Greenhouse Effect and the Global Energy Balance

Size: px
Start display at page:

Download "Greenhouse Effect and the Global Energy Balance"

Transcription

1 Greenhouse Effect and the Global Energy Balance

2 Energy transmission ( a a refresher) There are three modes of energy transmission to consider. Conduction: the transfer of energy in a substance by means of molecular excitation without any net external motion. Convection: the transfer of energy by mass motions within a fluid or gas, resulting in actual transport of energy. Radiation: the propagation of electromagnetic waves through space.

3

4 Convection

5 ELECTROMAGNETIC RADIATION how the earth receives the sun s energy

6

7 Blackbodies if an object has a temperature greater than 0K, it has a blackbody curve Temperature tells us 1. How much energy the body emits 2. At what wavelength of radiation most of the energy is emitted E = σt 4 λ max = 2897/T Sun s blackbody curve Blackbody curve for the sun

8 Balancing Act ABSORPTION, EMISSION, and EQUILIBRIUM the idea of a blackbody The earth absorbs all incident radiation and reemits at longwave radiation (thermal) Wien's Law -- curves the wavelength of energy emitted the most

9 Balancing Act ABSORPTION, EMISSION, and EQUILIBRIUM the idea of a blackbody The earth absorbs all incident radiation and reemits at longwave radiation (thermal) This occurs at equal rates (think day and night) As such, earth is said to be at radiative equilibrium temperature 255K (-18C, 0F) Earth s observed average surface temperature is actually 288K (15C, 59F)! WHY? Lets track the incoming radiation

10 The atmosphere selectively absorbs and emits radiation

11 Atmospheric composition PERMANENT GASES

12 VARIABLE GASES Atmospheric composition

13 A blackbody without an atmosphere All incoming (incident) radiation is absorbed an equilibrium temperature is reached and equally, outgoing energy is emitted at a different wavelength

14 A blackbody with an atmosphere. Note the increased average surface temperature which gases are responsible?

15 Atmospheric composition VARIABLE GASES and GREENHOUSE GASES

16 Recall incident radiation, as it passes through the atmosphere, is both reflected and absorbed

17 Of the solar radiation absorbed by the surface and the atmosphere, there exists a net gain Absorbed by greenhouse gases NET GAIN Because the earth radiates day and night

18 We can observe that modes of energy transfer play a role in the warming of the atmosphere Earth s surface receives 147 units from the sun and the atmosphere Earth s surface radiates 117 units net gain = 30 units The atmosphere receives 130 units 19 units from the sun and 111 units from the earth The atmosphere loses 160 units net loss = 30 units That loss is the gain, i.e., the warming of the atmosphere 30 units = 7 units (conduction, convection) + 23 units (latent heat)

19 THE ATMOSPHERIC GREENHOUSE EFFECT How the atmosphere absorbs energy from the sun and the earth The y-axis is the percent of radiation absorbed by the atmosphere The x-axis is the wavelength of radiation absorbed short to long wave Other contributions

20 THE ATMOSPHERIC GREENHOUSE EFFECT How the atmosphere absorbs energy from the sun and the earth If you add those individual contributions together you get

21 THE ATMOSPHERIC GREENHOUSE EFFECT How the atmosphere absorbs energy from the sun and the earth SUN s ENERGY EARTH S ENERGY

22 THE ATMOSPHERIC GREENHOUSE EFFECT So, let s review, sequence of steps: 1. Solar radiation absorbed by earth s surface. 2. Earth gives off infrared radiation. 3. Greenhouse gases absorb some of the Earth s infrared radiation. 4. Greenhouse gases (water and CO 2 ) give off infrared radiation in all directions. 5. Earth absorbs downward directed infrared radiation Result: warmer surface temperature

23 Putting it together Activity: Drawing the Earth s energy balance

24 Remember incident radiation, as it passes through the atmosphere, is both reflected and absorbed Let s examine the reflected part

25 Taking a closer look at incoming solar radiation Each beam of incoming sunlight can be either: Reflected back to space: ALBEDO Clouds Atmosphere Surface Or absorbed; either by atmosphere (e.g. clouds or ozone) or Earth s surface. Activity time

26

CHAPTER 2 Energy and Earth

CHAPTER 2 Energy and Earth CHAPTER 2 Energy and Earth This chapter is concerned with the nature of energy and how it interacts with Earth. At this stage we are looking at energy in an abstract form though relate it to how it affect

More information

ESCI 107/109 The Atmosphere Lesson 2 Solar and Terrestrial Radiation

ESCI 107/109 The Atmosphere Lesson 2 Solar and Terrestrial Radiation ESCI 107/109 The Atmosphere Lesson 2 Solar and Terrestrial Radiation Reading: Meteorology Today, Chapters 2 and 3 EARTH-SUN GEOMETRY The Earth has an elliptical orbit around the sun The average Earth-Sun

More information

Energy Pathways in Earth s Atmosphere

Energy Pathways in Earth s Atmosphere BRSP - 10 Page 1 Solar radiation reaching Earth s atmosphere includes a wide spectrum of wavelengths. In addition to visible light there is radiation of higher energy and shorter wavelength called ultraviolet

