Electromagnetic Wave Propagation High School Science Demonstration Melanie Leong June 25, 2003.

Slides:



Advertisements
Similar presentations
Radio Waves and Signals Week 4. We imagine radio signals/waves travel as sine waves. The ripple of these waves are started by the vibration of an electron.
Advertisements

Phy107 Fall From last time… Interference of waves –Constructive and Destructive interference Doppler effect –Change in apparent frequency due to.
Chaos, Communication and Consciousness Module PH19510 Lecture 6 Radio Days.
Chapter 22 Electromagnetic Waves. Units of Chapter 22 Changing Electric Fields Produce Magnetic Fields; Maxwell’s Equations Production of Electromagnetic.
Astronomy and the Electromagnetic Spectrum
Technician License Course Chapter 2 Lesson Plan Module 2 – Radio Waves & Signals.
Electromagnetic Waves
Radio Astronomy Listening to the Sky Jeremy P. Carlo N2ZLQ Renfrew County Amateur Radio Club January 17, 2011.
The Energy of Waves Physical Science.
L 28 Electricity and Magnetism [6] magnetism Faraday’s Law of Electromagnetic Induction –induced currents –electric generator –eddy currents Electromagnetic.
L 28 Electricity and Magnetism [6] magnetism Faraday’s Law of Electromagnetic Induction –induced currents –electric generator –eddy currents Electromagnetic.
Introduction to Radio Astronomy Updated February 2009.
Copyright : Hi Tech Criminal Justice, Raymond E. Foster Police Technology Police Technology Chapter Three Police Technology Wireless Communications.
EM Waves Physics 102 Professor Lee Carkner Lecture 24.
ELECTRONIC COMMUNICATION. Electronic Communication  Three parts : Transmitter, Receiver and Channel  Channel uses electrical energy  Graphic communication.
Let’s review electromagnetism. Electric Generator.
EM Waves Physics 102 Professor Lee Carkner Lecture 26.
Introduction to Wireless Communication. History of wireless communication Guglielmo Marconi invented the wireless telegraph in 1896 Communication by encoding.
AERIALS AND RADIO FREQUENCY PROPAGATION By Farhan Saeed.
Waves disturbances (but in a good way! Mostly ). Definition Tuesday July 15, 2014Waves2 Waves are disturbances that transfer energy!
Light, Photon Energies, and Atomic Spectra
Nineteenth century produced a revolution in understanding of electricity and magnetism Culminated in the work of James Maxwell. Electricity and magnetism.
The history of the radio, or wireless telegraph, dates back more than a century. Advancements over time, including voice transmissions, have led to the.
Introduction to Radio Waves Vincent L. Fish source: Windows to the Universe (UCAR)‏ Image courtesy of NRAO/AUI.
Chapter 2 Decoding the Hidden Messages in Starlight
Radio Communication SL – Option F.1. Radio communication includes any form of communication that uses radio (EM) waves to transfer information –TV, mobile.
Lecture 11 Electromagnetic Waves Chapter 21.8  Outline Discovery and Studies of Electromagnetic Waves Properties of Electromagnetic Waves The Spectrum.
Electromagnetic Spectrum
Electromagnetic Waves Chapter Introduction: Maxwell’s equations Electricity and magnetism were originally thought to be unrelated Electricity.
The Electromagnetic Spectrum and Light. Wavelength - The distance between two consecutive peaks of a wave.
RET 2013: INFORMATION IN RADIO WAVES Ken Jacobs Tim Scaduto.
Communication systems Dr. Bahawodin Baha School of Engineering University of Brighton, UK July 2007.
Guiding Questions 1. How fast does light travel? How can this speed be measured? 2. Why do we think light is a wave? What kind of wave is it? 3. How is.
4 th Period SI EM Spectrum 8 Jan 2009 NOTE: Infrared Rays are missing. The “infrared group” never turned in as of 3:15 Friday. This group will feel bad.
