Chapter 04: Atmosphere and Surface Energy Balance. Energy Essentials Energy Balance in the Troposphere Energy Balance at Earth s Surface

Size: px
Start display at page:

Download "Chapter 04: Atmosphere and Surface Energy Balance. Energy Essentials Energy Balance in the Troposphere Energy Balance at Earth s Surface"

Transcription

1 Chapter 04: Atmosphere and Surface Energy Balance Energy Essentials Energy Balance in the Troposphere Energy Balance at Earth s Surface

2 Energy Essentials Energy Pathways and Principles

3 Energy Pathways and Principles Transmission: Passage of energy through atmosphere or water Atmosphere Energy Inputs: Shortwave energy in from the Sun Ultraviolet light, visible light, near-infrared wavelengths Longwave Radiation Outputs: thermal infrared radiation Atmospheric Energy Budget: Inputs + Outputs Fig. 2.8, p. 48

4 Energy Pathways and Principles Insolation Input: The single energy input driving the Earth- Atmosphere system, including all the radiation that arrives at the Earth s surface, both direct and diffuse (scattered by the atmosphere). Insolation decreases poleward from 25 latitude in both hemispheres; Equatorial and tropic latitudes high insolation ( W/m 2 ); Low-latitude desert areas has the great annual insolation ( W/m 2 ). Why? Because cloudless skies occurs so often in deserts! Fig. 4.2, p. 91

5 Energy Pathways and Principles Scattering (Diffuse Radiation): Changing direction of light s movement, without altering its wavelengths Gas molecules, dust particles, pollutants, ice, cloud droplets, water vapor, etc. Scattering represents about 7% of Earth s reflectivity, or albedo. Rayleigh Scattering: Different sizes of molecules or particles causes scattering of different wavelengths The shorter the wavelength, the grater the scattering; The longer the wavelength, the less the scattering Fig. 4.1, p. 90

6 Why sunsets and sunrises are often red? At sunsets and sunrises, lights needs to travel longer; More shorter waves from the sun get reflected and scattered; Only longer wavelengths reach you: that s RED Fig. 2.6, p. 47

7 Energy Pathways and Principles Refraction: Change in speed and direction of light (when light entering a different medium; e.g., from empty space to atmospheric gases, or from air to water; etc.) - Spoon in a cup filled with water - Rainbow (light refracted by myriad raindrops)

8 Energy Pathways and Principles Reflection: Arriving energy bounces directly back into space without being absorbed or performing any work. Albedo: The reflectivity quality, or intrinsic brightness, of a surface (light surfaces are more reflective than dark surfaces) Albedo R I Fig. 4.5, p. 93

9 Energy Pathways and Principles Cloud- albedo forcing: increase in albedo caused by clouds. Outcome: reflect insolation and cool Earth s surface Fig. 4.7, p. 95 Cloud- greenhouse forcing: clouds acts as insulation, trapping longwave radiation emitted by Earth Outcome: increase in greenhouse warming

10 Energy Principles -- Absorption Absorption: Assimilation of radiation by molecules of matter and its conversion from one form of energy to another Outcome: Energy delivered to the matter or transferred to chemical energy (e.g., photosynthesis). Once absorbed, the radiation no longer exists /fall04/atmo336/lectures/sec3/energybudget.html

11 Heat Transfer Figure 4.10 Conduction Molecule to molecule transfer (diffuses through a substance) Convection Energy transferred by movement (involves a strong vertical motion) Advection Energy transferred by movement (involves a predominantly horizontal motion) Radiation Energy traveling through air or space

12 Energy Balance in the Troposphere The Greenhouse Effect and Atmospheric Warming Clouds and Earth s Greenhouse Earth Atmosphere Radiation Balance

13 The Greenhouse Effect and Atmospheric Warming

14 Clouds and Greenhouse Forcing Figure 4.11

15 Earth Atmosphere Radiation Balance Figure 4.12

16 Energy Budget by Latitude Outcome: 1. Between the tropics, energy surpluses dominate; 2. In polar regions, energy deficits prevail; 3. Around ~36 latitude, a balance exists; 4. The imbalance of net radiation from tropic surpluses to polar deficits drives global circulation of both energy and mass: Winds, ocean currents, dynamic weather systems Figure 4.13

