Emissivity and Remote Sensing

Size: px
Start display at page:

Download "Emissivity and Remote Sensing"

Transcription

1 Emissivity and Remote Sensing Introduction: In the last laboratory with reflectivity we touched on the subject of emissivity. In comparison to reflectivity, emissivity is actually a bit more complex from a physics point of view. In the following diagram, the overall concepts of reflectivity and emissivity are presented in simplified form: Where does emissivity come into the diagram? Emissivity is defined as the ratio of absorbed radiation energy to total incoming radiation energy compared to a theoretical blackbody (which absorbs everything), and thus is a measure of absorptivity. In physics, energy is neither created or destroyed and incident photon energy is divided into a lower energy photon, which is re-emitted, and into molecular collisions and movement which is called, interestingly, nonradiative energy. Collisions continue to result in emission of lower wavelengths until motion is dissipated. The measurable part of emissivity is when sensors can pick up on re-radiated wavelengths (IR).

2 A number of atomic substances are identified by individual wavelengths (IR, visible and UV) that are absorbed and then immediately re-emitted in the same wavelength when electrons jump to the next orbital level and then fall back to baseline, with little chance of collision and vibrational (non-radiative) consumption of energy. These patterns are called absorption and emission spectra- the visible emission spectrum of most atoms appears as a set of characteristic color bands at distinct wavelengths. Molecules often do not have the same sharp spectra due to collision incidents or deviated emission pathways, resulting in Stokes shift and colored bands of absorption. courtesy Absorption and emission spectra of molecular perylene

3 Solar radiation is well-documented in terms of wavelength emission, all of which are incident on the earth s surface. boojum.as.arizona.edu/.../spectra/spectra.html The heating of the atmosphere is due to absorption by greenhouse gases of re-radiated IR radiation from the earth s surface. These atmospheric molecules then re-radiate part of this energy as longer wavelength IR in all directions, including back to the earth s surface. IR radiation is often called heat radiation because it results in vibration of molecules and higher temperature (hν = mv 2 /2 = mcδt). atlas.nrcan.gc.ca/.../figure_4.jpg/image_view

4 Note below that earth s continuous radiation spectrum shows mostly radiation in the infrared region, as expected. Measurement of Emissivity: Of interest is the fact that temperatures of different materials in thermal equilibrium in the same location are all the same, but infrared radiation differs by material. As we have seen, substances absorb different frequencies and radiate out lower frequencies due to collision consumption. Emissivity is also dependent on the temperature of the object and the incident wavelength of light on the material. This is of use in our laboratory, where we are looking at emissivity which varies by material properties, not temperature or incident wavelength. In real life, on a global scale, temperatures are not the same for different substances and objects, and since emissivity is also dependent on temperature, satellite images give different values based on type of material and relative temperature. Thermal (infrared) thermometers have detectors that typically measure in the 0.7 to 20 micron range. All are non contact thermometers. Ideally, a good thermal sensor will detect a wide range of wavelengths in the IR and keep its own thermal emissions to a minimum. Internal temperature references allow the sensor to assign a temperature to the incoming IR radiation. courtesy

5 Contact thermometers measure thermal energy by conduction, i.e., vibrational energy passed on to the thermometer, draining energy from the material to set thermometer molecules in motion. The two substances equilibrate close to the original temperature of the material being measured. Each will continue to give off characteristic infrared radiation, however, since vibrational patterns for each will differ. Satellite measured emissivities are translated at times into gray tones, where higher emissivity values are represented by lighter grays and lower values by darker grays, or the entire set of shades are assigned false colors. earth.esa.int/ers/article_archive/etna html (Mt. Etna plume) (Landsat)

6 Laboratory- emissivity of common materials Procedure: 1. Students will use a laser infrared sensor, which when aimed at various materials will give the radiation level, or emissivity of the material. 2. The sensor can be aimed by students at each material at approximately the same height, or set up in a more accurate way by attaching the sensor to a ring stand by clamp. 3. Place each material to be tested on a platform or in a Petri dish on the platform if there is the potential of a mess. 4. The sensor trigger is pulled and a red laser guide should appear on the materialhold until digital readout is stable and release and the sensor will register IR radiation as temperature. 5. Record temperatures and compare to literature values.

