The Electromagnetic Spectrum EG5503 (GIS & Earth Observation)

Slides:



Advertisements
Similar presentations
EM Waves.
Advertisements

Solar Energy and Weather
Chapter 16: Weather Factors
The Atmosphere: Structure and Temperature
Electromagnetic Radiation
Radiant Energy Electromagnetic wave, crest, trough, medium,
Principles of Radiation. 1. All object possesses (sensible) heat and emit 1. All object possesses (sensible) heat and emit radiation energy as long as.
Energy Ability to do work Many different forms Conservation of energy (Law) Transformed: example: – Radiant to Thermal – Kinetic to Thermal (friction)
Waves and Light. A wave is a pattern that moves. A wave is a pattern that moves. As the pattern moves, the medium may “jiggle”, but on average it stays.
16-1 Energy in Earth’s Atmosphere. (pages 542–545) 1
27 Light Light is the ONLY thing you see! All visible objects either emit or reflect light.
MET 60: Chapter: 4 (W&H) and 2 (Stull) Radiative Transfer Dr. Craig Clements San José State University.
Energy interactions in the atmosphere
Radiation Heat Transfer. The third method of heat transfer How does heat energy get from the Sun to the Earth? There are no particles between the Sun.
Handout (yellow) Solar Energy and the Atmosphere Standard 3 Objective 1 Indicators a, b, and c Standard 3 Objectives 1, 2, and 3 Workbook Pages 3,
Chapter 2: Weather Factors
ElectroMagnetic Radiation Spectrum The basics about light and waves.
Prof.Dr. Gehan Mosaad. At the end of this lecture the student must be able to:  Define electrotherapy, electric current and electromagnetic spectrum.
Solar Energy & the Atmosphere
The sun as a source of Energy Atmospheric Processes.
Waves.
Index Unit 03 Electron Configuration Module 01: Light as a Wave Based on the PowerPoints By Mr. Kevin Boudreaux, Angelo State Univerisity U03Mod01 Light.
OPTICAL MINERALOGY Dr. AZZA RAGAB.
1 Met 10 Weather Processes Jeff Gawrych Temperature, Heat Transfer and Earth’s Energy Balance.
Lesson 2 Distinguish between transmission, absorption and scattering of radiation. Discuss examples of the transmission, absorption and scattering of EM.
Light. Visible light (commonly referred to simply as light) is electromagnetic radiation that is visible to the human eye, and is responsible for the.
Waves S8P4: Students will explore the wave nature of sound and electromagnetic radiation.
Earth Science Golodolinski/Black 2009
Climate Long time, Large Area. Weather short term, small area.
EG1204: Earth Systems: an introduction Meteorology and Climate Lecture 2 Energy, radiation and temperature.
Electromagnetic Energy
The Atmosphere: Energy Transfer & Properties Weather Unit Science 10.
Topic 6. Without energy from the sun, conditions on Earth would be different. What is the energy that is radiated from the Sun? The energy that is radiated.
Chapter 18 – The Electromagnetic Spectrum and Light
Warm Up 3/6/08 More solar energy reaches the equatorial regions than the polar regions because the equatorial regions a. are covered by a greater area.
RADIATION. Insolation in tercepted sol ar radi ation.
Atmosphere: Structure and Temperature Bell Ringers:  How does weather differ from climate?  Why do the seasons occur?  What would happen if carbon.
GEOG 1112: Weather and Climate Global Energy System Sept 11, 2014.
Chapter 22 Section 2 Handout
The Atmosphere: Structure and Temperature
Warm-Up What would happen if there was no more ozone? What would happen if there was no more ozone? –We would die. What are the four layers of the atmosphere?
Ideas for Web Projects Biography of any scientist mentioned in the book High-energy Radiation (UV, X-ray,  -ray) Noble Gases (properties, use, where can.
Chapter 16 : Weather Factors Section1 : Energy in the Atmosphere By : Katelyn Angers.
Journal #22 What is the purpose of a barometer? What is the most commonly used barometer?
Effects of Electromagnetic Waves Light: Temperature, Scattering & Absorption.
Composition of the Atmosphere 14 Atmosphere Characteristics  Weather is constantly changing, and it refers to the state of the atmosphere at any given.
17 Chapter 17 The Atmosphere: Structure and Temperature.
 A system of satellites, ground monitoring stations, and receivers that determine your exact location at or above Earth’s surface.  Global Positioning.
Copyright © Houghton Mifflin Harcourt Publishing Company Unit 3 Lesson 1 The Electromagnetic Spectrum.
Electromagnetic Radiation Principles
Energy from the Sun Radiation is the transfer of energy by electromagnetic waves. Ninety-nine percent of the radiation from the Sun consists of visible.
3.1 Heat Transfer in the Atmosphere
Waves Friday, January 8, 2010.
Today's Outline Topic: Energy Transfer Class Outline: - Weather Tracking - Energy Transfer note - Worksheet - Start a documentary Today’s Assigned.
The Greenhouse Effect.
Behavior of Waves.
Electromagnetic Radiation
17.1 Atmosphere Characteristics
What is light?.
Energy from the Sun Sun’s energy travels 148 million km to Earth in only 8 minutes Earth receives less than one-billionth of the Sun’s energy Reaches Earth.
Radiation in the Atmosphere
17.2 Heating the Atmosphere
Quiz # 2 1. In which portion of the electromagnetic spectrum is the sun’s peak energy? 2. In which portion of the electromagnetic spectrum is the earth’s.
Heating the Atmosphere
Introduction and Basic Concepts
Introduction and Basic Concepts
REMOTE SENSING.
Electromagnetic Radiation
Energy in the Earth’s Atmosphere
Presentation transcript:

The Electromagnetic Spectrum EG5503 (GIS & Earth Observation)

Lecture Topics What is the Electromagnetic Spectrum? What is the Electromagnetic Spectrum? The concept of wavelength The concept of wavelength Properties of EMR waves Properties of EMR waves EMR and the Sun-Atmosphere system EMR and the Sun-Atmosphere system How does remote sensing exploit EMR How does remote sensing exploit EMR

What is the Electromagnetic Spectrum? The term radiation covers a wide variety of natural phenomena The term radiation covers a wide variety of natural phenomena All radiation involves the exchange of energy All radiation involves the exchange of energy The energy associated with electromagnetic radiation is called radiant energy The energy associated with electromagnetic radiation is called radiant energy Radiant energy may exist in the absence of matter Radiant energy may exist in the absence of matter

What is the Electromagnetic Spectrum? All types of EMR are transmitted, or propagated, as waves All types of EMR are transmitted, or propagated, as waves In common with all waves, the two most fundamental properties of electromagnetic waves are length and frequency In common with all waves, the two most fundamental properties of electromagnetic waves are length and frequency The longer the wavelength the lower the frequency and vice versa The longer the wavelength the lower the frequency and vice versa

The concept of wavelength Wavelength is usually measured in metres (the SI unit of length), micrometres (1µm=10 -6 m) and nanometres (1nm=10 -9 m) Wavelength is usually measured in metres (the SI unit of length), micrometres (1µm=10 -6 m) and nanometres (1nm=10 -9 m) The SI unit of frequency is hertz (cycles per second) The SI unit of frequency is hertz (cycles per second) The electromagnetic spectrum may be defined as the entire range of radiation wavelengths The electromagnetic spectrum may be defined as the entire range of radiation wavelengths

Electromagnetic spectrum with enhanced detail for visible region of the spectrum Note the large range of wavelengths encompassed in the spectrum - it is over twenty orders of magnitude!

Properties of EMR radiation Transfer energy from place to place Transfer energy from place to place Can be emitted and absorbed by matter Can be emitted and absorbed by matter Do not need a material medium to travel through Do not need a material medium to travel through Travel at 3 X 10 8 metres per second in a vacuum Travel at 3 X 10 8 metres per second in a vacuum Can be polarised (made to vibrate in a plane) Can be polarised (made to vibrate in a plane) Can be reflected and refracted Can be reflected and refracted Can be diffracted (e.g. using a prism) Can be diffracted (e.g. using a prism) Carry no electric charge Carry no electric charge

EMR and the Sun-atmosphere system In order to understand how we can measure the physical environment with remote sensing, we must first understand solar radiation In order to understand how we can measure the physical environment with remote sensing, we must first understand solar radiation The amount of energy received by a surface perpendicular to the Sun’s rays at the Earth’s outer atmosphere is called the solar constant (about 1370 J m -2 s -1 average) The amount of energy received by a surface perpendicular to the Sun’s rays at the Earth’s outer atmosphere is called the solar constant (about 1370 J m -2 s -1 average)

EMR and the Sun-atmosphere system About 50% of incoming solar radiation is lost by the atmosphere: scattered (30%) and absorbed (20%) About 50% of incoming solar radiation is lost by the atmosphere: scattered (30%) and absorbed (20%) Scattering involves the absorption and re- emission of energy by particles Scattering involves the absorption and re- emission of energy by particles Absorption (unlike scattering) involves energy exchange Absorption (unlike scattering) involves energy exchange

EMR and the Sun-atmosphere system Wavelengths less than and greater than 0.8µm (800nm) are often referred to as shortwave and longwave radiation respectively Wavelengths less than and greater than 0.8µm (800nm) are often referred to as shortwave and longwave radiation respectively The shortwave solar radiation consists of ultraviolet and visible The shortwave solar radiation consists of ultraviolet and visible The terrestrial longwave component is known as infrared The terrestrial longwave component is known as infrared

EMR and the Sun-atmosphere system Just under 50% of the radiation reaching the Earth’s surface is in the visible range Just under 50% of the radiation reaching the Earth’s surface is in the visible range Components of visible light are referred to as colours Components of visible light are referred to as colours Each colour behaves differently and white light can be separated out by use of a prism Each colour behaves differently and white light can be separated out by use of a prism Colour separation occurs because of differential refraction Colour separation occurs because of differential refraction

EMR and the Sun-atmosphere system The human eye cannot see infrared radiation The human eye cannot see infrared radiation Infrared radiation is absorbed by water vapour and carbon dioxide in the troposphere Infrared radiation is absorbed by water vapour and carbon dioxide in the troposphere The atmosphere’s relative transparency to incoming solar (SW) radiation, and ability to absorb/re-emit outgoing infrared (LW) radiation is the natural greenhouse effect The atmosphere’s relative transparency to incoming solar (SW) radiation, and ability to absorb/re-emit outgoing infrared (LW) radiation is the natural greenhouse effect

Remote Sensing and EMR Remote sensing exploits the different characteristics of the electromagnetic spectrum Remote sensing exploits the different characteristics of the electromagnetic spectrum Satellites use channels - a channel corresponds to a specific waveband, or portion of the electromagnetic spectrum Satellites use channels - a channel corresponds to a specific waveband, or portion of the electromagnetic spectrum The European geostationary weather satellite METEOSAT for example has 3 channels The European geostationary weather satellite METEOSAT for example has 3 channels

CHANNELSPECTRAL RANGEUSE Visible0.45 to 1µmDaytime imaging Infrared10.5 to 12.5 µmTemperature estimation and Imaging Water Vapour5.7 to 7.1 µmTropospheric humidity estimation

Any Questions ?