11/18/2010. Only part of the spectrum we can see. A rainbow of colors, each corresponding to a different wavelength.

Size: px
Start display at page:

Download "11/18/2010. Only part of the spectrum we can see. A rainbow of colors, each corresponding to a different wavelength."

Transcription

1 The sun is the source of energy to heat the Earth s surface. Solar energy makes it s way to Earth by an energy transfer mechanism called radiation. Energy transferred this way travels outwards in all directions from it s source. The sun emits an array of electromagnetic radiation of varying wavelengths. Light Heat Ultraviolet Radiation All wavelengths travel through space at the speed of light. Waves or rays come in varying length. The shortest waves are gamma rays. The longest are radio waves. Infrared radiation is felt as heat. Ultraviolet rays cause sunburn. Only part of the spectrum we can see. A rainbow of colors, each corresponding to a different wavelength. 5 1

2 Longest wavelength produces the color red. All objects, regardless of temperature, emit radiation. Shortest wavelength produces the color violet. The hotter the radiating body, the shorter the wavelengths of emission. The sun emits energy in the visible range. The Earth radiates energy in the infrared range. Objects that are good absorbers of radiation are also good emitters. Earth and Sun absorb and radiate with nearly 100% efficiency. Gases are selective absorbers and radiators. INTERACTIV E Scattering is the process by which gases and tiny particles in the atmosphere redirect light. This is how light reaches into a shaded area or room when sunlight is absent. The percentage of total radiation reflected by a surface. Albedo varies with conditions, but the averages are: 30% reflected back to space 5% by the atmosphere 20% by clouds 5% by the land/sea surface 2

3 The angle of the sun s rays influence the percentage of light reflected. The greater the angle of the sun, the longer the path through the atmosphere. Rays striking the Earth near the poles must travel through more atmosphere than those near the equator. A longer path through the atmosphere increases the amount of scattering and reflection. When albedo increases, there is less solar energy available. When albedo decreases, there is more solar energy available. The term Greenhouse Effect describes how the Earth is heated. Video Clip 3

4 Carbon dioxide (CO2) and water vapor (H2O) are the primary heat-absorbing gases. They reradiate this energy away in all directions. Some of this energy is trapped by the atmosphere in the form of heat. The Earth is about 30 degrees Celcius (50 degrees Farenheit) warmer than it would be without the an atmosphere. Since gases are selective absorbers, the atmosphere transfers most incoming heat to the Earth s surface, where it is absorbed. Air is heated when water vapor and carbon dioxide absorb the longer wavelength radiation emitted by the Earth. Any change in the air s carbon dioxide content could alter the temperature in the lower atmosphere. Fossil fuel combustion has contributed to an increase of about % of CO 2 since Significant temperature increases could lead to the melting of the polar ice caps and changes to weather patterns. 4

5 2. Sun: 2. Stove: 3. Sunscreen: 4. Electromagnetic spectrum: 5. Visible spectrum: 6. Prism: 7. Iceberg: 8. Wavelengths: Scattering: Albedo: Earth s Energy Budget: BW: Color: Solar Radiation: Greenhouse: Greenhouse Effect: Ice Age: Climate Change: 5

Chapter 2. Heating Earth's Surface & Atmosphere

Chapter 2. Heating Earth's Surface & Atmosphere Chapter 2 Heating Earth's Surface & Atmosphere Topics Earth-Sun Relationships Energy, Heat and Temperature Mechanisms of Heat Transfer What happens to Incoming Solar Radiation? Radiation Emitted by the

More information

HEATING THE ATMOSPHERE

HEATING THE ATMOSPHERE HEATING THE ATMOSPHERE Earth and Sun 99.9% of Earth s heat comes from Sun But

More information

Directed Reading. Section: Solar Energy and the Atmosphere RADIATION. identical point on the next wave. waves

Directed Reading. Section: Solar Energy and the Atmosphere RADIATION. identical point on the next wave. waves Skills Worksheet Directed Reading Section: Solar Energy and the Atmosphere 1. How is Earth s atmosphere heated? 2. Name the two primary sources of heat in the atmosphere. RADIATION In the space provided,

More information

4.2 Properties of Visible Light Date: (pages )

4.2 Properties of Visible Light Date: (pages ) 4.2 Properties of Visible Light Date: (pages 144-149) Visible light is a mixture of all the colours of the rainbow. A prism refracts light separating the colours. A second prism can recombine the colours

More information

PHYS:1200 LECTURE 18 THERMODYNAMICS (3)

PHYS:1200 LECTURE 18 THERMODYNAMICS (3) 1 PHYS:1200 LECTURE 18 THERMODYNAMICS (3) This lecture presents a more detailed discussion of heat flow by radiation and its importance in the physics of the atmosphere. We will discuss some important

More information

Key Concept Heat in Earth s atmosphere is transferred by radiation, conduction, and convection.