7 There are characteristic emissivity values published for a number of materials. Typically, materials with high specific heats tend to be better absorbers/emitters. Emissivity is measured as a decimal value, since 1 represents 100% absorption of incident radiation. A caution about literature values: Incident wavelength and target temperature make a difference. Values listed below did not reference either of these for the most part. The dry and wet soil, skin, snow and electrical tape values were referenced at an incident wavelength range of 3.4 to 5 microns and temperatures well beyond room temperature. Thus laboratory values may differ considerably. We compared our temperatures to a blackbody temperature of our own device- wet charcoal. Literature values: Infrared-USA.com; Material Asphalt Red brick Lime clay brick Glass Clay Literature lab emissivity

8 Clay tiles 0.33 Cloth 0.95 Copper, polished 0.07* Copper, oxidized 0.87 Black elec tape 0.97 Granite-rough 0.90 Grass 0.98 Ice Iron, not oxidized 0.05 Iron, oxidized 0.74 Limestone Paper Plastic 0.95 Soil, dry 0.92 Soil, wet 0.95 Sand 0.90 Sandstone 0.67 Snow 0.80 to 0.90 Straw Water Wood Wood (sawdust) 0.75 Zinc (polished) 0.02* *Shiny metal values must be calculated as the difference in IR thermometer readings between bare metal and metal covered with a thin black coat of paint. Be careful to cover the entire sample of metal with black paint or attenuated reflectance may still reach the IR sensor on the thermometer. Questions 1. How do the laboratory values differ from literature values? If there are differences, an explanation for the differences. 2. How do metals behave in terms of absorption and suggest a reason for their overall Behavior (note the low emissivities). Look up the specific heat of copper and water. How do specific heats seem to correlate with absorption? 3. Note the two images for the westward ocean current off the east coast of the U.S. What do you think the false colors represent in terms of thermoclines?

9 rs.gso.uri.edu/amy/feature.gif Gulf Stream June 1988 Gulf Stream January How can information on temperature of water (currents, etc.) help us? (Hint: Think of fishing, shipping, environmental problems): 5. Is there a difference in the terms emissivity and emittivity? 6. Laboratory experiments for emissivities of materials depend on holding temperature, incident wavelength and area of testing constant. The area is held constant by holding the thermometer at a constant length from the target. The instrument in our lab expresses the following target areas for a corresponding length: 5 cm: cm 2 10 cm: 0.25 cm 2 20 cm: 0.50 cm 2 Is this a linear relationship? Demonstrate how you know this. Project what the area is for the thermometer held at 12 cm from the target.

10 6. Compare the two USDA maps below and speculate as to how this area of North Dakota changed from 2000 to In these maps crop areas are colored red. What could be the cause of the differences? How do land thermal images help us? (Hint: Think of crops, weather, land use): 7. Locate a pair of thermal images for any area and describe the differences and possible causes. You might want to investigate slash and burn agriculture in South America or Africa, desertification in Middle East or western U.S., etc. Here is a list of possible web sites, but use your own if you like: Naturalhazards.nasa.gov Earthobservatory.nasa.gov Science.nasa.gov seamless.usgs.gov ned.usgs.gov soildatamart.nrcs.usda.gov nationalmap.gov county-map.digital-topo-maps.com

Emissivity and Remote Sensing

Emissivity and Remote Sensing Emissivity and Remote Sensing Introduction: In the last laboratory with reflectivity we touched on the subject of emissivity. In comparison to reflectivity, emissivity is actually a bit more complex from

More information

Reflectivity in Remote Sensing

Reflectivity in Remote Sensing Reflectivity in Remote Sensing The amount of absorbance and reflection of white light by a substance is dependent upon the molecular makeup of the substance. Humans have used dyes for years to obtain colors-

