OPAC 101 Introduction to Optics

Similar documents
What are the six common sources of light?

2. Discrete means unique, that other states don t overlap it. 3. Electrons in the outer electron shells have greater potential energy.

Modern optics Lasers

Light Emission. Today s Topics. Excitation/De-Excitation 10/26/2008. Excitation Emission Spectra Incandescence

Experiment 24: Spectroscopy

Higher -o-o-o- Past Paper questions o-o-o- 3.4 Spectra

Chemistry 212 ATOMIC SPECTROSCOPY

APAS Laboratory { PAGE } Spectroscopy SPECTROSCOPY

The Spectroscopy of Stars

1 Electrons are emitted from a metal surface when it is illuminated with suitable electromagnetic radiation. ...[1]

Chapter 5: Light and Matter: Reading Messages from the Cosmos

Light Emission.

LASERS AGAIN? Phys 1020, Day 17: Questions? LASERS: Next Up: Cameras and optics Eyes to web: Final Project Info

progressive electromagnetic wave

Atomic Theory C &03

Chapter 5 Light and Matter: Reading Messages from the Cosmos. 5.1 Light in Everyday Life. How do we experience light?

Light and Matter: Reading Messages from the Cosmos. White light is made up of many different colors. Interactions of Light with Matter

Experiment 4 Radiation in the Visible Spectrum

LASER. Challenging MCQ questions by The Physics Cafe. Compiled and selected by The Physics Cafe

ASTRO Fall 2012 LAB #7: The Electromagnetic Spectrum

Because light behaves like a wave, we can describe it in one of two ways by its wavelength or by its frequency.

Atomic Spectroscopy. Objectives

Atomic Spectra for Atoms and Ions. Light is made up of different wavelengths

Chapter 5 Electrons In Atoms

Chapter 5 Light and Matter: Reading Messages from the Cosmos

A100H Exploring the Universe: The interaction of light and matter. Martin D. Weinberg UMass Astronomy

Higher Physics. Particles and Waves

Chapter 24 Photonics Question 1 Question 2 Question 3 Question 4 Question 5

End-of-Chapter Exercises

LASER. Light Amplification by Stimulated Emission of Radiation

Classical and Planck picture. Planck s constant. Question. Quantum explanation for the Wein Effect.

Interested in exploring science or math teaching as a career?

Black Body Radiation and Planck's Quantum Hypothesis

Chapter 5 Light and Matter: Reading Messages from the Cosmos. How do we experience light? Colors of Light. How do light and matter interact?

LASERS. Dr D. Arun Kumar Assistant Professor Department of Physical Sciences Bannari Amman Institute of Technology Sathyamangalam

Properties of Electromagnetic Radiation Chapter 5. What is light? What is a wave? Radiation carries information

Experiment 3 1. The Michelson Interferometer and the He- Ne Laser Physics 2150 Experiment No. 3 University of Colorado

Prof. Jeff Kenney Class 5 June 1, 2018

RAY OPTICS 6. DISPERSION POINTS TO REMEMBER

Core Concept. PowerPoint Lectures to accompany Physical Science, 8e. Chapter 7 Light. New Symbols for this Chapter 3/29/2011

What can laser light do for (or to) me?

A World of Color. Session 2. OLLI at Illinois Spring D. H. Tracy

AS 101: Day Lab #2 Summer Spectroscopy


Introduction to Electromagnetic Radiation and Radiative Transfer

Light is an important form of energy for all of us

Light sources. Excited gas atoms are the primaty source of radiation in combustion and discharge lamps. lamps is not continuous!

Chapter 17, Electromagnetic Waves Physical Science, McDougal-Littell, 2008

Ch 9 Electrons in Atoms & the Periodic Table Study Sheet Acc. Chemistry SCANTRON. Name /99. 3) Light is a type of matter. 3)

Name the region of the electromagnetic radiation emitted by the laser. ...

Experiment 3 Electromagnetic Radiation and Atom Interaction

1) Introduction 2) Photo electric effect 3) Dual nature of matter 4) Bohr s atom model 5) LASERS

What makes the color pink? Black and white TV summary. Different color phosphors. Color TV. Different color pixels

(i) Show that the energy of a single photon is about 3 x J.

