air

Objective: specify input-output relationship

Page 42: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-42

Thin lens in air

Model: refraction from first (positive) surface+ refraction from second (negative) surface

Ignore space in-between (thin lens approx.)

Page 43: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-43

Thin lens in air

Page 44: Lenses and Imaging (Part I)

Thin lens in air

MIT 2.71/2.71009/15/04 wk2-b-44

Page 45: Lenses and Imaging (Part I)

Thin lens in air

Power of thefirst surface

Power of thesecond surface

MIT 2.71/2.71009/15/04 wk2-b-45

Page 46: Lenses and Imaging (Part I)

Thin lens in air

MIT 2.71/2.71009/15/04 wk2-b-46

Lens-maker’sformula

thin lens

thin lens

Page 47: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-47

Thin lens in air

thin lens

thin lens Ray bending is proportionalto the distance from the axis

Page 48: Lenses and Imaging (Part I)

MIT 2.71/2.71009/15/04 wk2-b-48

The power of surfaces

• Positive power bends rays “inwards”

Simple sphericalrefractor (positive)

Plano-convexlens

Bi-convexlens

• Negative power bends rays “outwards”

Simple sphericalrefractor (negative)

Plano-convexlens

Bi-convexlens