More information

ATM S 111, Global Warming: Understanding the Forecast

ATM S 111, Global Warming: Understanding the Forecast ATM S 111, Global Warming: Understanding the Forecast DARGAN M. W. FRIERSON DEPARTMENT OF ATMOSPHERIC SCIENCES DAY 1: OCTOBER 1, 2015 Outline How exactly the Sun heats the Earth How strong? Important concept

More information

Solar Flux and Flux Density. Lecture 3: Global Energy Cycle. Solar Energy Incident On the Earth. Solar Flux Density Reaching Earth

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

More information

Cloud Radiation and the Law of Attraction

Cloud Radiation and the Law of Attraction Convec,on, cloud and radia,on Convection redistributes the thermal energy yielding (globally-averaged), a mean lapse rate of ~ -6.5 o C/km. Radiative processes tend to produce a more negative temperature

More information

The Earth s Atmosphere

The Earth s Atmosphere THE SUN-EARTH SYSTEM III The Earth s Atmosphere Composition and Distribution of the Atmosphere The composition of the atmosphere and the way its gases interact with electromagnetic radiation determine

More information

Chapter 2: Solar Radiation and Seasons

Chapter 2: Solar Radiation and Seasons Chapter 2: Solar Radiation and Seasons Spectrum of Radiation Intensity and Peak Wavelength of Radiation Solar (shortwave) Radiation Terrestrial (longwave) Radiations How to Change Air Temperature? Add

More information

Take away concepts. What is Energy? Solar Energy. EM Radiation. Properties of waves. Solar Radiation Emission and Absorption

Take away concepts. What is Energy? Solar Energy. EM Radiation. Properties of waves. Solar Radiation Emission and Absorption Take away concepts Solar Radiation Emission and Absorption 1. 2. 3. 4. 5. 6. Conservation of energy. Black body radiation principle Emission wavelength and temperature (Wein s Law). Radiation vs. distance

More information

Solar Energy. Outline. Solar radiation. What is light?-- Electromagnetic Radiation. Light - Electromagnetic wave spectrum. Electromagnetic Radiation

Solar Energy. Outline. Solar radiation. What is light?-- Electromagnetic Radiation. Light - Electromagnetic wave spectrum. Electromagnetic Radiation Outline MAE 493R/593V- Renewable Energy Devices Solar Energy Electromagnetic wave Solar spectrum Solar global radiation Solar thermal energy Solar thermal collectors Solar thermal power plants Photovoltaics

More information

Teaching Time: One-to-two 50-minute periods

Teaching Time: One-to-two 50-minute periods Lesson Summary Students create a planet using a computer game and change features of the planet to increase or decrease the planet s temperature. Students will explore some of the same principles scientists

More information

TOPIC 5 (cont.) RADIATION LAWS - Part 2

TOPIC 5 (cont.) RADIATION LAWS - Part 2 TOPIC 5 (cont.) RADIATION LAWS - Part 2 Quick review ELECTROMAGNETIC SPECTRUM Our focus in this class is on: UV VIS lr = micrometers (aka microns) = nanometers (also commonly used) Q1. The first thing

More information

a) species of plants that require a relatively cool, moist environment tend to grow on poleward-facing slopes.

a) species of plants that require a relatively cool, moist environment tend to grow on poleward-facing slopes. J.D. McAlpine ATMS 611 HMWK #8 a) species of plants that require a relatively cool, moist environment tend to grow on poleward-facing slopes. These sides of the slopes will tend to have less average solar

More information

Corso di Fisica Te T cnica Ambientale Solar Radiation

Corso di Fisica Te T cnica Ambientale Solar Radiation Solar Radiation Solar radiation i The Sun The Sun is the primary natural energy source for our planet. It has a diameter D = 1.39x10 6 km and a mass M = 1.989x10 30 kg and it is constituted by 1/3 of He

More information

Seasonal & Daily Temperatures. Seasons & Sun's Distance. Solstice & Equinox. Seasons & Solar Intensity

Seasonal & Daily Temperatures. Seasons & Sun's Distance. Solstice & Equinox. Seasons & Solar Intensity Seasonal & Daily Temperatures Seasons & Sun's Distance The role of Earth's tilt, revolution, & rotation in causing spatial, seasonal, & daily temperature variations Please read Chapter 3 in Ahrens Figure

More information

CHAPTER 3 Heat and energy in the atmosphere

CHAPTER 3 Heat and energy in the atmosphere CHAPTER 3 Heat and energy in the atmosphere In Chapter 2 we examined the nature of energy and its interactions with Earth. Here we concentrate initially on the way in which energy interacts with the atmosphere

More information

Clouds and the Energy Cycle

Clouds and the Energy Cycle August 1999 NF-207 The Earth Science Enterprise Series These articles discuss Earth's many dynamic processes and their interactions Clouds and the Energy Cycle he study of clouds, where they occur, and

More information

Electromagnetic Radiation Energy that comes to us from the sun is transported in the form of waves known as electromagnetic energy.