Today. Spectra. Thermal Radiation. Wien s Law. Stefan-Boltzmann Law. Kirchoff s Laws. Emission and Absorption. Spectra & Composition

Thermal Radiation By: Prof. K M Joshi

Laserphysik. Prof. Yong Lei & Dr. Yang Xu. Fachgebiet Angewandte Nanophysik, Institut für Physik

L 18 Thermodynamics [3] Heat flow. Conduction. Convection. Thermal Conductivity. heat conduction. Heat transfer

EM SPECTRUM, WAVELENGTH, FREQUENCY, AND ENERGY WORKSHEET

Experiment 9. Emission Spectra. measure the emission spectrum of a source of light using the digital spectrometer.

Lightbulbs. Lecture 18 : Blackbody spectrum Improving lightbulb efficiency

The Electromagnetic Spectrum

10/21/2015. Lightbulbs. Blackbody spectrum. Temperature and total emitted power (brightness) Blackbody spectrum and temperature

EXPERIMENT 17: Atomic Emission

ACTIVITY 2 Exploring Light Patterns

Duncan. Electrons, Energy, & the Electromagnetic Spectrum Notes Simplified, 2-D Bohr Model: Figure 1. Figure 2. Figure 3

Instructor: Welcome to. Phys 774: Principles of Spectroscopy. Fall How can we produce EM waves? Spectrum of Electromagnetic Radiation and Light

The Nature of Light I: Electromagnetic Waves Spectra Kirchoff s Laws Temperature Blackbody radiation

From Last Time Pearson Education, Inc.

Chapter 28 Assignment Solutions

Electromagnetic waves

LECTURE # 17 Modern Optics Matter Waves

Unit I LASER Engineering Physics

Atomic Emission Spectra

Sunlight. 1 radiation.

ELECTROMAGNETIC WAVES ELECTROMAGNETIC SPECTRUM

Light. Mike Maloney Physics, SHS

Chapter 4 Spectroscopy

Taking fingerprints of stars, galaxies, and interstellar gas clouds

aka Light Properties of Light are simultaneously

Preview from Notesale.co.uk Page 1 of 38

X-Rays from Atoms. These are called K α X-rays See table 29.1 for the energy of K α X-rays produced by some elements. Section 29.3

DAY LABORATORY EXERCISE: SPECTROSCOPY

Susan Cartwright Our Evolving Universe 1

Modern physics ideas are strange! L 36 Modern Physics [2] The Photon Concept. How are x-rays produced? The uncertainty principle

Chapter 5 Electrons In Atoms

Today. Kirchoff s Laws. Emission and Absorption. Stellar Spectra & Composition. Doppler Effect & Motion. Extrasolar Planets

c = λν 10/23/13 What gives gas-filled lights their colors? Chapter 5 Electrons In Atoms

Taking fingerprints of stars, galaxies, and interstellar gas clouds. Absorption and emission from atoms, ions, and molecules

PHYS General Physics II Lab The Balmer Series for Hydrogen Source. c = speed of light = 3 x 10 8 m/s

Chapter 13. Phys 322 Lecture 34. Modern optics

DIFFRACTION GRATING. OBJECTIVE: To use the diffraction grating in the formation of spectra and in the measurement of wavelengths.

Photochemical principles

hf = E 1 - E 2 hc = E 1 - E 2 λ FXA 2008 Candidates should be able to : EMISSION LINE SPECTRA

Chapter 6. Quantum Theory and the Electronic Structure of Atoms Part 1

Single Slit Diffraction and Resolving Power. Quantum Mechanics: Blackbody Radiation & Photoelectric Effect. Physics 102: Lecture 22

9/16/08 Tuesday. Chapter 3. Properties of Light. Light the Astronomer s Tool. and sometimes it can be described as a particle!

Question 11.1: Find the

Chapter 11 FUNDAMENTALS OF THERMAL RADIATION

Lecture5PracticeQuiz.txt

Transcription:

OPAC 101 Introduction to Optics Topic 2 Light Sources Department of http://www1.gantep.edu.tr/~bingul/opac101 Optical & Acustical Engineering Gaziantep University Sep 2017 Sayfa 1

Light Sources: maybe natural or artificial Sunlight, skylight Fire Incandecent sources Blackbody sources Tungsten flament Discharge lamps (Gas Filled Tubes) Monochromatic and spectral sources High-intensity sources Semiconductor light-emitting diodes (LEDs) Coherent source (laser) Sayfa 2

Day Light: combination of sunlight and skylight Sayfa 3

Sun Wavelength distribution measured in our laboratory Sayfa 4

Tungsten Bulb Tungsten Halogen Lamb is an incandescent (=akkor) lamp that has a small amount of a halogen such as iodine or bromine added. Sayfa 5

Tungsten Bulb Typical wavelength distribution as a function of temperature: Sayfa 6

