Torben Königk Rossby Centre/ SMHI
|
|
- Florence Spencer
- 5 years ago
- Views:
Transcription
1 Fundamentals of Climate Modelling Torben Königk Rossby Centre/ SMHI
2 Outline Introduction Why do we need models? Basic processes Radiation Atmospheric/Oceanic circulation Model basics Resolution Parameterizations Limitations
3 Why do we need models? Weather forecast What will the weather be in Norrköping tomorrow? What activities shall we plan for the weekend?
4 Why do we need models? Climate analysis How large is the natural variability? Mechanisms of climate processes?
5 Why do we need models? Climate scenarios How will the climate be in Norrköping in 30 years? Do we will have more extremes? How is sea level changing? Simulated temperature change until
6 The Climate System : What do we need to include?
7 Radiation: Black body radiation A black body absorbs all incident radiation A blackbody emits radiation according to Planck s law (shape of curves) Wien s displacement law give the temperature of a radiation source (maximum of curves) Total flux given by the Stefan-Boltzmann law (integration over the curve) wavelength [µm]
8 Longwave radiation of the Earth Emitted radiation at the Earth s surface 4-100µm (maximum at around 10µm) CO 2 and O 3 absorb at wavelengths within the Earth s emission spectrum. Increases in their concentration will increase the natural greenhouse effect and warm the planet. Water Vapour is the most active abosrbing gas in the IR spectrum.
9 Solar radiation Absorption of incoming solar radiation small Incoming radiation may be reflected by clouds, particles or by the ground The albedo (A) is the ratio between reflected and incoming radiation Cloud albedo varies (30-90%) Global average ca 30% (including clouds) Properties of the ground Snow Old snow Ice Sand Grass Forest Water Water (Sun close to horizon) Albedo (%)
10 Radiation balance of the Earth Assume balance between outgoing and incoming radiation on long term basis Solar constant 1368 W m -2 planetary albedo 30% Outgoing terrestrial radiation (longwave) is absorbed and reemitted in the atmosphere. The net effect is a warming of the surface (Te = 288 K)
11 Radiation Balance, Differential Heating Imbalances leads to temperature differences and thereby pressure gradients generating the general circulation of the atmosphere (and the oceans) Long term imbalance leads to climate change
12 Atmospheric motion Air is under influence of a number of forces resulting in movements (winds and turbulence) The forces are; the pressure gradient force, gravity, friction, centrifugal forces and the Coriolis force, The Coriolis force is an apparent force that leads to a deflection to the right (left) of all motion in the northern (southern) hemisphere It is proportional to the speed and depends on latitude (increasing towards the poles)
13 Atmospheric Circulation No rotation of the Earth cooling heating cooing Conservation of absolute angular momemtum and the stability of fluid flows leads to the break up of a thermally direct circulation around 30 poleward of the equator. Here the atmosphere develops instabilities (extra-tropical cyclones) that efficiently transport energy and momentum poleward.
14 Large scale ocean circulation The ocean circulation is driven by density contrasts in the ocean. Regions of intense heat loss from the ocean, surface winds and salinity of the ocean (sea ice melt, runoff, precipitation) govern the circulation. The continents play an important role.
15 Equations describing the atmosphere u t r u + V u + ω p fv + φ = x v r v φ + V v + ω + fu + = t p y φ = α p T r T + V T + ω αω / Cp = t p F X F y Q / Cp r V q t + p α = RT r + V ω = 0 p q q + ω p The atmosphere is governed by a set of physical laws expressing how the air moves, heating and cooling, moisture, and so on. Although the equations describing atmospheric behaviour can be formulated, they cannot be solved analytically. Instead, numerical methods are needed to provide approximate solutions. = S q
16 A global climate model (model describing the general circulation - GCM) In a GCM grid boxes cover the entire planet (ocean and atmosphere) Typical size is km in the horizontal Iayers in the vertical both in atmosphere and ocean Typical time step can be 30 min
17 Climate Model The information needed to run a GCM (atmosphere and ocean) is: Initial state of all the variables in all boxes A description of the land surface (topography and land use) Solar radiation Gas and aerosol composition of the atmosphere The resources needed to run a GCM (atmosphere and ocean) are: Super computer (many processors & 100 TB disk) Takes 2 weeks for 100 years simulation
18 Space and time scales Typical timescales of variation in the climate system. Atmosphere (seconds to weeks) Surface vegetation (weeks to years) Surface snow and sea-ice (days to years) Upper Ocean (days to years) Deep Ocean (months to multi-century) Glaciers (years to multi-century) Continental distribution and mountain building (100s to 1000s of thousand years)
19 Parametrized processes in a climate model Sea ice processes Mixing Deep Convection Eddies
20 The Development of Climate models Mid-1970s Mid-1980s Early 1990s Late 1990s Early 2000s Late 2000s Source: IPCC, TAR, 2001
21 Initialization/ chaotic behaviour NWP integrations started from very similar initial conditions may result in quite different forecasts Simulations with climate models can never be directly compared to observations: Never compare a single month or year from a model simulations to the corresponding year in reality! Compare statistics of a longer period (decades or more)!