Key Concept Heat in Earth s atmosphere is transferred by radiation, conduction, and convection. Section 2 Atmospheric Heating Key Concept Heat in Earth s atmosphere is transferred by radiation, conduction, and convection. What You Will Learn Solar energy travels through space as radiation and passes

More information

Prentice Hall EARTH SCIENCE. Tarbuck Lutgens

Prentice Hall EARTH SCIENCE. Tarbuck Lutgens Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 17 The Atmosphere: Structure and Temperature 17.1 Atmosphere Characteristics Composition of the Atmosphere Weather is constantly changing, and it refers

More information

1. The frequency of an electromagnetic wave is proportional to its wavelength. a. directly *b. inversely

1. The frequency of an electromagnetic wave is proportional to its wavelength. a. directly *b. inversely CHAPTER 3 SOLAR AND TERRESTRIAL RADIATION MULTIPLE CHOICE QUESTIONS 1. The frequency of an electromagnetic wave is proportional to its wavelength. a. directly *b. inversely 2. is the distance between successive

More information

Earth s Energy Budget: How Is the Temperature of Earth Controlled?

Earth s Energy Budget: How Is the Temperature of Earth Controlled? 1 NAME Investigation 2 Earth s Energy Budget: How Is the Temperature of Earth Controlled? Introduction As you learned from the reading, the balance between incoming energy from the sun and outgoing energy

More information

Name(s) Period Date. Earth s Energy Budget: How Is the Temperature of Earth Controlled?

Name(s) Period Date. Earth s Energy Budget: How Is the Temperature of Earth Controlled? Name(s) Period Date 1 Introduction Earth s Energy Budget: How Is the Temperature of Earth Controlled? As you learned from the reading, the balance between incoming energy from the sun and outgoing energy

More information

ATM S 111: Global Warming Solar Radiation. Jennifer Fletcher Day 2: June

ATM S 111: Global Warming Solar Radiation. Jennifer Fletcher Day 2: June ATM S 111: Global Warming Solar Radiation Jennifer Fletcher Day 2: June 22 2010 Yesterday We Asked What factors influence climate at a given place? Sunshine (and latitude) Topography/mountains Proximity

More information

Meteorology Pretest on Chapter 2

Meteorology Pretest on Chapter 2 Meteorology Pretest on Chapter 2 MULTIPLE CHOICE 1. The earth emits terrestrial radiation a) only at night b) all the time c) only during winter d) only over the continents 2. If an imbalance occurs between

More information

Topic 5 Practice Test

Topic 5 Practice Test Base your answers to questions 1 and 2 on the diagram below, which represents the greenhouse effect in which heat energy is trapped in Earth's atmosphere 1. The Earth surface that best absorbs short-wave

More information

Introduction to Electromagnetic Radiation and Radiative Transfer

Introduction to Electromagnetic Radiation and Radiative Transfer Introduction to Electromagnetic Radiation and Radiative Transfer Temperature Dice Results Visible light, infrared (IR), ultraviolet (UV), X-rays, γ-rays, microwaves, and radio are all forms of electromagnetic

More information

Investigating Planets Name: Block: E1:R6

Investigating Planets Name: Block: E1:R6 FYI: Planetary Temperatures and Atmospheres Read FYI: A Planet s Temperature, The Importance of an Atmosphere, and The Greenhouse Effect As you read answer the following questions about the readings: Word/Term

More information

1. Weather and climate.

1. Weather and climate. Lecture 31. Introduction to climate and climate change. Part 1. Objectives: 1. Weather and climate. 2. Earth s radiation budget. 3. Clouds and radiation field. Readings: Turco: p. 320-349; Brimblecombe:

More information

NOTES: 5.3 Light and Atomic Spectra (more Quantum Mechanics!)

NOTES: 5.3 Light and Atomic Spectra (more Quantum Mechanics!) NOTES: 5.3 Light and Atomic Spectra (more Quantum Mechanics!) Light WAVE or PARTICLE? Electromagnetic Radiation Electromagnetic radiation includes: -radio waves -microwaves -infrared waves -visible light

More information

Energy and Insolation Review 2

Energy and Insolation Review 2 Energy and Insolation Review 2 The diagram below shows a container of water that is being heated. 1. The movement of water shown by the arrows is most likely caused by (1) density differences (2) insolation

More information

Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.

Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc. Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric properties

More information

9/1/14. Chapter 2: Heating Earth s Surface and Atmosphere. The Atmosphere: An Introduction to Meteorology, 12 th. Lutgens Tarbuck

9/1/14. Chapter 2: Heating Earth s Surface and Atmosphere. The Atmosphere: An Introduction to Meteorology, 12 th. Lutgens Tarbuck Chapter 2: Heating Earth s Surface and Atmosphere The Atmosphere: An Introduction to Meteorology, 12 th Lutgens Tarbuck Lectures by: Heather Gallacher, Cleveland State University! Earth s two principal

More information

Energy and the Earth AOSC 200 Tim Canty

Energy and the Earth AOSC 200 Tim Canty Energy and the Earth AOSC 200 Tim Canty Class Web Site: http://www.atmos.umd.edu/~tcanty/aosc200 Topics for today: Energy absorption Radiative Equilibirum Lecture 08 Feb 21 2019 1 Today s Weather Map http://www.wpc.ncep.noaa.gov/sfc/namussfcwbg.gif

More information

Lecture 6. Solar vs. terrestrial radiation and the bare rock climate model.

Lecture 6. Solar vs. terrestrial radiation and the bare rock climate model. Lecture 6 Solar vs. terrestrial radiation and the bare rock climate model. Radiation Controls energy balance of Earth Is all around us all the time. Can be labeled by its source (solar, terrestrial) or

More information

Energy, Temperature, & Heat. Energy, Temperature, & Heat. Temperature Scales 1/17/11

Energy, Temperature, & Heat. Energy, Temperature, & Heat. Temperature Scales 1/17/11 Energy, Temperature, & Heat Energy is the ability to do work (push, pull, lift) on some form of matter. Chapter 2 Potential energy is the potential for work (mass x gravity x height) Kinetic energy is

More information

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Physics Problem Solving 10: The Greenhouse Effect. Section Table and Group

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Physics Problem Solving 10: The Greenhouse Effect. Section Table and Group MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Physics 8.02 Problem Solving 10: The Greenhouse Effect Section Table and Group Names Hand in one copy per group at the end of the Friday Problem Solving

More information

The Atmosphere: Structure and Temperature

The Atmosphere: Structure and Temperature Chapter The Atmosphere: Structure and Temperature Geologists have uncovered evidence of when Earth was first able to support oxygenrich atmosphere similar to what we experience today and more so, take

More information

Lecture 5: Greenhouse Effect

Lecture 5: Greenhouse Effect Lecture 5: Greenhouse Effect S/4 * (1-A) T A 4 T S 4 T A 4 Wien s Law Shortwave and Longwave Radiation Selected Absorption Greenhouse Effect Global Energy Balance terrestrial radiation cooling Solar radiation

More information

Frequency: the number of complete waves that pass a point in a given time. It has the symbol f. 1) SI Units: Hertz (Hz) Wavelength: The length from

Frequency: the number of complete waves that pass a point in a given time. It has the symbol f. 1) SI Units: Hertz (Hz) Wavelength: The length from Frequency: the number of complete waves that pass a point in a given time. It has the symbol f. 1) SI Units: Hertz (Hz) Wavelength: The length from the one crest of a wave to the next. I. Electromagnetic

More information

ATS150 Global Climate Change Spring 2019 Candidate Questions for Exam #1

ATS150 Global Climate Change Spring 2019 Candidate Questions for Exam #1 1. How old is the Earth? About how long ago did it form? 2. What are the two most common gases in the atmosphere? What percentage of the atmosphere s molecules are made of each gas? 3. About what fraction

More information

Earth s Atmosphere. Energy Transfer in the Atmosphere. 3. All the energy from the Sun reaches Earth s surface.

Earth s Atmosphere. Energy Transfer in the Atmosphere. 3. All the energy from the Sun reaches Earth s surface. CHAPTER 11 LESSON 2 Earth s Atmosphere Energy Transfer in the Atmosphere Key Concepts How does energy transfer from the Sun to Earth and to the atmosphere? How are air circulation patterns within the atmosphere

More information

Topic 6: Insolation and the Seasons

Topic 6: Insolation and the Seasons Topic 6: Insolation and the Seasons Solar Radiation and Insolation Insolation: In Sol ation The Sun is the primary source of energy for the earth. The rate at which energy is radiated is called Intensity

More information

Lecture 4: Radiation Transfer

Lecture 4: Radiation Transfer Lecture 4: Radiation Transfer Spectrum of radiation Stefan-Boltzmann law Selective absorption and emission Reflection and scattering Remote sensing Importance of Radiation Transfer Virtually all the exchange

More information

Chapter 11 Lecture Outline. Heating the Atmosphere

Chapter 11 Lecture Outline. Heating the Atmosphere Chapter 11 Lecture Outline Heating the Atmosphere They are still here! Focus on the Atmosphere Weather Occurs over a short period of time Constantly changing Climate Averaged over a long period of time