Electromagnetic Waves Chapter 35. Electromagnetic (EM) Waves Can travel through space Radio, Microwaves, IR, Light, UV, X-rays, Gamma Rays All on the.
Astronomy and the Electromagnetic Spectrum
RF Noise and Radio-Astronomy. A Brief History of Radio Astronomy 1860's Maxwell develops equations that govern electromagnetic (EM) waves. 1860's-1930's.
Technician License Course Chapter 2 Lesson Plan Module 2 – Radio Signals and Waves.
Let There Be Light…Explained! Electron Configuration Introduction 1.
Donna Kubik PHYS162 Fall, Because of its electric and magnetic properties, light is called electromagnetic radiation. It consists of perpendicular,
APHY201 10/24/ Maxwell’s Equations   1865 – James Maxwell unifies electricity and magnetism and shows that their fields move through space.
 Students will be able to define electromagnetic radiation.  Students will be able to explain how telescopes work.  Students will be able to describe.
By: Sean Chandler. In 1926, Hungarian engineer Kálmán Tihanyi designed a television system utilizing fully electronic scanning and display elements, and.
PHYS 1442 – Section 004 Lecture #16 Weednesday March 19, 2014 Dr. Andrew Brandt Chapter 22 Maxwell and the c.
Communications Systems. 1Analogue modulation: time domain (waveforms), frequency domain (spectra), amplitude modulation (am), frequency modulation (fm),
Technician License Course Chapter 2 Radio and Electronics Fundamentals
Objectives To be able to understand how radio was invented and by who To gain an understanding of how radio has developed over the centuries and the difference.
Waves Basics. Expectations Upon completion of this unit you will be able to: Define waves and wave pulses. Identify the two types of wave pulses. Define.
Electrons in Atoms 13.3 Physics and the Quantum Mechanical Model
Chapter 9.1 Notes Electromagnetic Waves Part 1. A changing electric field can produce a changing Magnetic Field.Magnetic Field. A changing magnetic field.
Technician License Course Chapter 2 Lesson Plan Module 2 – Radio Signals and Waves.
Astronomy Day Three Radiation, E-M Spectrum, Black Body Radiation, Doppler Effect.
S3 INNOVATION SENDING SIGNALS. STARTER – IN YOUR GROUPS… Apart from speaking give three examples of ways that information can be sent from one place to.
5.1 Electromagnetic Radiation. Wave motion The transfer of energy without matter is called wave motion Two Types.
Astronomy Day Three Radiation, E-M Spectrum, Black Body Radiation, Doppler Effect.
Chapter 3. INTRODUCTION TO CELLULAR COMMUNICATION :  Mobile communication systems include one of the largest mass-market application areas of digital.
Reginald Aubrey Fessenden. On 23 December 1900 Fessenden made the first human voice transmission by wireless. One, two, three, four. Is it snowing where.
Phy107 Fall From Last Time… Charges and currents Electric and magnetic forces Work, potential energy and voltage Today… Electric fields, magnetic.
L 29 Electricity and Magnetism [6]
L 30 Electricity and Magnetism [7]
L 28 Electricity and Magnetism [6] magnetism Faraday’s Law of Electromagnetic Induction –induced currents –electric generator –eddy currents Electromagnetic.
Power in an AC Circuit No power losses are associated with capacitors and pure inductors in an AC circuit No power losses are associated with capacitors.
Observing and exploring space
Technician License Course Chapter 2
Overview Communication is the transfer of information from one place to another. This should be done - as efficiently as possible - with as much fidelity/reliability.
From last time… Faraday: Inductance: flux = (inductance) x (current)
DO NOW In your notes… answer the following question using bullet points: What do you know about light? Causes sunburn Allows plants to make food Allows.
Radio Links.
Properties of Waves.
Introduction to Microwave
Presentation transcript:

Electromagnetic Wave Propagation High School Science Demonstration Melanie Leong June 25, 2003

Early Radio to Radio Astronomy A Brief History of Radio & A Quick Introduction to Radio Astronomy Onizuka Visitor Center Presentation Melanie Leong July 5, 2003

Agenda Brief History of Radio Explanation of Electromagnetic Waves and Frequency Electromagnetic Wave Propagation - Spark Gap Generator Quick Introduction to Radio Astronomy

A Brief History of Radio Radio is a new subject in terms of science & astronomy We receive transmitted radio waves for enjoyment, entertainment, and information 100 years ago Radio, as we know it, did not exist. 1884, James Clerk Maxwell –Calculated the speed electromagnetic waves travel is approximately the speed of light. –Visible light forms only a small part of the spectrum of electromagnetic waves.

History of Radio (p2) 1888, Heinrich Hertz –Proved that electricity could be transformed into electromagnetic waves. –These waves travel at the speed of light. 1896, Guglielmo Marconi –Built a wireless telegraph, a spark gap transmitter & receiver –On December 12, 1901, accomplished the “Atlantic Leap” from Poldhu, Cornwall, England to Signal Hill, Newfoundland

History of Radio (p3) 1900, Reginald Fessenden –Continuous Waves necessary to transmit speech and music –December 23, 1900, First wireless voice message to colleague “Hello Brant. One. Two. Three. Four. Is it snowing where you are Mr. Theissen? If it is, telegraph back and let me know.” Transmit and receive stations were only 1 mile apart, but this heralded the beginning of radio telephony. –On Christmas Day 1906, Ships 100 miles away heard Fessenden’s voice and “O Holy Night” playing on their morse code receivers. – , Radio Broadcast Development

History of Radio (p4) 1924, Spark transmission was phased out 1870’s-1920’s, Telephone developed and in service 1932, Karl Jansky –While doing research for Bell Labs for transatlantic radio service, he observed radio waves coming from the center of the Milky Way Galaxy. –Not allowed to investigate more , Grote Reber –In 1933, Read about Jansky’s work, published in the NY Times –By 1939, Built the first radio telescope in his backyard –By 1941, Measured and recorded the first radio sky map

Grote Reber’s Radio Sky Maps

What are Electromagnetic Waves? An electromagnetic wave is an energy wave produced from an electrical discharge. Electromagnetic waves have rise and fall cycles. The number of rise and fall cycles per second is its frequency. We can’t see or feel them, but they are around us.

Explanation of Frequency Everything you see, and can’t see, resonate at a specific frequency. Frequencies are sinusoidal waves. Speed of Light = Frequency x Wavelength Example: The wavelength of a signal resonating at 3kHz is: 3 x 10 8 m/s= 100 kilometers or ~ 62 miles! 3 x 10 3 Hz Lower frequencies have longer wavelengths. This characteristic allows these frequencies to be used for Morse code and amateur radio.

Diagram of Waves & Frequency

Frequency Bands

Simple Demo Reviewing what we know: Electromagnetic waves propagate through space. If there is an excitation - electrical discharge, what do you predict will happen? Electromagnetic waves will propagate from its source to throughout the room. That means a detector placed anywhere in this room will indicate that the waves have propagated.

Diagram of Demonstration key battery + - ignition coil radio

Field Coverage This spark gap generator transmits broadband emissions - It covers a large band of frequencies. With a radio tuned to an AM or Shortwave station, noise will be heard when the spark gap transmitter is energized. (530kHz to 4200kHz) Tune to another AM/Shortwave station, you should get the same electrical discharge noise. If the signal is regulated, or tuned, to one band of frequencies, communication can be gained.

Field Coverage (p2) If there is a powerful discharge and you walked outside and down the street. Will the noise still be detected? Yes! Which is why full time activation is prohibited by the FCC.

EM Wave Summary Electromagnetic Wavelength - Distance of One Cycle (peak to peak) Electromagnetic Frequency - Number of Cycles in One Second Speed of Light = Wavelength x Frequency Electromagnetic Waves propagate through space from an electrical discharge Electromagnetic Wave Propagation Uses - Communications, Astronomy, and much more

What is Radio Astronomy? It is the study of electromagnetic emissions from celestial objects in the radio spectrum band. Atoms and molecules in space emit their own unique electromagnetic waves. Radio telescopes can see “cold” objects, they do not emit light Able to detect radio sources behind interstellar clouds hidden from optical viewing. Can detect distant galaxies at the edge of the Universe

CSO Atmospheric Transmission

350 µm Survey of Orion KL

Sagittarius A - Galactic Center

Arches Cluster in Sagittarius - Optical

Arches Cluster in Sagittarius - Radio

Sagittarius Arches in Optical & Radio

Sgr Arches in Optical & X-Ray/IR

Sagittarius - Arches Cluster Optical X-Ray/InfraredRadio

Summary There’s much more out there than visible light. What is seen in radio waves is very different than optical. Electromagnetic waves detected by Radio Telescopes tell us more about what else is going on out there. All spectrum bands are used to observe, measure, and interpret what is going on out in the Universe. Many different ground based and space based telescopes are made to accomplish this.