More information

Energy Balance and Temperature. Ch. 3: Energy Balance. Ch. 3: Temperature. Controls of Temperature

Energy Balance and Temperature. Ch. 3: Energy Balance. Ch. 3: Temperature. Controls of Temperature Energy Balance and Temperature 1 Ch. 3: Energy Balance Propagation of Radiation Transmission, Absorption, Reflection, Scattering Incoming Sunlight Outgoing Terrestrial Radiation and Energy Balance Net

More information

Energy Balance and Temperature

Energy Balance and Temperature Energy Balance and Temperature 1 Ch. 3: Energy Balance Propagation of Radiation Transmission, Absorption, Reflection, Scattering Incoming Sunlight Outgoing Terrestrial Radiation and Energy Balance Net

More information

Blackbody Radiation. A substance that absorbs all incident wavelengths completely is called a blackbody.

Blackbody Radiation. A substance that absorbs all incident wavelengths completely is called a blackbody. Blackbody Radiation A substance that absorbs all incident wavelengths completely is called a blackbody. What's the absorption spectrum of a blackbody? Absorption (%) 100 50 0 UV Visible IR Wavelength Blackbody

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

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

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

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

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

HL-800K Infrared Laser Thermometer. -50 C to +800 C (13:1 ratio) User Manual

HL-800K Infrared Laser Thermometer. -50 C to +800 C (13:1 ratio) User Manual HL-800K Infrared Laser Thermometer -50 C to +800 C (13:1 ratio) User Manual TABLE OF CONTENTS INTRODUCTION... 3 FEATURES... 3 WIDE APPLICATION RANGE... 3 SAFETY... 3 DISTANCE & SPOT SIZE... 4 SPECIFICATIONS...

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

PHYSICS 289 Experiment 3 Fall Heat transfer and the Greenhouse Effect

PHYSICS 289 Experiment 3 Fall Heat transfer and the Greenhouse Effect PHYSICS 289 Experiment 3 Fall 2006 Heat transfer and the Greenhouse Effect Only a short report is required: worksheets, graphs and answers to the questions. Introduction In this experiment we study the

More information

How does the surface type and moisture content affect the surfaceʼs temperature?

How does the surface type and moisture content affect the surfaceʼs temperature? How does the surface type and moisture content affect the surfaceʼs temperature? Introduction In addition to the output of and the distance from the energy source, surface type (surface reflectivity, specific

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

User Manual. Stick-Style Water-Resistant Infrared Thermometer with 8:1 Distance-to-Sight Ratio. Model with NIST-Traceable Calibration

User Manual. Stick-Style Water-Resistant Infrared Thermometer with 8:1 Distance-to-Sight Ratio. Model with NIST-Traceable Calibration User Manual Stick-Style Water-Resistant Infrared Thermometer with 8:1 Distance-to-Sight Ratio with NIST-Traceable Calibration Model 20250-09 THE STANDARD IN PRECISION MEASUREMENT Introduction The Digi-Sense

More information

Stick-Style Water-Resistant Infrared Thermometer for Foodservice Applications with 4:1 Distance-to-Sight Ratio Model

Stick-Style Water-Resistant Infrared Thermometer for Foodservice Applications with 4:1 Distance-to-Sight Ratio Model Stick-Style Water-Resistant Infrared Thermometer for Foodservice Applications with 4:1 Distance-to-Sight Ratio Model 35625-15 THE STANDARD IN PRECISION MEASUREMENT 1 DGMAN_35625-15_(ENG_FR).indd 1 7/8/2014

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

Extrasolar planets Detection and habitability

Extrasolar planets Detection and habitability Extrasolar planets Detection and habitability October 23rd 2014 Detecting exoplanets Primary methods : Direct imaging Transit Radial velocity Direct imaging Planets are much fainter than their host star

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

Infrared Experiments of Thermal Energy and Heat Transfer

Infrared Experiments of Thermal Energy and Heat Transfer Infrared Experiments of Thermal Energy and Heat Transfer You will explore thermal energy, thermal equilibrium, heat transfer, and latent heat in a series of hands-on activities augmented by the thermal