More information

Lecture 4: Heat, and Radiation

Lecture 4: Heat, and Radiation Lecture 4: Heat, and Radiation Heat Heat is a transfer of energy from one object to another. Heat makes things warmer. Heat is measured in units called calories. A calorie is the heat (energy) required

More information

Lecture Outlines PowerPoint. Chapter 16 Earth Science 11e Tarbuck/Lutgens

Lecture Outlines PowerPoint. Chapter 16 Earth Science 11e Tarbuck/Lutgens Lecture Outlines PowerPoint Chapter 16 Earth Science 11e Tarbuck/Lutgens 2006 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors

More information

Spectrum of Radiation. Importance of Radiation Transfer. Radiation Intensity and Wavelength. Lecture 3: Atmospheric Radiative Transfer and Climate

Spectrum of Radiation. Importance of Radiation Transfer. Radiation Intensity and Wavelength. Lecture 3: Atmospheric Radiative Transfer and Climate Lecture 3: Atmospheric Radiative Transfer and Climate Radiation Intensity and Wavelength frequency Planck s constant Solar and infrared radiation selective absorption and emission Selective absorption

More information

The Atmosphere and Atmospheric Energy Chapter 3 and 4

The Atmosphere and Atmospheric Energy Chapter 3 and 4 The Atmosphere and Atmospheric Energy Chapter 3 and 4 Size of the Earth s Atmosphere Atmosphere produced over 4.6 billion years of development Protects us from radiation Completely surrounds the earth

More information

Temperature Scales

Temperature Scales TEMPERATURE is a measure of the internal heat energy of a substance. The molecules that make up all matter are in constant motion. By internal heat energy, we really mean this random molecular motion.

More information

Period 13 Solutions: Earth as an Energy System

Period 13 Solutions: Earth as an Energy System Period 13 Solutions: Earth as an Energy System 13.1 The Earth-Sun System 1) Energy from the sun Observe the models of the Earth, Moon, and Sun in the room. a) Imagine that the distance between the Earth

More information

Lecture 3: Atmospheric Radiative Transfer and Climate

Lecture 3: Atmospheric Radiative Transfer and Climate Lecture 3: Atmospheric Radiative Transfer and Climate Solar and infrared radiation selective absorption and emission Selective absorption and emission Cloud and radiation Radiative-convective equilibrium

More information

Black Body Radiation and Planck's Quantum Hypothesis

Black Body Radiation and Planck's Quantum Hypothesis Section 3: Black Body Radiation and Planck's Quantum Hypothesis Definitions Opaque materials: materials in which no light is allowed to pass through; all light is either absorbed or reflected. Radiation:

More information

Lecture 5: Greenhouse Effect

Lecture 5: Greenhouse Effect /30/2018 Lecture 5: Greenhouse Effect Global Energy Balance S/ * (1-A) terrestrial radiation cooling Solar radiation warming T S Global Temperature atmosphere Wien s Law Shortwave and Longwave Radiation

More information

In the space provided, write the letter of the description that best matches the term or phrase. as waves. thermosphere

In the space provided, write the letter of the description that best matches the term or phrase. as waves. thermosphere Skills Worksheet Concept Review In the space provided, write the letter of the description that best matches the term or phrase. 1. layers of the atmosphere 2. radiation 3. conduction 4. convection 5.

More information

Very Dynamic! Energy in the Earth s Atmosphere. How Does it Get Here? All Objects Radiate Energy!

Very Dynamic! Energy in the Earth s Atmosphere. How Does it Get Here? All Objects Radiate Energy! Energy in the Earth s Atmosphere Unit Essential Question: What are the different features of the atmosphere that characterize our weather. How does the atmosphere influence life and how does life influence

More information

Atmospheric Radiation

Atmospheric Radiation Atmospheric Radiation NASA photo gallery Introduction The major source of earth is the sun. The sun transfer energy through the earth by radiated electromagnetic wave. In vacuum, electromagnetic waves

More information

Lecture 3: Global Energy Cycle

Lecture 3: Global Energy Cycle Lecture 3: Global Energy Cycle Planetary energy balance Greenhouse Effect Vertical energy balance Latitudinal energy balance Seasonal and diurnal cycles Solar Flux and Flux Density Solar Luminosity (L)

More information

Section 2: The Atmosphere

Section 2: The Atmosphere Section 2: The Atmosphere Preview Classroom Catalyst Objectives The Atmosphere Composition of the Atmosphere Air Pressure Layers of the Atmosphere The Troposphere Section 2: The Atmosphere Preview, continued

More information

Name Class Date. What two models do scientists use to describe light? What is the electromagnetic spectrum? How can electromagnetic waves be used?