Tungsten Bulb Wavelength distribution measured in our laboratory Sayfa 7

Flame Wavelength distribution measured in our laboratory Sayfa 8

Discharge Lamps(Gas Filled Tubes) Gas-discharge lamps are a family of artificial light sources that generate light by sending an electric discharge through an ionized gas, a plasma. Typically, such lamps use a noble gas (argon, neon, krypton, and xenon) or a mixture of these gases. Each gas, depending on its atomic structure, emits certain wavelengths. The emission spectrum determines the color of the light from the lamp. Sayfa 9

Discharge Lamps (Gas Filled Tubes) Sayfa 10

Some Wavelength distributions measured in our laboratory Sayfa 11

LED A light-emitting diode (LED) is a semiconductor light source. Circuit Symbol: A LED can produce the visible, ultraviolet and infrared wavelengths, with very high brightness. Sayfa 12

Wavelength distributions of some colored LEDs measured in our laboratory. Sayfa 13

Wavelength distribution of a white LED measured in our laboratory. Sayfa 14

LEDs in ILLUMINATION Admittedly, illumination is one of the main requirements of people. LED (Light Emitting Diode) is an energy-saving light source providing high light efficiency and long life time. Nowadays, many cities across North America, China and Europe start to prefer LED for internal/external/street illumination. In Türkiye, both government politics and companies working many years on the illumination sector foresee that all illumination systems are going to be based on LEDs in the near future. Long Distance Illumination LED Projector Sayfa 15

LASER Laser" stands for Light Amplification by Stimulated Emission of Radiation A laser is a device that emits light through a process of optical amplification based on the stimulated emission of photons. A Laser is coherent, monochromatic and collimated light. A Laser light can be * visible * infrared * ultraviolet * X-ray Sayfa 16

Laser is highly collimated --> beam divergence ~ mrad (milli-radians) Properties of an example laser pointer (GLP-III-594) Sayfa 17

EXAMLPE Consider laser pointer whose aperture diameter is D = 1.5 mm and beam divergence is Δθ = 1.5 mrad (=0.086 o ). What is the diameter of the laser spot on a screen at a distance L = 100 m away from the pointer? SOLUTION Δθ/2 L D D From figure: tan( / 2) D' / 2 L D 2L tan( / 2) (2)(100 m) tan(0.086 o / 2) 0.15 m 15 cm Sayfa 18

LED vs Laser Comparison of Beam Divergence of LED and Laser Sayfa 19

LED vs Laser blue green red Spectral width of the laser is 10,000 times narrower than the spectral width of a light-emitting diode. LED Helium-Neon laser spectrum Sayfa 20

Laser Radiation Lasers can cause damage in biological tissues, both to the eye and to the skin. Unprotected Human Eye is extremely sensitive to laser radiation and can be permanently damaged from direct or reflected beams. High power lasers can also burn the skin. Sayfa 21

Blackbody Radiation If you turn on an electric stove, the stove plate heats up until it becomes red or orange hot. The red glow that you see consists of photons with energies in the visible red range. When the stove plate was cold, it also emitted photons, but those were of too low energy to be seen by our eyes. Sayfa 22

All objects radiate energy continuously in the form of electromagnetic waves produced by thermal vibrations of the molecules. The characteristics of this radiation depend on the temperature and properties of the object s surface. Every second, approximately 1370 J of electromagnetic radiation from the Sun passes perpendicularly through each 1 m 2 at the top of the Earth s atmosphere. Sayfa 23

BlackBody: ideal absorber & ideal emitter Hot objects emits thermal radiation. From a classical viewpoint, thermal radiation originates from accelerated charged particles in the atoms near the surface of the object; Blackbody is an ideal system that absorbs all radiation incident on it. The electromagnetic radiation emitted by the black body is called blackbody radiation. Sayfa 24

Blackbody Spectrum When a black body heated a distribution of wavelength is observed. The distribution was perfectly explanined by M. Planck (1900). Sayfa 25

Blackbody Spectrum Intensity of blackbody radiation versus wavelength at three temperatures. The amount of radiation emitted (the area under a curve) increases with increasing temperature. Sayfa 26

BlackBody: spectrum Intensity of blackbody radiation versus wavelength and temperatures. max T 0.0029 m K λ max = peak position T = surface temperature Sayfa 27

BlackBody max T 0.0029 m K Sayfa 28

Example Can you estimate the surface temperature of Sun? (See distibution on page 3) max T 0.0029 m K Sayfa 29