22 Summary Climate models are an important tool to investigate past, present and future climates. Differential heating of the Earth causes atmospheric and oceanic circulation. Clouds, gases and particles are important for radiation balance. Main uncertainties of climate models are connected to low resolution and the need to parametrize small-scale processes. Climate is the statistics of weather.
EST 5101 Climate Change Science Chapter 5. Climate Models. Rezaul Karim Environmental Science & Technology Jessore University of science & Technology
EST 5101 Climate Change Science Chapter 5. Climate Models Rezaul Karim Environmental Science & Technology Jessore University of science & Technology Chapter outline overview of climate modelling; How Are
More informationClimate Modeling Dr. Jehangir Ashraf Awan Pakistan Meteorological Department
Climate Modeling Dr. Jehangir Ashraf Awan Pakistan Meteorological Department Source: Slides partially taken from A. Pier Siebesma, KNMI & TU Delft Key Questions What is a climate model? What types of climate
More informationCOURSE CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION
COURSE CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION DATE 4 JUNE 2014 LEADER CHRIS BRIERLEY Course Outline 1. Current climate 2. Changing climate 3. Future climate change 4. Consequences 5. Human
More informationCourse Outline CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION. 1. Current climate. 2. Changing climate. 3. Future climate change
COURSE CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION DATE 4 JUNE 2014 LEADER CHRIS BRIERLEY Course Outline 1. Current climate 2. Changing climate 3. Future climate change 4. Consequences 5. Human
More information1. Weather and climate.
Lecture 31. Introduction to climate and climate change. Part 1. Objectives: 1. Weather and climate. 2. Earth s radiation budget. 3. Clouds and radiation field. Readings: Turco: p. 320-349; Brimblecombe:
More informationLecture 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 informationCourse Outline. About Me. Today s Outline CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION. 1. Current climate. 2.
Course Outline 1. Current climate 2. Changing climate 3. Future climate change 4. Consequences COURSE CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION DATE 4 JUNE 2014 LEADER 5. Human impacts 6.