Electromagnetic Radiation Energy that comes to us from the sun is transported in the form of waves known as electromagnetic energy. Electromagnetic Radiation Energy that comes to us from the sun is transported in the form of waves known as electromagnetic energy. This combines electricity and magnetism such that setting up an electric

More information

Treasure Hunt. Lecture 2 How does Light Interact with the Environment? EMR Principles and Properties. EMR and Remote Sensing

Treasure Hunt. Lecture 2 How does Light Interact with the Environment? EMR Principles and Properties. EMR and Remote Sensing Lecture 2 How does Light Interact with the Environment? Treasure Hunt Find and scan all 11 QR codes Choose one to watch / read in detail Post the key points as a reaction to http://www.scoop.it/t/env202-502-w2

More information

Materials Needed: Choose one of the following methods depending on how familiar your students are with the internet and how to use it.

Materials Needed: Choose one of the following methods depending on how familiar your students are with the internet and how to use it. Teacher Information Lesson Title: Global Warming, Green House Effect and Climate Changes Lesson Description: This lesson helps students to understand or review their understanding of global warming, the

More information

Fundamentals of Climate Change (PCC 587): Water Vapor

Fundamentals of Climate Change (PCC 587): Water Vapor Fundamentals of Climate Change (PCC 587): Water Vapor DARGAN M. W. FRIERSON UNIVERSITY OF WASHINGTON, DEPARTMENT OF ATMOSPHERIC SCIENCES DAY 2: 9/30/13 Water Water is a remarkable molecule Water vapor

More information

Chapter 2. The global energy balance. 2.1 Planetary emission temperature

Chapter 2. The global energy balance. 2.1 Planetary emission temperature Chapter 2 The global energy balance We consider now the general problem of the radiative equilibrium temperature of the Earth. The Earth is bathed in solar radiation and absorbs much of that incident upon

More information

Review 1. Multiple Choice Identify the choice that best completes the statement or answers the question.

Review 1. Multiple Choice Identify the choice that best completes the statement or answers the question. Review 1 Multiple Choice Identify the choice that best completes the statement or answers the question. 1. When hydrogen nuclei fuse into helium nuclei a. the nuclei die. c. particles collide. b. energy

More information

Greenhouse Glazing Effects on Heat Transfer for Winter Heating and Summer Cooling

Greenhouse Glazing Effects on Heat Transfer for Winter Heating and Summer Cooling Greenhouse Glazing Effects on Heat Transfer for Winter Heating and Summer Cooling David R. Mears, Ph.D. Bioresource Engineering Department of Plant Biology and Pathology Rutgers University 20 Ag Extension

More information

Module 2.2. Heat transfer mechanisms

Module 2.2. Heat transfer mechanisms Module 2.2 Heat transfer mechanisms Learning Outcomes On successful completion of this module learners will be able to - Describe the 1 st and 2 nd laws of thermodynamics. - Describe heat transfer mechanisms.

More information

Electromagnetic Radiation (EMR) and Remote Sensing

Electromagnetic Radiation (EMR) and Remote Sensing Electromagnetic Radiation (EMR) and Remote Sensing 1 Atmosphere Anything missing in between? Electromagnetic Radiation (EMR) is radiated by atomic particles at the source (the Sun), propagates through

More information

Radiation Transfer in Environmental Science

Radiation Transfer in Environmental Science Radiation Transfer in Environmental Science with emphasis on aquatic and vegetation canopy media Autumn 2008 Prof. Emmanuel Boss, Dr. Eyal Rotenberg Introduction Radiation in Environmental sciences Most

More information

Copyrighted Material. 1 Basics of Climate. The climate s delicate, the air most sweet. William Shakespeare, A Winter s Tale

Copyrighted Material. 1 Basics of Climate. The climate s delicate, the air most sweet. William Shakespeare, A Winter s Tale 1 Basics of Climate The climate s delicate, the air most sweet. William Shakespeare, A Winter s Tale To appreciate the role of the ocean in climate, we need to have a basic understanding of how the climate

More information

How does snow melt? Principles of snow melt. Energy balance. GEO4430 snow hydrology 21.03.2006. Energy flux onto a unit surface:

How does snow melt? Principles of snow melt. Energy balance. GEO4430 snow hydrology 21.03.2006. Energy flux onto a unit surface: Principles of snow melt How does snow melt? We need energy to melt snow/ ice. GEO443 snow hydrology 21.3.26 E = m L h we s K = ρ h = w w we f E ρ L L f f Thomas V. Schuler t.v.schuler@geo.uio.no E energy

More information

From lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation?

From lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation? From lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation? From lowest energy to highest energy, which of the following correctly

More information

PTYS/ASTR 206 Section 2 Spring 2007 Homework #2 (Page 1/5) NAME: KEY

PTYS/ASTR 206 Section 2 Spring 2007 Homework #2 (Page 1/5) NAME: KEY PTYS/ASTR 206 Section 2 Spring 2007 Homework #2 (Page 1/5) NAME: KEY Due Date: start of class 2/6/2007 5 pts extra credit if turned in before 9:00AM (early!) (To get the extra credit, the assignment must

More information

Introduction to the Greenhouse Effect

Introduction to the Greenhouse Effect Introduction to the Greenhouse Effect Planetary Temperature by Arthur Glasfeld and Margret Geselbracht ver the past 10-15 years there has been growing concern over changes in the climate and the possibility

More information

Overview. What is EMR? Electromagnetic Radiation (EMR) LA502 Special Studies Remote Sensing

Overview. What is EMR? Electromagnetic Radiation (EMR) LA502 Special Studies Remote Sensing LA502 Special Studies Remote Sensing Electromagnetic Radiation (EMR) Dr. Ragab Khalil Department of Landscape Architecture Faculty of Environmental Design King AbdulAziz University Room 103 Overview What

More information

1. At which temperature would a source radiate the least amount of electromagnetic energy? 1) 273 K 3) 32 K 2) 212 K 4) 5 K

1. At which temperature would a source radiate the least amount of electromagnetic energy? 1) 273 K 3) 32 K 2) 212 K 4) 5 K 1. At which temperature would a source radiate the least amount of electromagnetic energy? 1) 273 K 3) 32 K 2) 212 K 4) 5 K 2. How does the amount of heat energy reflected by a smooth, dark-colored concrete

More information

1. Theoretical background

1. Theoretical background 1. Theoretical background We consider the energy budget at the soil surface (equation 1). Energy flux components absorbed or emitted by the soil surface are: net radiation, latent heat flux, sensible heat

More information

2 Absorbing Solar Energy

2 Absorbing Solar Energy 2 Absorbing Solar Energy 2.1 Air Mass and the Solar Spectrum Now that we have introduced the solar cell, it is time to introduce the source of the energy the sun. The sun has many properties that could

More information

ENERGY & ENVIRONMENT

ENERGY & ENVIRONMENT Greenhouse molecules, their spectra and function in the atmosphere by Jack Barrett Reprinted from ENERGY & ENVIRNMENT VLUME 16 No. 6 2005 MULTI-SCIENCE PUBLISING C. LTD. 5 Wates Way, Brentwood, Essex CM15

More information

The Ideal Gas Law. Gas Constant. Applications of the Gas law. P = ρ R T. Lecture 2: Atmospheric Thermodynamics

The Ideal Gas Law. Gas Constant. Applications of the Gas law. P = ρ R T. Lecture 2: Atmospheric Thermodynamics Lecture 2: Atmospheric Thermodynamics Ideal Gas Law (Equation of State) Hydrostatic Balance Heat and Temperature Conduction, Convection, Radiation Latent Heating Adiabatic Process Lapse Rate and Stability

More information

INSPIRE GK12 Lesson Plan. The Chemistry of Climate Change Length of Lesson

INSPIRE GK12 Lesson Plan. The Chemistry of Climate Change Length of Lesson Lesson Title The Chemistry of Climate Change Length of Lesson 180 min Created By David Wilson Subject Physical Science / Chemistry / Organic Chemistry Grade Level 8-12 State Standards 2c, 4d / 2a, 4d /

More information

Energy Transport. Focus on heat transfer. Heat Transfer Mechanisms: Conduction Radiation Convection (mass movement of fluids)

Energy Transport. Focus on heat transfer. Heat Transfer Mechanisms: Conduction Radiation Convection (mass movement of fluids) Energy Transport Focus on heat transfer Heat Transfer Mechanisms: Conduction Radiation Convection (mass movement of fluids) Conduction Conduction heat transfer occurs only when there is physical contact

More information

What Is Heat? What Is Heat?

What Is Heat? What Is Heat? What Is Heat? Paul shivered inside the wood cabin. It was cold outside, and inside the cabin it wasn t much warmer. Paul could hear the rain beating down on the roof. Every few minutes there would be a

More information

FACTS ABOUT CLIMATE CHANGE

FACTS ABOUT CLIMATE CHANGE FACTS ABOUT CLIMATE CHANGE 1. What is climate change? Climate change is a long-term shift in the climate of a specific location, region or planet. The shift is measured by changes in features associated

More information

Overview of the IR channels and their applications

Overview of the IR channels and their applications Ján Kaňák Slovak Hydrometeorological Institute Jan.kanak@shmu.sk Overview of the IR channels and their applications EUMeTrain, 14 June 2011 Ján Kaňák, SHMÚ 1 Basics in satellite Infrared image interpretation

More information

5. The Nature of Light. Does Light Travel Infinitely Fast? EMR Travels At Finite Speed. EMR: Electric & Magnetic Waves

5. The Nature of Light. Does Light Travel Infinitely Fast? EMR Travels At Finite Speed. EMR: Electric & Magnetic Waves 5. The Nature of Light Light travels in vacuum at 3.0. 10 8 m/s Light is one form of electromagnetic radiation Continuous radiation: Based on temperature Wien s Law & the Stefan-Boltzmann Law Light has