More information

2. Energy Balance. 1. All substances radiate unless their temperature is at absolute zero (0 K). Gases radiate at specific frequencies, while solids

2. Energy Balance. 1. All substances radiate unless their temperature is at absolute zero (0 K). Gases radiate at specific frequencies, while solids I. Radiation 2. Energy Balance 1. All substances radiate unless their temperature is at absolute zero (0 K). Gases radiate at specific frequencies, while solids radiate at many Click frequencies, to edit

More information

Basic cloud Interpretation using Satellite Imagery

Basic cloud Interpretation using Satellite Imagery Basic cloud Interpretation using Satellite Imagery Introduction Recall that images from weather satellites are actually measurements of energy from specified bands within the Electromagnetic (EM) spectrum.

More information

Sunlight and Temperature

Sunlight and Temperature Sunlight and Temperature Name Purpose: Study microclimate differences due to sunlight exposure, location, and surface; practice environmental measurements; study natural energy flows; compare measurements;

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

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

Kinds of Energy. Defining Energy is Hard! EXPLAIN: 1. Energy and Radiation. Conservation of Energy. Sco; Denning CSU ESMEI ATS 1

Kinds of Energy. Defining Energy is Hard! EXPLAIN: 1. Energy and Radiation. Conservation of Energy. Sco; Denning CSU ESMEI ATS 1 Defining Energy is Hard! EXPLAIN: 1. Energy and Radiation Energy is the capacity to perform work (but physicists have a special definition for work, too!) Part of the trouble is that scientists have appropriated

More information

Heat Transfer. Conduction, Convection, and Radiation. Review: Temperature

Heat Transfer. Conduction, Convection, and Radiation. Review: Temperature Heat Transfer Conduction, Convection, and Radiation Review: Temperature! Temperature is:! The quantity that tells how hot or cold something is compared with a standard! A measure of the average kinetic

More information

A) usually less B) dark colored and rough D) light colored with a smooth surface A) transparency of the atmosphere D) rough, black surface

A) usually less B) dark colored and rough D) light colored with a smooth surface A) transparency of the atmosphere D) rough, black surface 1. Base your answer to the following question on the diagram below which shows two identical houses, A and B, in a city in North Carolina. One house was built on the east side of a factory, and the other

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

ESS15 Lecture 7. The Greenhouse effect.

ESS15 Lecture 7. The Greenhouse effect. ESS15 Lecture 7 The Greenhouse effect. Housekeeping. First midterm is in one week. Open book, open notes. Covers material through end of Friday s lecture Including today s lecture (greenhouse effect) And

More information

8.5 GREENHOUSE EFFECT 8.6 GLOBAL WARMING HW/Study Packet

8.5 GREENHOUSE EFFECT 8.6 GLOBAL WARMING HW/Study Packet 8.5 GREENHOUSE EFFECT 8.6 GLOBAL WARMING HW/Study Packet Required: READ Tsokos, pp 434-450 Hamper pp 294-307 SL/HL Supplemental: none REMEMBER TO. Work through all of the example problems in the texts

More information

Emissivity: Understanding the difference between apparent and actual infrared temperatures

Emissivity: Understanding the difference between apparent and actual infrared temperatures Emissivity: Understanding the difference between apparent and actual infrared temperatures By L. Terry Clausing, P.E. ASNT Certified NDT Level III T/IR, for Fluke Corporation Application Note Taking infrared

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

Section 7. Temperature Measurement

Section 7. Temperature Measurement Section 7 Temperature Measurement 7/25/2017 Engineering Measurements 7 1 Working Definition Temperature is a measure of the average kinetic energy of the molecules that make of a substance. After time,

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

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

Chapter 02 Energy and Matter in the Atmosphere

Chapter 02 Energy and Matter in the Atmosphere Chapter 02 Energy and Matter in the Atmosphere Multiple Choice Questions 1. The most common gas in the atmosphere is. A. oxygen (O2). B. carbon dioxide (CO2). C. nitrogen (N2). D. methane (CH4). Section:

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

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

There are four phases of matter: Phases of Matter

There are four phases of matter: Phases of Matter HEAT SCIENCE There are four phases of matter: Phases of Matter There are four phases of matter: Phases of Matter Animation States of Matter Solids Solids: Are rigid, crystalline Hold their shape Have little

More information

Spectral reflectance: When the solar radiation is incident upon the earth s surface, it is either

Spectral reflectance: When the solar radiation is incident upon the earth s surface, it is either Spectral reflectance: When the solar radiation is incident upon the earth s surface, it is either reflected by the surface, transmitted into the surface or absorbed and emitted by the surface. Remote sensing

More information

Fundamentals of Remote Sensing

Fundamentals of Remote Sensing Division of Spatial Information Science Graduate School Life and Environment Sciences University of Tsukuba Fundamentals of Remote Sensing Prof. Dr. Yuji Murayama Surantha Dassanayake 10/6/2010 1 Fundamentals

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

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

Absorptivity, Reflectivity, and Transmissivity

Absorptivity, Reflectivity, and Transmissivity cen54261_ch21.qxd 1/25/4 11:32 AM Page 97 97 where f l1 and f l2 are blackbody functions corresponding to l 1 T and l 2 T. These functions are determined from Table 21 2 to be l 1 T (3 mm)(8 K) 24 mm K

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

Properties of Electromagnetic Radiation Chapter 5. What is light? What is a wave? Radiation carries information

Properties of Electromagnetic Radiation Chapter 5. What is light? What is a wave? Radiation carries information Concepts: Properties of Electromagnetic Radiation Chapter 5 Electromagnetic waves Types of spectra Temperature Blackbody radiation Dual nature of radiation Atomic structure Interaction of light and matter

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

Electromagnetic Radiation. Radiation and the Planetary Energy Balance. Electromagnetic Spectrum of the Sun

Electromagnetic Radiation. Radiation and the Planetary Energy Balance. Electromagnetic Spectrum of the Sun Radiation and the Planetary Energy Balance Electromagnetic Radiation Solar radiation warms the planet Conversion of solar energy at the surface Absorption and emission by the atmosphere The greenhouse

More information

The gases: gases: H2O O and What What are The two two most most abundant gases The The two two most most abundant abundant Greenhouse

The gases: gases: H2O O and What What are The two two most most abundant gases The The two two most most abundant abundant Greenhouse This gas is NOT a Greenhouse Gas. 1. O 2 2. O 3 CH 4 3. CH 4. Freon 11 (a CFC) What are The gases: H 2 O and CO 2. 1. The two most abundant gases. 2. The two most abundant Greenhouse gases. 3. The two

More information

Chapter 2: The global ledger of radiation and heat

Chapter 2: The global ledger of radiation and heat Chapter 2: The global ledger of radiation and heat PROPERTIES OF RADIATION Everything radiates at all wavelengths! This includes the Sun, Earth, a candy bar, even us Fortunately, most objects don t radiate

More information

high energy state for the electron in the atom low energy state for the electron in the atom

high energy state for the electron in the atom low energy state for the electron in the atom Atomic Spectra Objectives The objectives of this experiment are to: 1) Build and calibrate a simple spectroscope capable of measuring wavelengths of visible light. 2) Measure several wavelengths of light

More information

INFRARED THERMOMETER Model : TM-959

INFRARED THERMOMETER Model : TM-959 LED target light, Emissivity adjustment INFRARED THERMOMETER Model : TM-959 Your purchase of this I N F R A R E D THERMOMETER marks a step forward for you into the field of precision measurement. Although

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

ABB temperature measurement Radiation thermometry. Measurement made easy. Process temperature measurement practice--non-contacting

ABB temperature measurement Radiation thermometry. Measurement made easy. Process temperature measurement practice--non-contacting Whitepaper_ WP_T_Non-Contacting_Temperature_Measurement ABB temperature measurement Radiation thermometry Measurement made easy Process temperature measurement practice--non-contacting By Gary Freeman,

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

THE EXOSPHERIC HEAT BUDGET

THE EXOSPHERIC HEAT BUDGET E&ES 359, 2008, p.1 THE EXOSPHERIC HEAT BUDGET What determines the temperature on earth? In this course we are interested in quantitative aspects of the fundamental processes that drive the earth machine.