17 Energy Balance at Earth s s Surface Simplified Surface Energy Balance NET Radiation = +SW (insolation) SW (reflection) +LW (infrared) LW (infrared) The Net Radiation (R) depends on the local surface conditions (e.g., a park, a front yard, or a place on campus)--

18 Energy Balance at Earth s s Surface Daily Radiation Patterns Figure 4.14 The daily temperature lag The annual temperature lags: similar to daily lags In N. Hemisphere, Jan. is the coldest after December Solstice

19 Simplified Surface Energy Balance NET R = SW (insolation( insolation) SW (reflection) +LW (infrared) LW (infrared) Not a perfect balance at zero, but for a longer time, the earth s surface balances the incoming and outgoing energy

20 Global NET R Figure 4.17 Global and local net budgets are important for managing the solar energy collection and concentration

21 Energy Balance at Earth s s Surface The Urban Environment Trees and grass land are important for Urban environments The central park in NY City has daytime temperature 5-10 C cooler than outside the park

22 The Urban Environment Figure 4.21

23 End of Chapter 4 1. Energy Essentials: Transmission; Energy Inputs; Radiation Outputs; Diffuse Radiation (Scattering); Refraction; Reflection; Albedo; Cloud- albedo forcing; Cloud- greenhouse forcing; Absorption; Heat Transfer. 2. Energy Balance in the Troposphere: The Greenhouse Effect; Earth Atmosphere Radiation Balance; Energy Budget by Latitude and outcome. Daily Radiation Patterns; Simplified Surface Energy Balance (Net( Radiation); The daily temperature lag; The annual temperature lags; The urban environment (heat island) 3. Energy Balance at Earth s Surface: Daily Radiation

24 End of Chapter 4 Robert W. Christopherson Charles E. Thomsen

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

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

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

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

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

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 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

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

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

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

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

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

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

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

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

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

California Standards Grades 9 12 Boardworks 2009 Science Contents Standards Mapping

California Standards Grades 9 12 Boardworks 2009 Science Contents Standards Mapping California Standards Grades 912 Boardworks 2009 Science Contents Standards Mapping Earth Sciences Earth s Place in the Universe 1. Astronomy and planetary exploration reveal the solar system s structure,

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

CHAPTER 5 Lectures 10 & 11 Air Temperature and Air Temperature Cycles

CHAPTER 5 Lectures 10 & 11 Air Temperature and Air Temperature Cycles CHAPTER 5 Lectures 10 & 11 Air Temperature and Air Temperature Cycles I. Air Temperature: Five important factors influence air temperature: A. Insolation B. Latitude C. Surface types D. Coastal vs. interior

More information

RADIATION IN THE TROPICAL ATMOSPHERE and the SAHEL SURFACE HEAT BALANCE. Peter J. Lamb. Cooperative Institute for Mesoscale Meteorological Studies

RADIATION IN THE TROPICAL ATMOSPHERE and the SAHEL SURFACE HEAT BALANCE. Peter J. Lamb. Cooperative Institute for Mesoscale Meteorological Studies RADIATION IN THE TROPICAL ATMOSPHERE and the SAHEL SURFACE HEAT BALANCE by Peter J. Lamb Cooperative Institute for Mesoscale Meteorological Studies and School of Meteorology The University of Oklahoma

More information

Chapter Overview. Seasons. Earth s Seasons. Distribution of Solar Energy. Solar Energy on Earth. CHAPTER 6 Air-Sea Interaction

Chapter Overview. Seasons. Earth s Seasons. Distribution of Solar Energy. Solar Energy on Earth. CHAPTER 6 Air-Sea Interaction Chapter Overview CHAPTER 6 Air-Sea Interaction The atmosphere and the ocean are one independent system. Earth has seasons because of the tilt on its axis. There are three major wind belts in each hemisphere.

More information

RADIATION (SOLAR) Introduction. Solar Spectrum and Solar Constant. Distribution of Solar Insolation at the Top of the Atmosphere

RADIATION (SOLAR) Introduction. Solar Spectrum and Solar Constant. Distribution of Solar Insolation at the Top of the Atmosphere RADIATION (SOLAR) 1859 Workshop Proceedings, Joint Research Centre, Ispra, Italy, pp. 45 53. Ulaby FT (1981)Microwave response of vegetation. In Kahle AB, Weill G, Carter WD (eds) Advances in Space Research,

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

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

The Balance of Power in the Earth-Sun System

The Balance of Power in the Earth-Sun System NASA Facts National Aeronautics and Space Administration www.nasa.gov The Balance of Power in the Earth-Sun System The Sun is the major source of energy for Earth s oceans, atmosphere, land, and biosphere.