More information

Chapter 18 Temperature, Heat, and the First Law of Thermodynamics. Problems: 8, 11, 13, 17, 21, 27, 29, 37, 39, 41, 47, 51, 57

Chapter 18 Temperature, Heat, and the First Law of Thermodynamics. Problems: 8, 11, 13, 17, 21, 27, 29, 37, 39, 41, 47, 51, 57 Chapter 18 Temperature, Heat, and the First Law of Thermodynamics Problems: 8, 11, 13, 17, 21, 27, 29, 37, 39, 41, 47, 51, 57 Thermodynamics study and application of thermal energy temperature quantity

More information

The Greenhouse Effect. Lan Ma Global Warming: Problems & Solutions 17 September, 2007

The Greenhouse Effect. Lan Ma Global Warming: Problems & Solutions 17 September, 2007 The Greenhouse Effect Lan Ma Global Warming: Problems & Solutions 17 September, 2007 What to cover today: How do we calculate the Earth s surface temperature? What makes a gas a greenhouse gas and how

More information

The Surface Energy Budget

The Surface Energy Budget The Surface Energy Budget The radiation (R) budget Shortwave (solar) Radiation Longwave Radiation R SW R SW α α = surface albedo R LW εσt 4 ε = emissivity σ = Stefan-Boltzman constant T = temperature Subsurface

More information

The Atmosphere. Introduction Greenhouse Effect/Climate Change/Global Warming

The Atmosphere. Introduction Greenhouse Effect/Climate Change/Global Warming Introduction Greenhouse Effect/Climate Change/Global Warming The Atmosphere The terms Greenhouse Effect, Climate Change, and Global Warming are often used interchangeably, yet they really refer to three

More information

Blackbody radiation. Main Laws. Brightness temperature. 1. Concepts of a blackbody and thermodynamical equilibrium.

Blackbody radiation. Main Laws. Brightness temperature. 1. Concepts of a blackbody and thermodynamical equilibrium. Lecture 4 lackbody radiation. Main Laws. rightness temperature. Objectives: 1. Concepts of a blackbody, thermodynamical equilibrium, and local thermodynamical equilibrium.. Main laws: lackbody emission:

More information

Light as a Wave. The Nature of Light. EM Radiation Spectrum. EM Radiation Spectrum. Electromagnetic Radiation

Light as a Wave. The Nature of Light. EM Radiation Spectrum. EM Radiation Spectrum. Electromagnetic Radiation The Nature of Light Light and other forms of radiation carry information to us from distance astronomical objects Visible light is a subset of a huge spectrum of electromagnetic radiation Maxwell pioneered

More information

The Three Heat Transfer Modes in Reflow Soldering

The Three Heat Transfer Modes in Reflow Soldering Section 5: Reflow Oven Heat Transfer The Three Heat Transfer Modes in Reflow Soldering There are three different heating modes involved with most SMT reflow processes: conduction, convection, and infrared

More information

Observed Cloud Cover Trends and Global Climate Change. Joel Norris Scripps Institution of Oceanography

Observed Cloud Cover Trends and Global Climate Change. Joel Norris Scripps Institution of Oceanography Observed Cloud Cover Trends and Global Climate Change Joel Norris Scripps Institution of Oceanography Increasing Global Temperature from www.giss.nasa.gov Increasing Greenhouse Gases from ess.geology.ufl.edu

More information

SOLAR ENERGY How much strikes the earth? How much can my building get? When is it too much?

SOLAR ENERGY How much strikes the earth? How much can my building get? When is it too much? SOLAR ENERGY How much strikes the earth? How much can my building get? When is it too much? The sun: friend of foe? Drawing by Le Corbusier ENGS 44 Sustainable Design Benoit Cushman-Roisin 14 April 2015

More information

Principle of Thermal Imaging

Principle of Thermal Imaging Section 8 All materials, which are above 0 degrees Kelvin (-273 degrees C), emit infrared energy. The infrared energy emitted from the measured object is converted into an electrical signal by the imaging

More information

How Do Oceans Affect Weather and Climate?

How Do Oceans Affect Weather and Climate? How Do Oceans Affect Weather and Climate? In Learning Set 2, you explored how water heats up more slowly than land and also cools off more slowly than land. Weather is caused by events in the atmosphere.

More information

- thus, the total number of atoms per second that absorb a photon is

- thus, the total number of atoms per second that absorb a photon is Stimulated Emission of Radiation - stimulated emission is referring to the emission of radiation (a photon) from one quantum system at its transition frequency induced by the presence of other photons

More information

Green Heating. Pupil Research Brief. Teachers Notes. Syllabus Coverage Subject Knowledge and Understanding. Route through the Brief UPIL ESEARCHER

Green Heating. Pupil Research Brief. Teachers Notes. Syllabus Coverage Subject Knowledge and Understanding. Route through the Brief UPIL ESEARCHER R P UPIL ESEARCHER Green Heating I NITIATIVE Pupil Research Brief Teachers Notes Syllabus Coverage Subject Knowledge and Understanding all types of electromagnetic radiation form a continuous spectrum

More information

AOSC 621 Lesson 15 Radiative Heating/Cooling

AOSC 621 Lesson 15 Radiative Heating/Cooling AOSC 621 Lesson 15 Radiative Heating/Cooling Effect of radiation on clouds: fog 2 Clear-sky cooling/heating rate: longwave CO2 O3 H2O 3 Clear-sky heating rate: shortwave Standard atmosphere Heating due

More information

Name: Class: Date: 10. Some substances, when exposed to visible light, absorb more energy as heat than other substances absorb.

