so much to remember, so little space

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So much to remember, so little space Diffraction Limits on Light

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So much to remember, so little space. Diffraction Limits on Light. What have we learned?. Any traveling sinusoidal wave may be described by y = y m sin( kx  w t + f ) Light always reflects with an angle of reflection equal to the angle of incidence (angles are measured to the normal). - PowerPoint PPT Presentation

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Page 1: So much to remember, so little space

So much to remember, so little space

Diffraction Limits on Light

Page 2: So much to remember, so little space

What have we learned?• Any traveling sinusoidal wave may be described by

y = ym sin(kx t + )

• Light always reflects with an angle of reflection equal to the angle of incidence (angles are measured to the normal).

• When light travels into a denser medium from a rarer medium, it slows down and bends toward the normal.

• The Fourier spectrum of a wider pulse will be narrower than that of a narrow pulse, so it has a smaller bandwidth.

• Your bandwidth B must be as large as the rate N at which you transfer different amplitudes.

• The rise time of each pulse must be no more than 70% of the duration of the pulse

Page 3: So much to remember, so little space

What Else Have We Learned?

• Can represent binary data with pulses in a variety of ways

• 10110 could look like . . .

Non-return-to-zero (NRZ)

Return-to-zero (RZ)

Bipolar Coding

Notice that the NRZ takes half the time of the others for the same pulse widths

Other schemes use tricks to reduce errors and BW requirements.

Page 4: So much to remember, so little space

Optical Waveguides Summary• Dispersion means spreading

• Signals in a fiber will have several sources of dispersion:– Chromatic:

• Material: index of refraction depends on wavelength (prism)

• Waveguide: some of wave travels through cladding with different index of refraction (primarily single-mode) – leads to wavelength-dependent effects

– Modal: different modes travel different paths and so require different amounts of time to travel down fiber (CUPS)

• Also have attenuation/loss due to scattering/absorption by fiber material, which depends on wavelength/frequency

Page 5: So much to remember, so little space

Optical Waveguide Summary (cont.)

• Modes in a fiber are specific field distributions that are independent of “z”, or length traveled down the fiber

• Fields of modes look like harmonics of standing waves

• Can make a single-mode fiber by:– reducing diameter of fiber so smaller cone of

light enters– reducing NA of fiber so smaller cone of light is

trapped

Page 6: So much to remember, so little space

What sets the limit on density of data stored?

For a specific example, what determines the density of data on a CD ROM?

Page 7: So much to remember, so little space

Interference of Waves

If crests match crests, then waves interfere constructively

Crests will match if waves are one wavelength, two wavelengths, … apart: path difference = m

Amax

2Amax

wave 1

wave 2

sum

Amax

Page 8: So much to remember, so little space

Destructive Interference

If crests match troughs (180° out of phase), then waves interfere destructively

Crests will match troughs if waves are one/half wavelength, three/half wavelengths, … apart: path difference = (m+½)

wave 1

wave 2

sum

Amax

Amax

Page 9: So much to remember, so little space

What This Means for Light

Light is electromagnetic radiation A light wave is oscillating electric and magnetic

fields The amplitude of the oscillation represents the

maximum electric (or magnetic) field and determines the intensity of light

Intensity depends on the square of the maximum electric field: I = Emax

2/(2c0) Constructive interference produces brighter light;

destructive interference produces dimmer light.

Page 10: So much to remember, so little space

Comparing Interference

Emax

2Emax

Medium amplitude of electric field yields medium intensity light

Double amplitude of electric field yields quadruple intensity (very bright) light

Zero amplitude of electric field yields zero intensity (no) light

Page 11: So much to remember, so little space

Coherent vs. Incoherent Light

• “Everyday light” is incoherent

• Laser light is an example of coherent light

• Simple wave equation describes coherent waves

y = ym sin(kx t + )

Page 12: So much to remember, so little space

Wavelet Approach to Interference and Diffraction

= wavelength

Direction of wave motion

Wave Crest

Wave Trough

Plane waves can be modeled as the interference of an array of point sources.

Page 13: So much to remember, so little space

Wavelet Approach to Interference and Diffraction

Any opening will cause plane wave to start spreading out.

= wavelength

a = aperture width

a

Direction of wave motion

Wave Crest

Wave Trough

Page 14: So much to remember, so little space

The Double Slit Experiment Waves spreading out from two points, such as

waves passing through two slits, will interfere

d

Wave crestWave troughSpot of constructive interference

Spot of destructive interference

Page 15: So much to remember, so little space

Diffraction Patterns Light traveling through a single slit also creates a

pattern, due to interference between wavefronts passing through different regions of the slit

a

Wave crestWave troughSpot of constructive interference

Spot of destructive interference

Page 16: So much to remember, so little space

Single Slit Math

Path length difference = a/2 sin

a y

D

ba/2

tan = y/D

b

Page 17: So much to remember, so little space

Diffraction Math

The locations of successive minima are given by

tan = y/D

for small angles, sin ~ ~ tan = y/D

.....)3 ,2 ,1(sin

,...)2 ,1 ,0( 2

1sin

2

nna

mma

Page 18: So much to remember, so little space

Diffraction by a circular aperture A circular aperture of diameter d

Single slit of width a

minimum)(1st 22.1sind

minimum)(1st sina

Page 19: So much to remember, so little space

Resolvability

Two objects are just resolved when the central diffraction maximum of one object is at the first minimum of the other. (Rayleigh’s criterion)

As before, approximately y/L

ddR

22.122.1

sin 1

Page 20: So much to remember, so little space

Comments on Resolvability

If want to resolve objects closer to each other (smaller y), need smaller wavelength of light or larger aperature

This is called the diffraction limit

dD

yR

22.1

Page 21: So much to remember, so little space

Why Do We Care?

• CD-ROMS and other optical storage devices

Page 22: So much to remember, so little space

Do the Activity, Continuing through it

After finishing Diffraction Pattern of a Red Laser, first two or three groups should jump to Green Laser part, then

give green lasers to other groups when done

Page 23: So much to remember, so little space

Before the next class, . . .

• Do Homework 8

• Read the handout about how CD ROMs work.

• Do Activity 07 Evaluation by Midnight Tonight

• Come with questions about the test material– Exam on Thursday, Feb. 14.