More information5. General Circulation Models
5. General Circulation Models I. 3-D Climate Models (General Circulation Models) To include the full three-dimensional aspect of climate, including the calculation of the dynamical transports, requires
More informationCLIMATE AND CLIMATE CHANGE MIDTERM EXAM ATM S 211 FEB 9TH 2012 V1
CLIMATE AND CLIMATE CHANGE MIDTERM EXAM ATM S 211 FEB 9TH 2012 V1 Name: Student ID: Please answer the following questions on your Scantron Multiple Choice [1 point each] (1) The gases that contribute to
More informationAssessment Schedule 2017 Earth and Space Science: Demonstrate understanding of processes in the atmosphere system (91414)
NCEA Level 3 Earth and Space Science (91414) 2017 page 1 of 6 Assessment Schedule 2017 Earth and Space Science: Demonstrate understanding of processes in the atmosphere system (91414) Evidence Statement
More informationThe Atmosphere. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems
The Atmosphere 1 How big is the atmosphere? Why is it cold in Geneva? Why do mountaineers need oxygen on Everest? 2 A relatively thin layer of gas over the Earths surface Earth s radius ~ 6400km Atmospheric
More informationGlaciology HEAT BUDGET AND RADIATION
HEAT BUDGET AND RADIATION A Heat Budget 1 Black body radiation Definition. A perfect black body is defined as a body that absorbs all radiation that falls on it. The intensity of radiation emitted by a
More informationEarth s Energy Balance and the Atmosphere
Earth s Energy Balance and the Atmosphere Topics we ll cover: Atmospheric composition greenhouse gases Vertical structure and radiative balance pressure, temperature Global circulation and horizontal energy
More informationIntroduction to Climate ~ Part I ~
2015/11/16 TCC Seminar JMA Introduction to Climate ~ Part I ~ Shuhei MAEDA (MRI/JMA) Climate Research Department Meteorological Research Institute (MRI/JMA) 1 Outline of the lecture 1. Climate System (
More informationElectromagnetic 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 informationGEO1010 tirsdag
GEO1010 tirsdag 31.08.2010 Jørn Kristiansen; jornk@met.no I dag: Først litt repetisjon Stråling (kap. 4) Atmosfærens sirkulasjon (kap. 6) Latitudinal Geographic Zones Figure 1.12 jkl TØRR ATMOSFÆRE Temperature
More informationChapter 6: Modeling the Atmosphere-Ocean System
Chapter 6: Modeling the Atmosphere-Ocean System -So far in this class, we ve mostly discussed conceptual models models that qualitatively describe the system example: Daisyworld examined stable and unstable
More informationThe Structure and Motion of the Atmosphere OCEA 101
The Structure and Motion of the Atmosphere OCEA 101 Why should you care? - the atmosphere is the primary driving force for the ocean circulation. - the atmosphere controls geographical variations in ocean
More information2/18/2013 Estimating Climate Sensitivity From Past Climates Outline
Estimating Climate Sensitivity From Past Climates Outline Zero-dimensional model of climate system Climate sensitivity Climate feedbacks Forcings vs. feedbacks Paleocalibration vs. paleoclimate modeling
More informationGlobal Climate Change
Global Climate Change Definition of Climate According to Webster dictionary Climate: the average condition of the weather at a place over a period of years exhibited by temperature, wind velocity, and
More informationATM S 111, Global Warming Climate Models
ATM S 111, Global Warming Climate Models Jennifer Fletcher Day 27: July 29, 2010 Using Climate Models to Build Understanding Often climate models are thought of as forecast tools (what s the climate going
More informationThe Planetary Circulation System
12 The Planetary Circulation System Learning Goals After studying this chapter, students should be able to: 1. describe and account for the global patterns of pressure, wind patterns and ocean currents
More informationObservation: predictable patterns of ecosystem distribution across Earth. Observation: predictable patterns of ecosystem distribution across Earth 1.
Climate Chap. 2 Introduction I. Forces that drive climate and their global patterns A. Solar Input Earth s energy budget B. Seasonal cycles C. Atmospheric circulation D. Oceanic circulation E. Landform
More informationEarth s Climate Patterns
Earth s Climate Patterns Reading: Chapter 17, GSF 10/2/09 Also Jackson (linked on course web site) 1 What aspects of climate affect plant distributions? Climate: long-term distribution of weather in an
More informationMAPH & & & & & & 02 LECTURE
Climate & Earth System Science Introduction to Meteorology & Climate MAPH 10050 Peter Lynch Peter Lynch Meteorology & Climate Centre School of Mathematical Sciences University College Dublin Meteorology
More informationClimate Roles of Land Surface
Lecture 5: Land Surface and Cryosphere (Outline) Climate Roles Surface Energy Balance Surface Water Balance Sea Ice Land Ice (from Our Changing Planet) Surface Albedo Climate Roles of Land Surface greenhouse
More informationWeather Forecasts and Climate AOSC 200 Tim Canty. Class Web Site: Lecture 27 Dec
Weather Forecasts and Climate AOSC 200 Tim Canty Class Web Site: http://www.atmos.umd.edu/~tcanty/aosc200 Topics for today: Climate Natural Variations Feedback Mechanisms Lecture 27 Dec 4 2018 1 Climate
More informationLecture 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 informationPlanetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.
Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric properties
More informationUnderstanding 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 informationQ.1 The most abundant gas in the atmosphere among inert gases is (A) Helium (B) Argon (C) Neon (D) Krypton
Q. 1 Q. 9 carry one mark each & Q. 10 Q. 22 carry two marks each. Q.1 The most abundant gas in the atmosphere among inert gases is (A) Helium (B) Argon (C) Neon (D) Krypton Q.2 The pair of variables that
More informationIntroduction to Atmospheric Circulation
Introduction to Atmospheric Circulation Start rotating table Cloud Fraction Dice Results from http://eos.atmos.washington.edu/erbe/ from http://eos.atmos.washington.edu/erbe/ from http://eos.atmos.washington.edu/erbe/
More informationClimate changes in Finland, but how? Jouni Räisänen Department of Physics, University of Helsinki
Climate changes in Finland, but how? Jouni Räisänen Department of Physics, University of Helsinki 19.9.2012 Outline Some basic questions and answers about climate change How are projections of climate
More informationClimate System. Sophie Zechmeister-Boltenstern
Climate System Sophie Zechmeister-Boltenstern Reference: Chapin F. St., Matson P., Mooney Harold A. 2002 Principles of Terrestrial Ecosystem Ecology. Springer, Berlin, 490 p. Structure of this lecture
More informationEarth Systems Science Chapter 3
Earth Systems Science Chapter 3 ELECTROMAGNETIC RADIATION: WAVES I. Global Energy Balance and the Greenhouse Effect: The Physics of the Radiation Balance of the Earth 1. Electromagnetic Radiation: waves,
More informationLecture 9: Climate Sensitivity and Feedback Mechanisms
Lecture 9: Climate Sensitivity and Feedback Mechanisms Basic radiative feedbacks (Plank, Water Vapor, Lapse-Rate Feedbacks) Ice albedo & Vegetation-Climate feedback Cloud feedback Biogeochemical feedbacks
More informationFluid 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 information1. 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 informationLecture 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 informationATMOSPHERIC CIRCULATION AND WIND
ATMOSPHERIC CIRCULATION AND WIND The source of water for precipitation is the moisture laden air masses that circulate through the atmosphere. Atmospheric circulation is affected by the location on the
More informationEarth s Heat Budget. What causes the seasons? Seasons
Earth s Heat Budget Solar energy and the global heat budget Transfer of heat drives weather and climate Ocean circulation A. Rotation of the Earth B. Distance from the Sun C. Variations of Earth s orbit
More informationClimate Modeling Research & Applications in Wales. John Houghton. C 3 W conference, Aberystwyth
Climate Modeling Research & Applications in Wales John Houghton C 3 W conference, Aberystwyth 26 April 2011 Computer Modeling of the Atmosphere & Climate System has revolutionized Weather Forecasting and
More informationGeneral Circulation. Nili Harnik DEES, Lamont-Doherty Earth Observatory
General Circulation Nili Harnik DEES, Lamont-Doherty Earth Observatory nili@ldeo.columbia.edu Latitudinal Radiation Imbalance The annual mean, averaged around latitude circles, of the balance between the
More informationChapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.
Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric
More informationMesoscale meteorological models. Claire L. Vincent, Caroline Draxl and Joakim R. Nielsen
Mesoscale meteorological models Claire L. Vincent, Caroline Draxl and Joakim R. Nielsen Outline Mesoscale and synoptic scale meteorology Meteorological models Dynamics Parametrizations and interactions
More informationRadiation in climate models.
Lecture. Radiation in climate models. Objectives:. A hierarchy of the climate models.. Radiative and radiative-convective equilibrium.. Examples of simple energy balance models.. Radiation in the atmospheric
More informationTopic # 11 HOW CLIMATE WORKS PART II
Topic # 11 HOW CLIMATE WORKS PART II The next chapter in the story: How differences in INSOLATION between low and high latitudes drive atmospheric circulation! pp 64 in Class Notes THE RADIATION BALANCE
More informationLecture 3: Global Energy Cycle
Lecture 3: Global Energy Cycle Planetary energy balance Greenhouse Effect Vertical energy balance Latitudinal energy balance Seasonal and diurnal cycles Solar Flux and Flux Density Solar Luminosity (L)
More informationConcepts of energy and heat
Concepts of energy and heat On the molecular level, what is heat? Energy absorbed by the molecule and converted to kinetic energy How is heat transferred? Conduction Convection Radiation Transfer of heat
More informationLet s make a simple climate model for Earth.