Name: Class: Date: 10. Some substances, when exposed to visible light, absorb more energy as heat than other substances absorb. Name: Class: Date: ID: A PS Chapter 13 Review Modified True/False Indicate whether the statement is true or false. If false, change the identified word or phrase to make the statement true. 1. In all cooling

More information

MCQ - ENERGY and CLIMATE

MCQ - ENERGY and CLIMATE 1 MCQ - ENERGY and CLIMATE 1. The volume of a given mass of water at a temperature of T 1 is V 1. The volume increases to V 2 at temperature T 2. The coefficient of volume expansion of water may be calculated

More information

What the Heck are Low-Cloud Feedbacks? Takanobu Yamaguchi Rachel R. McCrary Anna B. Harper

What the Heck are Low-Cloud Feedbacks? Takanobu Yamaguchi Rachel R. McCrary Anna B. Harper What the Heck are Low-Cloud Feedbacks? Takanobu Yamaguchi Rachel R. McCrary Anna B. Harper IPCC Cloud feedbacks remain the largest source of uncertainty. Roadmap 1. Low cloud primer 2. Radiation and low

More information

ATMOSPHERIC STRUCTURE. The vertical distribution of temperature, pressure,

ATMOSPHERIC STRUCTURE. The vertical distribution of temperature, pressure, ATMOSPHERIC STRUCTURE. The vertical distribution of temperature, pressure, density, and composition of the atmosphere constitutes atmospheric structure. These quantities also vary with season and location

More information

AZ State Standards. Concept 3: Conservation of Energy and Increase in Disorder Understand ways that energy is conserved, stored, and transferred.

AZ State Standards. Concept 3: Conservation of Energy and Increase in Disorder Understand ways that energy is conserved, stored, and transferred. Forms of Energy AZ State Standards Concept 3: Conservation of Energy and Increase in Disorder Understand ways that energy is conserved, stored, and transferred. PO 1. Describe the following ways in which

More information

Comments on How Exterior Paints and Interior Paints Can Play Roles in Conserving Energy. For Tech Traders Inc. By H. F. Poppendiek

Comments on How Exterior Paints and Interior Paints Can Play Roles in Conserving Energy. For Tech Traders Inc. By H. F. Poppendiek Comments on How Exterior Paints and Interior Paints Can Play Roles in Conserving Energy For Tech Traders Inc. By H. F. Poppendiek June 2002 GEOSCIENCE LTD 620 Marindustry Drive San Diego, California 92121

More information

Convection, Conduction & Radiation

Convection, Conduction & Radiation Convection, Conduction & Radiation There are three basic ways in which heat is transferred: convection, conduction and radiation. In gases and liquids, heat is usually transferred by convection, in which

More information

Multiple Choice Identify the choice that best completes the statement or answers the question.

Multiple Choice Identify the choice that best completes the statement or answers the question. Test 2 f14 Multiple Choice Identify the choice that best completes the statement or answers the question. 1. Carbon cycles through the Earth system. During photosynthesis, carbon is a. released from wood

More information

Climate Change and Renewable Energy A Perspective from a Measurements Viewpoint

Climate Change and Renewable Energy A Perspective from a Measurements Viewpoint Climate Change and Renewable Energy A Perspective from a Measurements Viewpoint Regional Workshop on Metrology and Technology Challenges of Climate Change and Renewable Energy Guatemala City, Guatemala

More information

Preview of Period 5: Thermal Energy, the Microscopic Picture

Preview of Period 5: Thermal Energy, the Microscopic Picture Preview of Period 5: Thermal Energy, the Microscopic Picture 5.1 Temperature and Molecular Motion What is evaporative cooling? 5.2 Temperature and Phase Changes How much energy is required for a phase

More information

Earth Sciences -- Grades 9, 10, 11, and 12. California State Science Content Standards. Mobile Climate Science Labs

Earth Sciences -- Grades 9, 10, 11, and 12. California State Science Content Standards. Mobile Climate Science Labs Earth Sciences -- Grades 9, 10, 11, and 12 California State Science Content Standards Covered in: Hands-on science labs, demonstrations, & activities. Investigation and Experimentation. Lesson Plans. Presented

More information

8.1 Radio Emission from Solar System objects

8.1 Radio Emission from Solar System objects 8.1 Radio Emission from Solar System objects 8.1.1 Moon and Terrestrial planets At visible wavelengths all the emission seen from these objects is due to light reflected from the sun. However at radio

More information

Physics 1010: The Physics of Everyday Life. TODAY Black Body Radiation, Greenhouse Effect

Physics 1010: The Physics of Everyday Life. TODAY Black Body Radiation, Greenhouse Effect Physics 1010: The Physics of Everyday Life TODAY Black Body Radiation, Greenhouse Effect 1 Admin Stuff Exams are at back of room, alphabetically in four piles. Please collect AFTER class Grades posted

More information

ESCI-61 Introduction to Photovoltaic Technology. Solar Radiation. Ridha Hamidi, Ph.D.

