Lecture #2 Seeing the light 1/29/13. What happens to light when it interacts with matter? Reflects Absorbed Refracts Changes speed Polarized Diffracts.

Slides:



Advertisements
Similar presentations
Properties of Light.
Advertisements

Electromagnetic Spectrum
Wave Nature of Light  Refraction  Interference  Young’s double slit experiment  Diffraction  Single slit diffraction  Diffraction grating.
Wave Behavior Another McGourty-Rideout Production.
Waves 2 Sound and Light.
Interference and Diffraction
The Wave Nature of Light
Snell’s Law Snell’s Law describes refraction as light strikes the boundary between two media n1 sin q1 = n2 sin q2 The index of refraction of a pure vacuum.
Notes on Waves. Waves are ENERGY! Travel through medium (Electromagnetic waves can travel through vacuum.) Medium doesn’t move, only energy travels.
L 29 Light and Optics - 1 Measurements of the speed of light: c = 3 × 10 8 m/s = 186,000 miles/s light propagating through matter – transparent vs. opaque.
LIGHT A FORM OF ELECTROMAGNETIC RADIATION THAT STIMULATES THE EYE.
WAVES Optics.
Interference Physics 202 Professor Lee Carkner Lecture 22.
Interference Physics 202 Professor Lee Carkner Lecture 24.
Whiteboard Warmup! A glass lens of refractive index n = 1.6 has a focal length of 30 cm while in air. What would happen to the focal length of the lens.
Phy 212: General Physics II Chapter 35: Interference Lecture Notes.
Chapter 16 Light Waves and Color
REFRACTION. When light travels from one material to another it usually changes direction The bending of light that occurs at the borderline of two materials.
Properties of ElectroMagnetic Radiation (Light)
Waves PSC1341 Chapter 4. Waves A wave is a repeating disturbance or movement that transfers energy through matter or space Waves can be mechanical and.
Lecture 15 Interference Chp. 35 Topics –Interference from thin films –Due to the wave nature of light –Change in wavelength and phase change in a medium.
1 PowerPoint Lectures to accompany Physical Science, 6e Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Chapter.
Light and Optics. Unit 8: Light and Optics Chapter 23: The Physical Nature of Light 23.1 Electromagnetic Spectrum 23.2 Interference, Diffraction, and.
LIGHT.
Thus, the image formed by lens 2 is located 30 cm to the left of lens 2. It is virtual (since i 2 < 0). 30 The magnification is m = (-i 1 /p 1 ) x (-i.
L 31 Light and Optics [1] Measurements of the speed of light: 186,000 miles per second (1 foot per nanosecond) light propagating through matter – transparent.
Mr. Rockensies Regents Physics. When light is seen as a single color, it is considered monochromatic When light has more than one color, it is referred.
Light and Optics Chapter 22, 23. Light as an Electromagnetic wave  Light exhibits behaviors which are characteristic of both waves and particles Interference,
1. Waves and Particles 2. Interference of Waves
Chapter 13 The Characteristics of light. Objectives Identify the components of the electromagnetic spectrum. Calculate the frequency or wavelength of.
PHENOMENA OF LIGHT Chapters 27, 29, & 31. Easy to get mixed up… Polarization (Light)Ch 27 Reflection (Water & Light)Ch 29 Refraction (Light)Ch 29 Dispersion.
In the previous chapter we were treating light as rays. A powerful simple method. Now we are treating light as a wave. Chapter 37 & 38: The wave nature.
Phys 102 – Lecture 17 Introduction to ray optics.
Optics ISAT 241 Analytical Methods III Fall 2003 David J. Lawrence.
Electromagnetic Waves
Electro- magnetic Waves. Electromagnetic Waves Waves consisting of oscillating electric and magnetic fields that move at the speed of light through space.
Maxwell’s Equations Differential forms electromagnetic waves y x z E ⊥ B, and E ⊥ k, B ⊥ k, k is the direction of the wave. Polarization of electromagnetic.
ResourcesChapter menu Bellringer What do you think light is? Is light made of matter? Can light travel through space? Explain your answers in your lab.
OPTICS Chapter 35 Reflection and Refraction. Geometrical Optics Optics is the study of the behavior of light (not necessarily visible light). This behavior.
Refraction: TIR and Dispersion AP Physics: M. Blachly Light and Optics.
Lecture Outline Chapter 22 College Physics, 7 th Edition Wilson / Buffa / Lou © 2010 Pearson Education, Inc.
PowerPoint Lectures to accompany Physical Science, 7e Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Chapter.
Higher Physics – Unit Waves. a a λ λ crest trough Wave Theory All waves transmit energy. The energy of a wave depends on its amplitude. a = amplitude.
Interference and Diffraction
Properties of ElectroMagnetic Radiation (Light)
Light Waves Interacting with Matter
L 29 Light and Optics - 1 Measurements of the speed of light: 186,000 miles per second (1 foot per nanosecond) light propagating through matter – transparent.
Refraction The bending of light due to a change in speed.
Wave Properties of Light. Characterization of Light Light has both a wavelike and particle like nature. Light has both a wavelike and particle like nature.
Chapter  Light travels fast and over long distances  Light carries energy and information  Light travels in straight lines  Light bounces and.
AP Physics 2 Unit 7 Refraction and Physical Optics.
16.1 – Light Fundamentals Visible light is part of a very broad range of frequencies called The Electromagnetic Spectrum. Visible light ranges from 700.
L 31 Light and Optics [1] Measurements of the speed of light: 186,000 miles per second light propagating through matter – transparent vs. opaque.
Your Name: Last, First…………………………………………… Name of Workshop Instructor: Last, First……………………….. Exam #2 ……………………………………………………… Date: March 22 nd, 2012…………………………………………
Light, Mirrors, and Lenses. Light is a part of the electromagnetic spectrum.
Chapter 16 Fundamentals of Light Understand sources of light and how light illuminates the universe around us. Chapter 16 In this chapter you will:
7 Properties of light pg. 69.
Light and Optics  The Electromagnetic Spectrum  Interference, Diffraction, and Polarization Wave Properties of Light.
L 31 Light and Optics [1] Measurements of the speed of light: 186,000 miles per second (1 foot per nanosecond) light propagating through matter – transparent.
L 31 Light and Optics [1] Measurements of the speed of light The bending of light – refraction Dispersion Total internal reflection Dispersion Rainbows.
L 29 Light and Optics - 1 Measurements of the speed of light: c = 3 × 108 m/s = 186,000 miles/s light propagating through matter – transparent vs. opaque.
LIGHT!!!!.
Part 2: Behaviors of Light
Seeing the light 2/15/11 Adam Smith
Light.
1. Waves and Particles 2. Interference of Waves
Presentation transcript:

Lecture #2 Seeing the light 1/29/13

What happens to light when it interacts with matter? Reflects Absorbed Refracts Changes speed Polarized Diffracts

What happens to light when we see?

Today’s topics Learning styles Waves Refraction Diffraction / interference Light sources Intensity Homework on web site for next week

We can think about light in several ways Light as a wave: oscillating electromagnetic field

We can think about light in several ways Light as a wave: oscillating electromagnetic field Light as a ray: direction of wave

We can think about light in several ways Light as a wave: oscillating electromagnetic field Light as a ray: direction of wave Light as a photon: packet of energy which excites electrons

Light as a wave Wave characteristics Wavelength Frequency Speed Wavefront goes in one direction = ray Travels in straight line till it encounters different material

Wavelength – distance btn peaks λ varies across visible spectrum 400 nm 700 nm

Frequency Frequency of wave depends on wavelength and speed c= λ  f f = c /  Units make sense:

Frequency Typical frequency of visible light Huge number So we characterize light by wavelength

Visible light is small part of the electromagnetic spectrum

Different colors correspond to different wavelengths Wavelength is proportional to 1/ frequency

Speed, c Speed of light in a vacuum (outer space) 3 x 10 8 meters / second (299,792,458 m/s) 6.7 x 10 8 miles per hour Moon is 384,403 km away Takes 1.2 s for light go from moon to earth Sun is 149,600,000 km Takes light 8 min 19 s to get from sun to earth

Speed of light in other materials Light moves slower in matter Index of refraction = speed in vacuum speed in matter n depends on material More light interacts, the slower it goes

Speed of light in a material (v) versus index of refraction, n v = c / n water glass diamond silicon

What happens when light goes from one material into another?