Let s make a simple climate model for Earth. What is the energy balance of the Earth? How is it controlled? ó How is it affected by humans? Energy balance (radiant energy) Greenhouse Effect (absorption
More informationThe PRECIS Regional Climate Model
The PRECIS Regional Climate Model General overview (1) The regional climate model (RCM) within PRECIS is a model of the atmosphere and land surface, of limited area and high resolution and locatable over
More informationKey Feedbacks in the Climate System
Key Feedbacks in the Climate System With a Focus on Climate Sensitivity SOLAS Summer School 12 th of August 2009 Thomas Schneider von Deimling, Potsdam Institute for Climate Impact Research Why do Climate
More informationChapter 3- Energy Balance and Temperature
Chapter 3- Energy Balance and Temperature Understanding Weather and Climate Aguado and Burt Influences on Insolation Absorption Reflection/Scattering Transmission 1 Absorption An absorber gains energy
More informationGlobal warming and Extremes of Weather. Prof. Richard Allan, Department of Meteorology University of Reading
Global warming and Extremes of Weather Prof. Richard Allan, Department of Meteorology University of Reading Extreme weather climate change Recent extreme weather focusses debate on climate change Can we
More information9/5/16. Section 3-4: Radiation, Energy, Climate. Common Forms of Energy Transfer in Climate. Electromagnetic radiation.
Section 3-4: Radiation, Energy, Climate Learning outcomes types of energy important to the climate system Earth energy balance (top of atm., surface) greenhouse effect natural and anthropogenic forcings
More informationContext: How does a climate model work?
www.atmosphere.mpg.de/enid/accenten > Nr. 7 March 2006 > C: Context 1 Context: How does a climate model work? Key words: modelling, scenarios, climate parameters, grid, physical formula Introduction The
More informationFactors That Affect Climate
Factors That Affect Climate Factors That Affect Climate Latitude As latitude (horizontal lines) increases, the intensity of solar energy decreases. The tropical zone is between the tropic of Cancer and
More informationEnergy 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 informationEnergy 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 information2018 Science Olympiad: Badger Invitational Meteorology Exam. Team Name: Team Motto:
2018 Science Olympiad: Badger Invitational Meteorology Exam Team Name: Team Motto: This exam has 50 questions of various formats, plus 3 tie-breakers. Good luck! 1. On a globally-averaged basis, which
More informationEnergy Systems, Structures and Processes Essential Standard: Analyze patterns of global climate change over time Learning Objective: Differentiate
Energy Systems, Structures and Processes Essential Standard: Analyze patterns of global climate change over time Learning Objective: Differentiate between weather and climate Global Climate Focus Question
More informationATMOS 5140 Lecture 1 Chapter 1
ATMOS 5140 Lecture 1 Chapter 1 Atmospheric Radiation Relevance for Weather and Climate Solar Radiation Thermal Infrared Radiation Global Heat Engine Components of the Earth s Energy Budget Relevance for
More informationLecture 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 informationATMO 436a. The General Circulation. Redacted version from my NATS lectures because Wallace and Hobbs virtually ignores it
ATMO 436a The General Circulation Redacted version from my NATS lectures because Wallace and Hobbs virtually ignores it Scales of Atmospheric Motion vs. Lifespan The general circulation Atmospheric oscillations
More informationLand Surface Sea Ice Land Ice. (from Our Changing Planet)
Lecture 5: Land Surface and Cryosphere (Outline) Land Surface Sea Ice Land Ice (from Our Changing Planet) Earth s s Climate System Solar forcing Atmosphere Ocean Land Solid Earth Energy, Water, and Biochemistry
More informationThe Transfer of Heat
The Transfer of Heat Outcomes: S2-4-03 Explain effects of heat transfer within the atmosphere and hydrosphere on the development and movement of wind and ocean currents. Coriolis Effect In our ecology
More informationTransient and Eddy. Transient/Eddy Flux. Flux Components. Lecture 3: Weather/Disturbance. Transient: deviations from time mean Time Mean