Name Class Date. What two models do scientists use to describe light? What is the electromagnetic spectrum? How can electromagnetic waves be used? CHAPTER 16 12 SECTION Sound and Light The Nature of Light KEY IDEAS As you read this section, keep these questions in mind: What two models do scientists use to describe light? What is the electromagnetic

More information

Lecture 2 Global and Zonal-mean Energy Balance

Lecture 2 Global and Zonal-mean Energy Balance Lecture 2 Global and Zonal-mean Energy Balance A zero-dimensional view of the planet s energy balance RADIATIVE BALANCE Roughly 70% of the radiation received from the Sun at the top of Earth s atmosphere

More information

Midterm Review #3-2018

Midterm Review #3-2018 1. The reaction below represents an energy-producing process. The reaction represents how energy is produced A) when water condenses in Earth's atmosphere B) during nuclear decay C) from the movement of

More information

Global Climate Change

Global Climate Change Global Climate Change Definition of Climate According to Webster dictionary Climate: the average condition of the weather at a place over a period of years exhibited by temperature, wind velocity, and

More information

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

L 18 Thermodynamics [3] Heat flow. Conduction. Convection. Thermal Conductivity. heat conduction. Heat transfer L 18 Thermodynamics [3] Heat transfer convection conduction emitters of seeing behind closed doors Greenhouse effect Heat Capacity How to boil water Heat flow HEAT the energy that flows from one system

More information

Energy: Warming the earth and Atmosphere. air temperature. Overview of the Earth s Atmosphere 9/10/2012. Composition. Chapter 3.

Energy: Warming the earth and Atmosphere. air temperature. Overview of the Earth s Atmosphere 9/10/2012. Composition. Chapter 3. Overview of the Earth s Atmosphere Composition 99% of the atmosphere is within 30km of the Earth s surface. N 2 78% and O 2 21% The percentages represent a constant amount of gas but cycles of destruction

More information

RADIATION and the EM Spectrum

RADIATION and the EM Spectrum RADIATION and the EM Spectrum Radioactivity is the of high-energy particles and/or of energy from a substance as a result of of its atoms. There are several types of radiation. Radiation from the sun is

More information

Lecture # 04 January 27, 2010, Wednesday Energy & Radiation

Lecture # 04 January 27, 2010, Wednesday Energy & Radiation Lecture # 04 January 27, 2010, Wednesday Energy & Radiation Kinds of energy Energy transfer mechanisms Radiation: electromagnetic spectrum, properties & principles Solar constant Atmospheric influence

More information

1 A 3 C 2 B 4 D. 5. During which month does the minimum duration of insolation occur in New York State? 1 February 3 September 2 July 4 December

1 A 3 C 2 B 4 D. 5. During which month does the minimum duration of insolation occur in New York State? 1 February 3 September 2 July 4 December INSOLATION REVIEW 1. The map below shows isolines of average daily insolation received in calories per square centimeter per minute at the Earth s surface. If identical solar collectors are placed at the

More information

Lecture 2: Global Energy Cycle

Lecture 2: Global Energy Cycle Lecture 2: Global Energy Cycle Planetary energy balance Greenhouse Effect Vertical energy balance Solar Flux and Flux Density Solar Luminosity (L) the constant flux of energy put out by the sun L = 3.9

More information

Planetary Science: Investigations 9-10 I-Check Quiz STUDY GUIDE- ANSWER KEY Name HR Date

Planetary Science: Investigations 9-10 I-Check Quiz STUDY GUIDE- ANSWER KEY Name HR Date 1. How are different types of radiation arranged along the electromagnetic spectrum? A. By how fast they travel incorrect answer B. By their sources incorrect answer C. By the amount of energy they carry

More information

Atoms and Radiation electromagnetic radiation Radiation electromagnetic

Atoms and Radiation electromagnetic radiation Radiation electromagnetic Atoms and Radiation The information about astronomical objects (planets, stars, galaxies) can be obtained by studying the electromagnetic radiation emitted by those objects. Astronomers use the laws of

More information

Greenhouse Effect. Julia Porter, Celia Hallan, Andrew Vrabel Miles, Gary DeFrance, and Amber Rose

Greenhouse Effect. Julia Porter, Celia Hallan, Andrew Vrabel Miles, Gary DeFrance, and Amber Rose Greenhouse Effect Julia Porter, Celia Hallan, Andrew Vrabel Miles, Gary DeFrance, and Amber Rose What is the Greenhouse Effect? The greenhouse effect is a natural occurrence caused by Earth's atmosphere