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

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

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

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

Multiple Choice Exam Questions

Multiple Choice Exam Questions Chapter 1 Multiple Choice Exam Questions 1. The primary source of energy for the earth's atmosphere is: a. energy from within the earth b. the sun c. erupting volcanoes d. lightning discharges associated

More information

6 th Grade Science Assessment: Weather & Water Select the best answer on the answer sheet. Please do not make any marks on this test.

6 th Grade Science Assessment: Weather & Water Select the best answer on the answer sheet. Please do not make any marks on this test. Select the be answer on the answer sheet. Please do not make any marks on this te. 1. Weather is be defined as the A. changes that occur in cloud formations from day to day. B. amount of rain or snow that

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

Waves Sound and Light

Waves Sound and Light Waves Sound and Light r2 c:\files\courses\1710\spr12\wavetrans.doc Ron Robertson The Nature of Waves Waves are a type of energy transmission that results from a periodic disturbance (vibration). They are

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

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

Seasonal Temperature Variations

Seasonal Temperature Variations Seasonal and Daily Temperatures Fig. 3-CO, p. 54 Seasonal Temperature Variations What causes the seasons What governs the seasons is the amount of solar radiation reaching the ground What two primary factors

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

Total radiative heating/cooling rates.

Total radiative heating/cooling rates. Lecture. Total radiative heating/cooling rates. Objectives:. Solar heating rates.. Total radiative heating/cooling rates in a cloudy atmosphere.. Total radiative heating/cooling rates in different aerosol-laden

More information

Optimum Solar Orientation: Miami, Florida

Optimum Solar Orientation: Miami, Florida Optimum Solar Orientation: Miami, Florida The orientation of architecture in relation to the sun is likely the most significant connection that we can make to place in regards to energy efficiency. In

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

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

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

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

8.5 Comparing Canadian Climates (Lab)

8.5 Comparing Canadian Climates (Lab) These 3 climate graphs and tables of data show average temperatures and precipitation for each month in Victoria, Winnipeg and Whitehorse: Figure 1.1 Month J F M A M J J A S O N D Year Precipitation 139

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

Humidity, Condensation, Clouds, and Fog. Water in the Atmosphere

Humidity, Condensation, Clouds, and Fog. Water in the Atmosphere Humidity, Condensation, Clouds, and Fog or Water in the Atmosphere The Hydrologic Cycle Where the Water Exists on Earth Evaporation From the Oceans and Land The Source of Water Vapor for the Atmosphere

More information

Changing Clouds in a Changing Climate: Anthropogenic Influences

Changing Clouds in a Changing Climate: Anthropogenic Influences Changing Clouds in a Changing Climate: Anthropogenic Influences Joel Norris Assistant Professor of Climate and Atmospheric Sciences Scripps Institution of Oceanography Global mean radiative forcing of

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

Semester 2. Final Exam Review

Semester 2. Final Exam Review Semester 2 Final Exam Review Motion and Force Vocab Motion object changes position relative to a reference point. Speed distance traveled in a period of time. Velocity speed in a direction. Acceleration

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

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

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

Name Period 4 th Six Weeks Notes 2015 Weather

Name Period 4 th Six Weeks Notes 2015 Weather Name Period 4 th Six Weeks Notes 2015 Weather Radiation Convection Currents Winds Jet Streams Energy from the Sun reaches Earth as electromagnetic waves This energy fuels all life on Earth including the

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

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

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

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

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

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

2. The map below shows high-pressure and low-pressure weather systems in the United States.

2. The map below shows high-pressure and low-pressure weather systems in the United States. 1. Which weather instrument has most improved the accuracy of weather forecasts over the past 40 years? 1) thermometer 3) weather satellite 2) sling psychrometer 4) weather balloon 6. Wind velocity is

More information

Characteristics of the. thermosphere

Characteristics of the. thermosphere Characteristics of the Atmosphere. If you were lost in the desert, you could survive for a few days without food and water. But you wouldn't last more than five minutes without the ' Objectives Describe

More information

Climate Lingo Bingo. Climate Discovery: Climate Future. http://.eo.ucar.edu. Teacher s Guide. National Science Content Standards Addressed:

Climate Lingo Bingo. Climate Discovery: Climate Future. http://.eo.ucar.edu. Teacher s Guide. National Science Content Standards Addressed: Climate Discovery: Climate Future Climate Lingo Bingo Teacher s Guide http://.eo.ucar.edu Subject Focus: Earth Science Environmental Science Political Science and Social Studies Materials & Preparations:

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

Ok, so if the Earth weren't tilted, we'd have a picture like the one shown below: 12 hours of daylight at all latitudes more insolation in the

Ok, so if the Earth weren't tilted, we'd have a picture like the one shown below: 12 hours of daylight at all latitudes more insolation in the Ok, so if the Earth weren't tilted, we'd have a picture like the one shown below: 12 hours of daylight at all latitudes more insolation in the tropics, less at higher latitudes Ok, so if the Earth weren't

More information

7613-1 - Page 1. Weather Unit Exam Pre-Test Questions

7613-1 - Page 1. Weather Unit Exam Pre-Test Questions Weather Unit Exam Pre-Test Questions 7613-1 - Page 1 Name: 1) Equal quantities of water are placed in four uncovered containers with different shapes and left on a table at room temperature. From which

More information

The Importance of Understanding Clouds

The Importance of Understanding Clouds NASA Facts National Aeronautics and Space Administration www.nasa.gov The Importance of Understanding Clouds One of the most interesting features of Earth, as seen from space, is the ever-changing distribution

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

ENVIRONMENTAL STRUCTURE AND FUNCTION: CLIMATE SYSTEM Vol. II - Low-Latitude Climate Zones and Climate Types - E.I. Khlebnikova

ENVIRONMENTAL STRUCTURE AND FUNCTION: CLIMATE SYSTEM Vol. II - Low-Latitude Climate Zones and Climate Types - E.I. Khlebnikova LOW-LATITUDE CLIMATE ZONES AND CLIMATE TYPES E.I. Khlebnikova Main Geophysical Observatory, St. Petersburg, Russia Keywords: equatorial continental climate, ITCZ, subequatorial continental (equatorial

More information

AP ENVIRONMENTAL SCIENCE 2007 SCORING GUIDELINES

AP ENVIRONMENTAL SCIENCE 2007 SCORING GUIDELINES AP ENVIRONMENTAL SCIENCE 2007 SCORING GUIDELINES Question 4 Some scientists estimate that by 2025 over 60 percent of the global human population will live in urban areas. Urban residents experience a variety

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

VARIATION IN LIGHT INTENSITY AT DIFFERENT LATITUDES AND SEASONS, EFFECTS OF CLOUD COVER, AND THE AMOUNTS OF DIRECT AND DIFFUSED LIGHT

VARIATION IN LIGHT INTENSITY AT DIFFERENT LATITUDES AND SEASONS, EFFECTS OF CLOUD COVER, AND THE AMOUNTS OF DIRECT AND DIFFUSED LIGHT VARIATION IN LIGHT INTENSITY AT DIFFERENT LATITUDES AND SEASONS, EFFECTS OF CLOUD COVER, AND THE AMOUNTS OF DIRECT AND DIFFUSED LIGHT Paul Burgess School of Applied Sciences, Cranfield University, Cranfield,

More information

Clouds: What They Are and What They Mean. Susannah Lopez. Introduction to Meteorology. 2 December 2008

Clouds: What They Are and What They Mean. Susannah Lopez. Introduction to Meteorology. 2 December 2008 Clouds: What They 1 Clouds: What They Are and What They Mean Susannah Lopez Introduction to Meteorology 2 December 2008 Clouds: What They 2 Clouds: What They Are and What They Mean Clouds are composed

More information

Earth s Cloud Feedback

Earth s Cloud Feedback Earth s Cloud Feedback Clouds are visible masses of liquid droplets and/or frozen crystals that remain suspended in the atmosphere. Molecule by molecule, water in a solid or liquid phase is 1000 times

More information

Clouds. A simple scientific explanation for the weather-curious. By Kira R. Erickson

Clouds. A simple scientific explanation for the weather-curious. By Kira R. Erickson Clouds A simple scientific explanation for the weather-curious By Kira R. Erickson Table of Contents 1 3 4 INTRO 2 Page 3 How Clouds Are Formed Types of Clouds Clouds and Weather More Information Page