Lecture 3: Weather/Disturbance Transients and Eddies Climate Roles Mid-Latitude Cyclones Tropical Hurricanes Mid-Ocean Eddies Transient and Eddy Transient: deviations from time mean Time Mean Eddy: deviations
More informationEarth s Climate System. Surface Albedo. Climate Roles of Land Surface. Lecture 5: Land Surface and Cryosphere (Outline) Land Surface Sea Ice Land Ice
Lecture 5: Land Surface and Cryosphere (Outline) Earth s Climate System Solar forcing Land Surface Sea Ice Land Ice Atmosphere Ocean Land Solid Earth Energy, Water, and Biochemistry Cycles (from Our Changing
More informationLecture 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 informationScience 1206 Chapter 1 - Inquiring about Weather
Science 1206 Chapter 1 - Inquiring about Weather 1.1 - The Atmosphere: Energy Transfer and Properties (pp. 10-25) Weather and the Atmosphere weather the physical conditions of the atmosphere at a specific
More informationEarth: 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 informationTopic # 11 HOW CLIMATE WORKS continued (Part II) pp in Class Notes
Topic # 11 HOW CLIMATE WORKS continued (Part II) pp 61-67 in Class Notes To drive the circulation, the initial source of energy is from the Sun: Not to scale! EARTH- SUN Relationships 4 Things to Know
More informationLecture 3. Background materials. Planetary radiative equilibrium TOA outgoing radiation = TOA incoming radiation Figure 3.1
Lecture 3. Changes in planetary albedo. Is there a clear signal caused by aerosols and clouds? Outline: 1. Background materials. 2. Papers for class discussion: Palle et al., Changes in Earth s reflectance
More informationLecture 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 informationBlackbody 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 informationLecture 7: The Monash Simple Climate
Climate of the Ocean Lecture 7: The Monash Simple Climate Model Dr. Claudia Frauen Leibniz Institute for Baltic Sea Research Warnemünde (IOW) claudia.frauen@io-warnemuende.de Outline: Motivation The GREB
More informationChapter 9 External Energy Fuels Weather and Climate
Natural Disasters Tenth Edition Chapter 9 External Energy Fuels Weather and Climate Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display. 9-1 Weather Versus Climate
More informationATS150 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 informationATOC OUR CHANGING ENVIRONMENT Class 19 (Chp 6) Objectives of Today s Class: The Cryosphere [1] Components, time scales; [2] Seasonal snow
ATOC 1060-002 OUR CHANGING ENVIRONMENT Class 19 (Chp 6) Objectives of Today s Class: The Cryosphere [1] Components, time scales; [2] Seasonal snow cover, permafrost, river and lake ice, ; [3]Glaciers and
More informationLecture 2: Light And Air
Lecture 2: Light And Air Earth s Climate System Earth, Mars, and Venus Compared Solar Radiation Greenhouse Effect Thermal Structure of the Atmosphere Atmosphere Ocean Solid Earth Solar forcing Land Energy,
More informationWeather & Climate. Sanjay S. Limaye Space Science & Engineering Center University of Wisconsin-Madison
Weather & Climate Sanjay S. Limaye Space Science & Engineering Center University of Wisconsin-Madison 1 What is Weather? Webster s New Collegiate Dictionary: state of the atmosphere with respect to heat
More informationClimate Change 2007: The Physical Science Basis
Climate Change 2007: The Physical Science Basis Working Group I Contribution to the IPCC Fourth Assessment Report Presented by R.K. Pachauri, IPCC Chair and Bubu Jallow, WG 1 Vice Chair Nairobi, 6 February
More informationLecture 2: Global Energy Cycle
Lecture 2: Global Energy Cycle Planetary energy balance Greenhouse Effect Vertical energy balance Solar Flux and Flux Density Solar Luminosity (L) the constant flux of energy put out by the sun L = 3.9
More informationFundamentals of Atmospheric Radiation and its Parameterization
Source Materials Fundamentals of Atmospheric Radiation and its Parameterization The following notes draw extensively from Fundamentals of Atmospheric Physics by Murry Salby and Chapter 8 of Parameterization
More informationTemperature (T) degrees Celsius ( o C) arbitrary scale from 0 o C at melting point of ice to 100 o C at boiling point of water Also (Kelvin, K) = o C