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

Climate Change Lecture Notes

Climate Change Lecture Notes Climate Change Lecture Notes (Topic 12A) page 1 Climate Change Lecture Notes Learning Outcomes for the Climate Change Unit 1. Students can list observations which suggest that the world is warming, and

More information

PTYS 214 Spring Announcements. Midterm 3 next Thursday! Midterms 4 and 5 more spread out

PTYS 214 Spring Announcements. Midterm 3 next Thursday! Midterms 4 and 5 more spread out PTYS 214 Spring 2018 Announcements Midterm 3 next Thursday! Midterms 4 and 5 more spread out 1 Previously Geothermal Energy Radioactive Decay Accretional Energy Heat of Differentiation Why Water? Phase

More information

Chapter 4. Spectroscopy. Dr. Tariq Al-Abdullah

Chapter 4. Spectroscopy. Dr. Tariq Al-Abdullah Chapter 4 Spectroscopy Dr. Tariq Al-Abdullah Learning Goals: 4.1 Spectral Lines 4.2 Atoms and Radiation 4.3 Formation of the Spectral Lines 4.4 Molecules 4.5 Spectral Line Analysis 2 DR. T. AL-ABDULLAH

More information

How does your eye form an Refraction

How does your eye form an Refraction Astronomical Instruments Eyes and Cameras: Everyday Light Sensors How does your eye form an image? How do we record images? How does your eye form an image? Refraction Refraction is the bending of light

More information

Lecture 6 - spectroscopy

Lecture 6 - spectroscopy Lecture 6 - spectroscopy 1 Light Electromagnetic radiation can be thought of as either a wave or as a particle (particle/wave duality). For scattering of light by particles, air, and surfaces, wave theory

More information

PTYS 214 Fall Announcements

PTYS 214 Fall Announcements PTYS 214 Fall 2017 Announcements Midterm 3 next Thursday! Midterms 4 and 5 more spread out Extra credit: attend Lynn Carter's evening lecture 10/4, 7:00 pm takes notes and get them signed / stamped! 1

More information

Light Up Your World Adapted from Reflecting on Reflectivity,

Light Up Your World Adapted from Reflecting on Reflectivity, Climate Change I m Supposed To Know What That Is? Light Up Your World Adapted from Reflecting on Reflectivity, http://www.climatechangenorth.ca Overview: Students often confuse global warming and the depletion

More information

Lecture 2-07: The greenhouse, global heat engine.

Lecture 2-07: The greenhouse, global heat engine. Lecture 2-07: The greenhouse, global heat engine http://en.wikipedia.org/ the sun s ultraviolet (left) and infrared radiation imagers.gsfc.nasa.gov/ems/uv.html www.odysseymagazine.com/images SOLAR FLARES

More information

What can laser light do for (or to) me?

What can laser light do for (or to) me? What can laser light do for (or to) me? Phys 1020, Day 15: Questions? Refection, refraction LASERS: 14.3 Next Up: Finish lasers Cameras and optics 1 Eyes to web: Final Project Info Light travels more slowly

More information

10.1 TEMPERATURE, THERMAL ENERGY AND HEAT Name: Date: Block: (Reference: pp of BC Science 10)

10.1 TEMPERATURE, THERMAL ENERGY AND HEAT Name: Date: Block: (Reference: pp of BC Science 10) 10.1 TEMPERATURE, THERMAL ENERGY AND HEAT Name: Date: Block: (Reference: pp. 424-435 of BC Science 10) kinetic molecular theory: explains that matter is made up of tiny that are constantly. These atoms