ESCI-61 Introduction to Photovoltaic Technology. Solar Radiation. Ridha Hamidi, Ph.D. 1 ESCI-61 Introduction to Photovoltaic Technology Solar Radiation Ridha Hamidi, Ph.D. 2 The Sun The Sun is a perpetual source of energy It has produced energy for about 4.6 billions of years, and it is

More information

CPI Links Content Guide & Five Items Resource

CPI Links Content Guide & Five Items Resource CPI Links Content Guide & Five Items Resource Introduction The following information should be used as a companion to the CPI Links. It provides clarifications concerning the content and skills contained

More information

POROUS BURNER - A New Approach to Infrared

POROUS BURNER - A New Approach to Infrared Page: 1 POROUS BURNER - A New Approach to Infrared 1. Preface There are several possibilities to produce infrared radiation in the technical sense. Regarding the source of energy you can distinguish between

More information

How To Build A Solar Energised Power Plant

How To Build A Solar Energised Power Plant Project Title Solar Energised Power Plant Project Description In recent years energy crisis has become one of the most talked about issues around the world. Especially in the developing countries, the

More information

TEACHER BACKGROUND INFORMATION THERMAL ENERGY

TEACHER BACKGROUND INFORMATION THERMAL ENERGY TEACHER BACKGROUND INFORMATION THERMAL ENERGY In general, when an object performs work on another object, it does not transfer all of its energy to that object. Some of the energy is lost as heat due to

More information

Forms of Energy. Freshman Seminar

Forms of Energy. Freshman Seminar Forms of Energy Freshman Seminar Energy Energy The ability & capacity to do work Energy can take many different forms Energy can be quantified Law of Conservation of energy In any change from one form

More information

Introduction to Chapter 27

Introduction to Chapter 27 9 Heating and Cooling Introduction to Chapter 27 What process does a hot cup of coffee undergo as it cools? How does your bedroom become warm during the winter? How does the cooling system of a car work?

More information

What is Solar Control?

What is Solar Control? A better environment inside and out. Solar, Safety and Security Window Films: Tech Bulletin Understanding Solar Performance Solar Gard solar control window films use advanced technology to benefit consumers

More information

UNIT 6a TEST REVIEW. 1. A weather instrument is shown below.

UNIT 6a TEST REVIEW. 1. A weather instrument is shown below. UNIT 6a TEST REVIEW 1. A weather instrument is shown below. Which weather variable is measured by this instrument? 1) wind speed 3) cloud cover 2) precipitation 4) air pressure 2. Which weather station

More information

Global Warming and Greenhouse Gases Reading Assignment

Global Warming and Greenhouse Gases Reading Assignment What is global warming? Global Warming and Greenhouse Gases Imagine you live in a timber shack in Alaska. It's chilly up there, so you build yourself a huge log fire and pile on all the wood you can find.

More information

Blackbody radiation derivation of Planck s radiation low

Blackbody radiation derivation of Planck s radiation low Blackbody radiation derivation of Planck s radiation low 1 Classical theories of Lorentz and Debye: Lorentz (oscillator model): Electrons and ions of matter were treated as a simple harmonic oscillators

More information

Science Standard 3 Energy and Its Effects Grade Level Expectations

Science Standard 3 Energy and Its Effects Grade Level Expectations Science Standard 3 Energy and Its Effects Grade Level Expectations Science Standard 3 Energy and Its Effects The flow of energy drives processes of change in all biological, chemical, physical, and geological

More information

CHAPTER 6 THE TERRESTRIAL PLANETS

CHAPTER 6 THE TERRESTRIAL PLANETS CHAPTER 6 THE TERRESTRIAL PLANETS MULTIPLE CHOICE 1. Which of the following is NOT one of the four stages in the development of a terrestrial planet? 2. That Earth, evidence that Earth differentiated.

More information

The Earth's Atmosphere. Layers of the Earth's Atmosphere

The Earth's Atmosphere. Layers of the Earth's Atmosphere The Earth's Atmosphere The atmosphere surrounds Earth and protects us by blocking out dangerous rays from the sun. The atmosphere is a mixture of gases that becomes thinner until it gradually reaches space.