More information

Introduction to Photovoltaics

Introduction to Photovoltaics INTRODUCTION Objectives Understand the photovoltaic effect. Understand the properties of light. Describe frequency and wavelength. Understand the factors that determine available light energy. Use software

More information

Chapter 3. Multiple Choice Questions

Chapter 3. Multiple Choice Questions Chapter 3 Multiple Choice Questions 1. In the case of electromagnetic energy, an object that is hot: a. radiates much more energy than a cool object b. radiates much less energy than a cool object c. radiates

More information

ATMOSPHERE PACKET CHAPTER 22 PAGES Section 1 page 546

ATMOSPHERE PACKET CHAPTER 22 PAGES Section 1 page 546 Name: Period: ATMOSPHERE PACKET CHAPTER 22 PAGES 546-564 Section 1 page 546 1. Identify five main components of the atmosphere 2. Explain the cause of atmospheric pressure. 3. Why is atmospheric pressure

More information

Central Coast Climate Science Education Dr. Ray Weymann

Central Coast Climate Science Education Dr. Ray Weymann Central Coast Climate Science Education Dr. Ray Weymann ray.climate@charter.net Lesson 3: The Greenhouse Effect Last edit: December 7, 2012 The greenhouse effect is an observed and well-understood fact,

More information

9/12/2011. Training Course Remote Sensing - Basic Theory & Image Processing Methods September 2011

9/12/2011. Training Course Remote Sensing - Basic Theory & Image Processing Methods September 2011 Training Course Remote Sensing - Basic Theory & Image Processing Methods 19 23 September 2011 Introduction to Remote Sensing Michiel Damen (September 2011) damen@itc.nl 1 Overview Electro Magnetic (EM)

More information

Chapter 3- Energy Balance and Temperature

Chapter 3- Energy Balance and Temperature Chapter 3- Energy Balance and Temperature Understanding Weather and Climate Aguado and Burt Influences on Insolation Absorption Reflection/Scattering Transmission 1 Absorption An absorber gains energy

More information

The Nature of Light. We have a dual model

The Nature of Light. We have a dual model Light and Atoms Properties of Light We can come to understand the composition of distant bodies by analyzing the light they emit This analysis can tell us about the composition as well as the temperature

More information

Mr. Lanik Practice Test Name:

Mr. Lanik Practice Test Name: Mr. Lanik Practice Test Name: 1. New York State s Catskills are classified as which type of landscape region? mountain plateau Adirondacks Catskills lowland plain 2. In which New York State landscape region

More information

2/22/ Atmospheric Characteristics

2/22/ Atmospheric Characteristics 17.1 Atmospheric Characteristics Atmosphere: the gaseous layer that surrounds the Earth I. In the past, gases came from volcanic eruptions A. Water vapor was a major component of outgassing B. Other gases

More information

Chapter 4 - Light. Name: Block:

Chapter 4 - Light. Name: Block: Chapter 4 Notes: Light Name: Block: Properties of Waves Waves are a repeating disturbance or movement that energy through matter or space without causing any displacement of material Features of a wave:

More information

Energy and Radiation. GEOG/ENST 2331 Lecture 3 Ahrens: Chapter 2

Energy and Radiation. GEOG/ENST 2331 Lecture 3 Ahrens: Chapter 2 Energy and Radiation GEOG/ENST 2331 Lecture 3 Ahrens: Chapter 2 Last lecture: the Atmosphere! Mainly nitrogen (78%) and oxygen (21%)! T, P and ρ! The Ideal Gas Law! Temperature profiles Lecture outline!

More information

- matter-energy interactions. - global radiation balance. Further Reading: Chapter 04 of the text book. Outline. - shortwave radiation balance

- matter-energy interactions. - global radiation balance. Further Reading: Chapter 04 of the text book. Outline. - shortwave radiation balance (1 of 12) Further Reading: Chapter 04 of the text book Outline - matter-energy interactions - shortwave radiation balance - longwave radiation balance - global radiation balance (2 of 12) Previously, we

More information

Period 13: Earth as an Energy System

Period 13: Earth as an Energy System Name Section Period 13: Earth as an Energy System 13.1 The Earth-Sun System 1) Energy from the sun Observe the models of the Earth, Moon, and Sun in the room. a) Imagine that the distance between the Earth

More information

3. Which color of the visible light has the shortest wavelength? A) violet B) green C) yellow D) red

3. Which color of the visible light has the shortest wavelength? A) violet B) green C) yellow D) red Name: Topic 6 Test 1. Which process is responsible for the greatest loss of energy from Earth's surface into space on a clear night? A) condensation B) conduction C) radiation D) convection 2. Base your

More information

Exercises Conduction (pages ) 1. Define conduction. 2. What is a conductor?