More information

Chapter 11 FUNDAMENTALS OF THERMAL RADIATION

Chapter 11 FUNDAMENTALS OF THERMAL RADIATION Chapter Chapter Fundamentals of Thermal Radiation FUNDAMENTALS OF THERMAL RADIATION Electromagnetic and Thermal Radiation -C Electromagnetic waves are caused by accelerated charges or changing electric

More information

General Physics (PHY 2130)

General Physics (PHY 2130) General Physics (PHY 2130) Lecture 34 Heat Heat transfer Conduction Convection Radiation http://www.physics.wayne.edu/~apetrov/phy2130/ Lightning Review Last lecture: 1. Thermal physics Heat. Specific

More information

Tananyag fejlesztés idegen nyelven

Tananyag fejlesztés idegen nyelven Tananyag fejlesztés idegen nyelven Prevention of the atmosphere KÖRNYEZETGAZDÁLKODÁSI AGRÁRMÉRNÖKI MSC (MSc IN AGRO-ENVIRONMENTAL STUDIES) Fundamentals in air radition properties Lecture 8 Lessons 22-24

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

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

Model ST-616CT. Instruction Manual. Infrared Thermo-Hygrometer. reedinstruments. www. com

Model ST-616CT. Instruction Manual. Infrared Thermo-Hygrometer. reedinstruments. www. com Model ST-616CT Infrared Thermo-Hygrometer Instruction Manual reedinstruments com Table of Contents Safety... 2 Features... 3 Specifications...4-5 Instrument Description...6-7 Operating Instructions...8-10

More information

The last 2 million years.

The last 2 million years. Lecture 5: Earth Climate History - Continued Ice core records from both Greenland and Antarctica have produced a remarkable record of climate during the last 450,000 years. Trapped air bubbles provide

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

Electromagnetic Waves

Electromagnetic Waves ELECTROMAGNETIC RADIATION AND THE ELECTROMAGNETIC SPECTRUM Electromagnetic Radiation (EMR) THE ELECTROMAGNETIC SPECTRUM Electromagnetic Waves A wave is characterized by: Wavelength (λ - lambda) is the

More information

The greenhouse effect

The greenhouse effect 16 Waves of amplitude of 1 m roll onto a beach at a rate of one every 12 s. If the wavelength of the waves is 120 m, calculate (a) the velocity of the waves (b) how much power there is per metre along

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

Understanding the Greenhouse Effect

Understanding the Greenhouse Effect EESC V2100 The Climate System spring 200 Understanding the Greenhouse Effect Yochanan Kushnir Lamont Doherty Earth Observatory of Columbia University Palisades, NY 1096, USA kushnir@ldeo.columbia.edu Equilibrium

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

Measuring Albedo. Materials Light meters Student worksheets

Measuring Albedo. Materials Light meters Student worksheets Measuring Albedo Materials Light meters Student worksheets Background: Albedo is a measure of reflectivity. It is the ratio of the solar radiation (short wave radiation) reflected by a surface to the total

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

SIT IN YOUR GROUP AREA TODAY!

SIT IN YOUR GROUP AREA TODAY! Tuesday Sep 23th SIT IN YOUR GROUP AREA TODAY! Wrap-Up of Topic #5 on the Radiation Laws to get ready for Topic # 6 Atmospheric & Structure & Composition RQ-3 was cutoff 30 minutes before class today if

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

INFRARED THERMOMETER TM0819

INFRARED THERMOMETER TM0819 INFRARED THERMOMETER Instruction Manual HORMES LIMITED cs@perfectprime.com G/F UNIT 3, 61 GLENTHORNE ROAD, LONDON W6 0LJ UNITED KINGDOM +44 203 7695377 Retailer Email Address Telephone P.1 CONTENTS 1.