More information

ES 106 Laboratory # 5 EARTH-SUN RELATIONS AND ATMOSPHERIC HEATING

ES 106 Laboratory # 5 EARTH-SUN RELATIONS AND ATMOSPHERIC HEATING ES 106 Laboratory # 5 EARTH-SUN RELATIONS AND ATMOSPHERIC HEATING 5-1 Introduction Weather is the state of the atmosphere at a particular place for a short period of time. The condition of the atmosphere

More information

Systems Thinking and Modeling Climate Change Amy Pallant, Hee-Sun Lee, and Sarah Pryputniewicz

Systems Thinking and Modeling Climate Change Amy Pallant, Hee-Sun Lee, and Sarah Pryputniewicz Systems Thinking and Modeling Climate Change Amy Pallant, Hee-Sun Lee, and Sarah Pryputniewicz You know the effects of the proverbial butterfly flapping its wings. But what about an automobile driver?

More information

Blackbody Radiation References INTRODUCTION

Blackbody Radiation References INTRODUCTION Blackbody Radiation References 1) R.A. Serway, R.J. Beichner: Physics for Scientists and Engineers with Modern Physics, 5 th Edition, Vol. 2, Ch.40, Saunders College Publishing (A Division of Harcourt

More information

Heat Energy FORMS OF ENERGY LESSON PLAN 2.7. Public School System Teaching Standards Covered

Heat Energy FORMS OF ENERGY LESSON PLAN 2.7. Public School System Teaching Standards Covered FORMS OF ENERGY LESSON PLAN 2.7 Heat Energy This lesson is designed for 3rd 5th grade students in a variety of school settings (public, private, STEM schools, and home schools) in the seven states served

More information

GREENHOUSE EFFECT & GLOBAL WARMING - The internet as the primary source of information

GREENHOUSE EFFECT & GLOBAL WARMING - The internet as the primary source of information GREENHOUSE EFFECT & GLOBAL WARMING - The internet as the primary source of information - The internet as a resource - Use reputable web sites Government agencies: EPA, NASA, DOE, etc Academic Institutions

More information

Tech Bulletin. Understanding Solar Performance

Tech Bulletin. Understanding Solar Performance Tech Bulletin Understanding Solar Performance Bekaert solar control window films use advanced technology to benefit consumers with quality solutions that enhance comfort and decrease energy use. By understanding

More information

7. Our Solar System. Planetary Orbits to Scale. The Eight Planetary Orbits

7. Our Solar System. Planetary Orbits to Scale. The Eight Planetary Orbits 7. Our Solar System Terrestrial & Jovian planets Seven large satellites [moons] Chemical composition of the planets Asteroids & comets The Terrestrial & Jovian Planets Four small terrestrial planets Like

More information

MAKING SENSE OF ENERGY Electromagnetic Waves

MAKING SENSE OF ENERGY Electromagnetic Waves Adapted from State of Delaware TOE Unit MAKING SENSE OF ENERGY Electromagnetic Waves GOALS: In this Part of the unit you will Learn about electromagnetic waves, how they are grouped, and how each group

More information

Chapter 10 Temperature and Heat

Chapter 10 Temperature and Heat Chapter 10 Temperature and Heat What are temperature and heat? Are they the same? What causes heat? What Is Temperature? How do we measure temperature? What are we actually measuring? Temperature and Its

More information

Name Class Date. spectrum. White is not a color, but is a combination of all colors. Black is not a color; it is the absence of all light.

Name Class Date. spectrum. White is not a color, but is a combination of all colors. Black is not a color; it is the absence of all light. Exercises 28.1 The Spectrum (pages 555 556) 1. Isaac Newton was the first person to do a systematic study of color. 2. Circle the letter of each statement that is true about Newton s study of color. a.

More information

February 17 th Video Conference Agenda

February 17 th Video Conference Agenda February 17 th Video Conference Agenda 8:30 am Video, audio and connection checks 9:00 am Brief intro by mediator, Ellen Holmes, followed by 3 to 5 minute Day in the Life of Presentations from each school.

More information

(Walter Glogowski, Chaz Shapiro & Reid Sherman) INTRODUCTION

(Walter Glogowski, Chaz Shapiro & Reid Sherman) INTRODUCTION Convection (Walter Glogowski, Chaz Shapiro & Reid Sherman) INTRODUCTION You know from common experience that when there's a difference in temperature between two places close to each other, the temperatures

More information

Science Tutorial TEK 6.9C: Energy Forms & Conversions

Science Tutorial TEK 6.9C: Energy Forms & Conversions Name: Teacher: Pd. Date: Science Tutorial TEK 6.9C: Energy Forms & Conversions TEK 6.9C: Demonstrate energy transformations such as energy in a flashlight battery changes from chemical energy to electrical

More information

Chapter 7: Greenhouse gases and particulate matter

Chapter 7: Greenhouse gases and particulate matter Additional material for Fundamentals of Sustainable Development, Niko Roorda, 2012. Chapter 7: Greenhouse gases and particulate matter Debates on the anthropogenic greenhouse effect and climate change

More information

Lesson Plan Simulating the Greenhouse Effect in a Terrarium.

Lesson Plan Simulating the Greenhouse Effect in a Terrarium. Lesson Plan Simulating the Greenhouse Effect in a Terrarium. Content Standards: 1. Matter and Energy in the Earth System Central Concepts 1.1 Identify Earth s principal sources of internal and external

More information