Exercises Conduction (pages ) 1. Define conduction. 2. What is a conductor? Exercises 22.1 Conduction (pages 431 432) 1. Define conduction. 2. What is a conductor? 3. are the best conductors. 4. In conduction, between particles transfer thermal energy. 5. Is the following sentence

More information

Wednesday, September 8, 2010 Infrared Trapping the Greenhouse Effect

Wednesday, September 8, 2010 Infrared Trapping the Greenhouse Effect Wednesday, September 8, 2010 Infrared Trapping the Greenhouse Effect Goals to look at the properties of materials that make them interact with thermal (i.e., infrared, or IR) radiation (absorbing and reemitting

More information

2. What does a mercury barometer measure? Describe this device and explain how it physically works.

2. What does a mercury barometer measure? Describe this device and explain how it physically works. Written Homework #1 Key NATS 101, Sec. 13 Fall 2010 40 Points total 10 points per graded question 10 points for attempting all questions. 1. What is the difference between mass and weight? Mass is an intrinsic

More information

Heat can be transferred by. and by radiation Conduction

Heat can be transferred by. and by radiation Conduction Heat can be transferred by conduction, by convection, and by radiation. The spontaneous transfer of heat is always from warmer objects to cooler objects. If several objects near one another have different

More information

SPECTRUM. Dispersion. This phenomenon can be observed in a lab environment using a

SPECTRUM. Dispersion. This phenomenon can be observed in a lab environment using a SPECTRUM Dispersion The phenomenon due to which a polychromatic light, like sunlight, splits into its component colours, when passed through a transparent medium like a glass prism, is called dispersion

More information

Ch22&23 Test. Multiple Choice Identify the choice that best completes the statement or answers the question.

Ch22&23 Test. Multiple Choice Identify the choice that best completes the statement or answers the question. Ch22&23 Test Multiple Choice Identify the choice that best completes the statement or answers the question. 1. The two most abundant compounds in the atmosphere are carbon dioxide and a. particulates.

More information

The Atmosphere. Composition of the Atmosphere. Section 2

The Atmosphere. Composition of the Atmosphere. Section 2 The Atmosphere Earth is surrounded by a mixture of gases known as the Nitrogen, oxygen, carbon dioxide, and other gases are all parts of this mixture. Earth s atmosphere changes constantly as these gases

More information

Troposphere and mesosphere Stratosphere and thermosphere radio

Troposphere and mesosphere Stratosphere and thermosphere radio Warm-up Page: 518, 1. What two layers of the atmosphere is temperature decreasing? Troposphere and mesosphere Page: 518, 2. What two layers of the atmsophere is temperature increasing? Stratosphere and

More information

RR#3- Multiple Choice

RR#3- Multiple Choice 1. Which type of land surface will most likely absorb the greatest amount of incoming solar radiation? 1) rough, dark-colored surface 2) rough, light-colored surface 3) smooth, dark-colored surface 4)

More information

10/31/2017. Calculating the temperature of earth (The greenhouse effect) IR radiation. The electromagnetic spectrum

10/31/2017. Calculating the temperature of earth (The greenhouse effect)   IR radiation. The electromagnetic spectrum Calculating the temperature of earth (The greenhouse effect) EM radiation so far Spectrum of EM radiation emitted by many objects may be approximated by the blackbody spectrum Blackbody spectrum (plot

More information

Let s Think for a Second

Let s Think for a Second Weather and Climate Let s Think for a Second Why is weather important in Ohio? Is climate important in Ohio? Spend 2 minutes sharing your thoughts with 1 partner. First, Let s Watch This. http://video.nationalgeographic.com/video/science/earthsci/climate-weather-sci/

More information

COMPOSITION OF THE ATMOSPHERE

COMPOSITION OF THE ATMOSPHERE Skills Worksheet Directed Reading Section: Characteristics of the Atmosphere 1. Define atmosphere. 2. Describe two important functions served by Earth s atmosphere. COMPOSITION OF THE ATMOSPHERE 3. The

More information

Lecture 2: Global Energy Cycle

Lecture 2: Global Energy Cycle Lecture 2: Global Energy Cycle Planetary energy balance Greenhouse Effect Selective absorption Vertical energy balance Solar Flux and Flux Density Solar Luminosity (L) the constant flux of energy put out

More information

Solar Flux and Flux Density. Lecture 2: Global Energy Cycle. Solar Energy Incident On the Earth. Solar Flux Density Reaching Earth