More information

Warming Earth and its Atmosphere The Diurnal and Seasonal Cycles

Warming Earth and its Atmosphere The Diurnal and Seasonal Cycles Warming Earth and its Atmosphere The Diurnal and Seasonal Cycles Or, what happens to the energy received from the sun? First We Need to Understand The Ways in Which Heat Can be Transferred in the Atmosphere

More information

Solar Radiation and Environmental Biophysics Geo 827, MSU Jiquan Chen Oct. 6, 2015

Solar Radiation and Environmental Biophysics Geo 827, MSU Jiquan Chen Oct. 6, 2015 Solar Radiation and Environmental Biophysics Geo 827, MSU Jiquan Chen Oct. 6, 2015 1) Solar radiation basics 2) Energy balance 3) Other relevant biophysics 4) A few selected applications of RS in ecosystem

More information

Remote Sensing C. Rank: Points: Science Olympiad North Regional Tournament at the University of Florida. Name(s): Team Name: School Name:

Remote Sensing C. Rank: Points: Science Olympiad North Regional Tournament at the University of Florida. Name(s): Team Name: School Name: Remote Sensing C Science Olympiad North Regional Tournament at the University of Florida Rank: Points: Name(s): Team Name: School Name: Team Number: Instructions: DO NOT BEGIN UNTIL GIVEN PERMISSION. DO

More information

Thermal Radiation By: Prof. K M Joshi

Thermal Radiation By: Prof. K M Joshi Thermal Radiation By: Prof. K M Joshi Radiation originate due to emission of matter and its subsequent transports does not required any matter / medium. Que: Then what is the nature of this transport???

More information

Taking Fingerprints of Stars, Galaxies, and Other Stuff. The Bohr Atom. The Bohr Atom Model of Hydrogen atom. Bohr Atom. Bohr Atom

Taking Fingerprints of Stars, Galaxies, and Other Stuff. The Bohr Atom. The Bohr Atom Model of Hydrogen atom. Bohr Atom. Bohr Atom Periodic Table of Elements Taking Fingerprints of Stars, Galaxies, and Other Stuff Absorption and Emission from Atoms, Ions, and Molecules Universe is mostly (97%) Hydrogen and Helium (H and He) The ONLY

More information

Mon April 17 Announcements: bring calculator to class from now on (in-class activities, tests) HW#2 due Thursday

Mon April 17 Announcements: bring calculator to class from now on (in-class activities, tests) HW#2 due Thursday Mon April 17 Announcements: bring calculator to class from now on (in-class activities, tests) HW#2 due Thursday Today: Fundamentals of Planetary Energy Balance Incoming = Outgoing (at equilibrium) Incoming

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

ME 476 Solar Energy UNIT TWO THERMAL RADIATION

ME 476 Solar Energy UNIT TWO THERMAL RADIATION ME 476 Solar Energy UNIT TWO THERMAL RADIATION Unit Outline 2 Electromagnetic radiation Thermal radiation Blackbody radiation Radiation emitted from a real surface Irradiance Kirchhoff s Law Diffuse and

More information

Mechanisms of heat transfer

Mechanisms of heat transfer Lecture 4 Mechanisms of heat transfer Pre-reading: 17.7 Review Heat can be transferred from one object to another due to a temperature difference. The properties of many objects change with temperature:

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

Remote Sensing. RAHS C Division Invitational

Remote Sensing. RAHS C Division Invitational Remote Sensing RAHS C Division Invitational 2017-18 Instructions: Answer all questions on this answer sheet. Sheets may be double sided, check both sides! If you separate the sheets of the test be sure

More information

Ready for some more SCIENCE Homer?

Ready for some more SCIENCE Homer? Ready for some more SCIENCE Homer? Alright brain, you don t like me and I don t like you; but let s get through this and I can get back to killing you with beer! Homer gives his brain a pep talk Disclaimer:

More information

Fluid Circulation Review. Vocabulary. - Dark colored surfaces absorb more energy.

Fluid Circulation Review. Vocabulary. - Dark colored surfaces absorb more energy. Fluid Circulation Review Vocabulary Absorption - taking in energy as in radiation. For example, the ground will absorb the sun s radiation faster than the ocean water. Air pressure Albedo - Dark colored

More information