1 2 3 4 Temperature (T) degrees Celsius ( o C) arbitrary scale from 0 o C at melting point of ice to 100 o C at boiling point of water Also (Kelvin, K) = o C plus 273.15 0 K is absolute zero, the minimum
More informationAtmospheric "greenhouse effect" - How the presence of an atmosphere makes Earth's surface warmer
Atmospheric "greenhouse effect" - How the presence of an atmosphere makes Earth's surface warmer Some relevant parameters and facts (see previous slide sets) (So/) 32 W m -2 is the average incoming solar
More informationIV. Atmospheric Science Section
EAPS 100 Planet Earth Lecture Topics Brief Outlines IV. Atmospheric Science Section 1. Introduction, Composition and Structure of the Atmosphere Learning objectives: Understand the basic characteristics
More informationPrentice Hall EARTH SCIENCE
Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 21 Climate 21.1 Factors That Affect Climate Factors That Affect Climate Latitude As latitude increases, the intensity of solar energy decreases. The
More informationExtremes of Weather and the Latest Climate Change Science. Prof. Richard Allan, Department of Meteorology University of Reading
Extremes of Weather and the Latest Climate Change Science Prof. Richard Allan, Department of Meteorology University of Reading Extreme weather climate change Recent extreme weather focusses debate on climate
More informationLecture 10: Climate Sensitivity and Feedback
Lecture 10: Climate Sensitivity and Feedback Human Activities Climate Sensitivity Climate Feedback 1 Climate Sensitivity and Feedback (from Earth s Climate: Past and Future) 2 Definition and Mathematic
More informationTopic # 12 How Climate Works
Topic # 12 How Climate Works A Primer on How the Energy Balance Drives Atmospheric & Oceanic Circulation, Natural Climatic Processes pp 63-68 in Class Notes How do we get energy from this........ to drive
More informationWinds and Currents in the Oceans
Winds and Currents in the Oceans Atmospheric Processes Density of air is controlled by temperature, pressure, and moisture content. 1. Warm air is less dense than cold air and moist air is less dense than
More informationPrentice Hall EARTH SCIENCE
Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 21 Climate 21.1 Factors That Affect Climate Factors That Affect Climate Latitude As latitude increases, the intensity of solar energy decreases. The
More informationChapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? About 10 km thick
Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds What is an atmosphere? Sources of Gas Losses of Gas Thermal Escape Earth s Atmosphere About 10 km thick Consists mostly of molecular
More informationThe Atmosphere. Importance of our. 4 Layers of the Atmosphere. Introduction to atmosphere, weather, and climate. What makes up the atmosphere?
The Atmosphere Introduction to atmosphere, weather, and climate Where is the atmosphere? Everywhere! Completely surrounds Earth February 20, 2010 What makes up the atmosphere? Argon Inert gas 1% Variable
More information- matter-energy interactions. - global radiation balance. Further Reading: Chapter 04 of the text book. Outline. - shortwave radiation balance
(1 of 12) Further Reading: Chapter 04 of the text book Outline - matter-energy interactions - shortwave radiation balance - longwave radiation balance - global radiation balance (2 of 12) Previously, we
More informationChapter 2 Solar and Infrared Radiation
Chapter 2 Solar and Infrared Radiation Chapter overview: Fluxes Energy transfer Seasonal and daily changes in radiation Surface radiation budget Fluxes Flux (F): The transfer of a quantity per unit area
More informationInsolation and Temperature variation. The Sun & Insolation. The Sun (cont.) The Sun
Insolation and Temperature variation Atmosphere: blanket of air surrounding earth Without our atmosphere: cold, quiet, cratered place Dynamic: currents and circulation cells June 23, 2008 Atmosphere important
More informationThe atmosphere: A general introduction Niels Woetmann Nielsen Danish Meteorological Institute
The atmosphere: A general introduction Niels Woetmann Nielsen Danish Meteorological Institute Facts about the atmosphere The atmosphere is kept in place on Earth by gravity The Earth-Atmosphere system
More information