Solar Flux and Flux Density. Lecture 2: Global Energy Cycle. Solar Energy Incident On the Earth. Solar Flux Density Reaching Earth Lecture 2: Global Energy Cycle Solar Flux and Flux Density Planetary energy balance Greenhouse Effect Selective absorption Vertical energy balance Solar Luminosity (L) the constant flux of energy put out

More information

Earth: the Goldilocks Planet

Earth: the Goldilocks Planet Earth: the Goldilocks Planet Not too hot (460 C) Fig. 3-1 Not too cold (-55 C) Wave properties: Wavelength, velocity, and? Fig. 3-2 Reviewing units: Wavelength = distance (meters or nanometers, etc.) Velocity

More information

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? About 10 km thick

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? About 10 km thick Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds What is an atmosphere? Sources of Gas Losses of Gas Thermal Escape Earth s Atmosphere About 10 km thick Consists mostly of molecular

More information

PHYSICS 231 INTRODUCTORY PHYSICS I

PHYSICS 231 INTRODUCTORY PHYSICS I PHYSICS 231 INTRODUCTORY PHYSICS I Lecture 17 Heat: Q = Energy transferred due to microscopic contact Recap - Heat Transfer Heat can: Change temperature Q = mc!t c = specific heat For water: c= 1.0 cal/(g

More information

General Comments about the Atmospheres of Terrestrial Planets

General Comments about the Atmospheres of Terrestrial Planets General Comments about the Atmospheres of Terrestrial Planets Mercury Very little atmosphere Contents: vaporized micrometeorites, solar wind Sky is black Venus Very thick (10% density of water), dense

More information

Radiation and the atmosphere

Radiation and the atmosphere Radiation and the atmosphere Of great importance is the difference between how the atmosphere transmits, absorbs, and scatters solar and terrestrial radiation streams. The most important statement that

More information

Outline. Planetary Atmospheres. General Comments about the Atmospheres of Terrestrial Planets. General Comments, continued

Outline. Planetary Atmospheres. General Comments about the Atmospheres of Terrestrial Planets. General Comments, continued Outline Planetary Atmospheres Chapter 10 General comments about terrestrial planet atmospheres Atmospheric structure & the generic atmosphere Greenhouse effect Magnetosphere & the aurora Weather & climate

More information

Chapter 2--Warming the Earth and the Atmosphere

Chapter 2--Warming the Earth and the Atmosphere Chapter 2--Warming the Earth and the Atmosphere Student: 1. Which of the following provides a measure of the average speed of air molecules? A. pressure B. temperature C. density D. heat 2. A change of

More information

Light The EM Spectrum

Light The EM Spectrum Light The EM Spectrum 1 Spectrum of Electromagnetic Radiation Region Wavelength (Angstroms) Wavelength (centimeters) Frequency (Hz) Energy (ev) Radio > 10 9 > 10 < 3 x 10 9 < 10-5 Microwave 10 9-10 6 10-0.01

More information

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

Chapter 5: Light and Matter: Reading Messages from the Cosmos Chapter 5 Lecture Chapter 5: Light and Matter: Reading Messages from the Cosmos Light and Matter: Reading Messages from the Cosmos 5.1 Light in Everyday Life Our goals for learning: How do we experience

More information

3. The very long ones are called waves, and the very short ones are called waves.

3. The very long ones are called waves, and the very short ones are called waves. NASA Mission: Science Introduction to the Electromagnetic Spectrum Web Quest Directions: Load the following website which will discuss the electromagnetic spectrum in detail. http://missionscience.nasa.gov/ems/01_intro.html

More information

G109 Alternate Midterm Exam October, 2004 Instructor: Dr C.M. Brown

G109 Alternate Midterm Exam October, 2004 Instructor: Dr C.M. Brown 1 Time allowed 50 mins. Answer ALL questions Total possible points;50 Number of pages:8 Part A: Multiple Choice (1 point each) [total 24] Answer all Questions by marking the corresponding number on the

More information

FOLLOW THE ENERGY! EARTH S DYNAMIC CLIMATE SYSTEM

FOLLOW THE ENERGY! EARTH S DYNAMIC CLIMATE SYSTEM Investigation 1B FOLLOW THE ENERGY! EARTH S DYNAMIC CLIMATE SYSTEM Driving Question How does energy enter, flow through, and exit Earth s climate system? Educational Outcomes To consider Earth s climate

More information

The order of the atmosphere layers. Unique characteristics of each layer. What do the temperatures do in each layer? Why is the temperature of the

The order of the atmosphere layers. Unique characteristics of each layer. What do the temperatures do in each layer? Why is the temperature of the Atmosphere Review Atmosphere Unit Review Plan Layers of Atmosphere Composition of Atmosphere Characteristics of Layers and Atmosphere Heat Transfer Global winds Importance of Atmosphere The order of the

More information