What do you think will happen to the angle between the ray and the normal as it enters the water? a.It will increase (move away from the normal) b.It will stay the same c.It will decrease (move towards the normal)

What characteristics of the ray and/or the materials could be causing this? a. b. c. Possible answers?

Snell’s law quantifies bending   n 1 sin θ   n 2 sin θ  n1n1 n2n2

Snell’s law   n1n1 n2n2 and so light bends in

Snell’s law   n1n1 n2n2 If go from low to high index - light bends in towards normal

Snell’s law - in reverse   n1n1 n2n2 If go from HI to LOW index -Light bends away from normal -Light path is reversible

Can download simulator from PhET Part of homework#2 uses this simulator

Effect of changing angle and materials Can use tools to measure angles, light speed and light intensity

Outcome: Objects are not where they appear to be

Hemisphere of light above becomes a cone below

Archer fish make an adjustment

Snell’s window – see light above as a cone of light below the water Shanon Conway

How does refraction depend on wavelength?

Pink Floyd

Refraction differs with wavelength

Index of refraction depends on how much light interacts with material Glass

Snell’s law   n 1 =1.00 n 2 = n 2 = n 2 = glass Air

Snell’s law   n 1 =1.00 n 2 = n 2 = n 2 = glass Air As n 2 gets bigger… sin  2 and  2 get smaller

Snell’s law   n 1 =1.00 n 2 = n 2 = n 2 = glass Air n 2 θ  Shorter wavelength -

Snell’s law   n 1 =1.00 n 2 = n 2 = n 2 = glass Air n 2 θ  Shorter wavelength – bends MORE

PhET only does what you tell it Doesn’t have built in relationships of n and wavelength

Applications of Snell’s law Eye design Glasses design Seeing across interfaces Separating wavelengths of light

Another way to separate wavelengths – Diffractive interference Double slit – each slit becomes a point source of light

Interference

If waves are in phase – constructive interference; if they are out of phase – destructive interference Construct Destruct Construct Destruct

Constructive interference Distance two rays travel must differ by a multiple # of whole wavelengths r = n  r  D D r

Constructive interference Distance two rays travel must differ by a multiple # of whole wavelengths r = Dsin  = nλ r  D xnxn L D r  Similar triangles  sin   L xnxn

Constructive interference occurs at distance x, which is given by: D D = distance between two slits L = distance between slits and screen x = distance between bright spots L x

Diffraction What happens as slits get closer together? For more closely spaced slits, D is smaller and bright bands are further apart What happens as wavelength gets longer?

Two slit interference

Diffraction Depends on wavelength Spots are further apart for longer 

Simulator

Diffraction depends on wavelength

Light sources

Light “source”?

Light source

Northern lights Phillipe Mousette, Quebec Canada

Biological light source Different species either make light through a luciferase reaction or have bacteria that make light and are symbionts.

Incandescent bulb California lawmaker proposes to ban the bulb

Fluorescent bulb Electric discharge inside bulb causes high speed electrons to strike coating which fluoresces

Light emitting diode

Laser

Sun is a high temperature light bulb Temperature is around 5800 K This produces broad spectrum light just like an incandescent lightbulb

Solar spectrum peaks near 500 nm

Actual solar spectrum

Measuring spectral distribution Use computerized spectrometer Collects light Disperses with diffraction grating Sends to multipixel detector

Ocean Optics spectrometer 1. Fiber in 2. Slit 3. Filter 4. Collimating mirror 5. Diffraction grating 6. Mirror 7. Lens 8. Detector

Spectra of different light sources

Relative brightness of sun and moon Sun light comes directly to earth Moonlight - sun is scattered off moon and comes to earth

Light intensity Sun is about brighter than a full moon We calculated sun to be 2 x 10 5 brighter 1candela/m 2 = 1 lux

Summary Waves Refraction - Snell’s law Interference - diffraction Light sources and spectral distribution Intensity Learning styles