More information

Climate Models: Uncertainties due to Clouds. Joel Norris Assistant Professor of Climate and Atmospheric Sciences Scripps Institution of Oceanography

Climate Models: Uncertainties due to Clouds. Joel Norris Assistant Professor of Climate and Atmospheric Sciences Scripps Institution of Oceanography Climate Models: Uncertainties due to Clouds Joel Norris Assistant Professor of Climate and Atmospheric Sciences Scripps Institution of Oceanography Global mean radiative forcing of the climate system for

More information

For further information, and additional background on the American Meteorological Society s Education Program, please contact:

For further information, and additional background on the American Meteorological Society s Education Program, please contact: Project ATMOSPHERE This guide is one of a series produced by Project ATMOSPHERE, an initiative of the American Meteorological Society. Project ATMOSPHERE has created and trained a network of resource agents

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

Solar Heating Basics. 2007 Page 1. a lot on the shape, colour, and texture of the surrounding

Solar Heating Basics. 2007 Page 1. a lot on the shape, colour, and texture of the surrounding 2007 Page 1 Solar Heating Basics Reflected radiation is solar energy received by collectorsfrom adjacent surfaces of the building or ground. It depends a lot on the shape, colour, and texture of the surrounding

More information

Energy - Heat, Light, and Sound

Energy - Heat, Light, and Sound Science Benchmark: 06:06 Heat, light, and sound are all forms of energy. Heat can be transferred by radiation, conduction and convection. Visible light can be produced, reflected, refracted, and separated

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

Forms of Energy Explain

Forms of Energy Explain Forms of Energy Explain DIRECTIONS 1. For the Explain portion of the section, work through each slide 2. For each form there are three slides: 1. Introduce the form of energy 2. Give examples of the form

More information

An Introduction to Twomey Effect

An Introduction to Twomey Effect An Introduction to Twomey Effect Guillaume Mauger Aihua Zhu Mauna Loa, Hawaii on a clear day Mauna Loa, Hawaii on a dusty day Rayleigh scattering Mie scattering Non-selective scattering. The impact of

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

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

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

FIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES

FIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES FIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES UNIVERSE CYCLE OVERVIEW OF FIRST GRADE UNIVERSE WEEK 1. PRE: Describing the Universe. LAB: Comparing and contrasting bodies that reflect light. POST: Exploring

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

Sunlight and its Properties. EE 495/695 Y. Baghzouz

Sunlight and its Properties. EE 495/695 Y. Baghzouz Sunlight and its Properties EE 495/695 Y. Baghzouz The sun is a hot sphere of gas whose internal temperatures reach over 20 million deg. K. Nuclear fusion reaction at the sun's core converts hydrogen to

More information

THIRD GRADE WEATHER 1 WEEK LESSON PLANS AND ACTIVITIES

THIRD GRADE WEATHER 1 WEEK LESSON PLANS AND ACTIVITIES THIRD GRADE WEATHER 1 WEEK LESSON PLANS AND ACTIVITIES WATER CYCLE OVERVIEW OF THIRD GRADE WATER WEEK 1. PRE: Comparing the different components of the water cycle. LAB: Contrasting water with hydrogen

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

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

Chapter 3 Earth - Sun Relations

Chapter 3 Earth - Sun Relations 3.1 Introduction We saw in the last chapter that the short wave radiation from the sun passes through the atmosphere and heats the earth, which in turn radiates energy in the infrared portion of the electromagnetic

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

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

CGC1D1: Interactions in the Physical Environment Factors that Affect Climate

CGC1D1: Interactions in the Physical Environment Factors that Affect Climate Name: Date: Day/Period: CGC1D1: Interactions in the Physical Environment Factors that Affect Climate Chapter 12 in the Making Connections textbook deals with Climate Connections. Use pages 127-144 to fill

More information

SPQ Module 3 Solar Power

SPQ Module 3 Solar Power SPQ Module 3 Solar Power The sun is the source of all life on earth. Yet we sometimes forget how central it is to our every activity. We stumble through our daily routine worrying about the mundane tribulations

More information

After a wave passes through a medium, how does the position of that medium compare to its original position?

After a wave passes through a medium, how does the position of that medium compare to its original position? Light Waves Test Question Bank Standard/Advanced Name: Question 1 (1 point) The electromagnetic waves with the highest frequencies are called A. radio waves. B. gamma rays. C. X-rays. D. visible light.

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