The Tropical Atmosphere: Hurricane Incubator
|
|
- Juliet O’Connor’
- 5 years ago
- Views:
Transcription
1 The Tropical Atmosphere: Hurricane Incubator Images from journals published by the American Meteorological Society are copyright AMS and used with permission.
2 A One-Dimensional Description of the Tropical Atmosphere
3 Elements of Thermal Balance: Solar Radiation Luminosity: 3.9 x J s -1 = 6.4 x 10 7 Wm -2 at top of photosphere Mean distance from earth: 1.5 x m Flux density at mean radius of earth S 0 L 0 4π d 2 2 = 1370 Wm
4 Stefan-Boltzmann Equation: F =σt4 σ = Wm 2 K 4 Sun: T 4 = σ Wm T 6,000 K
5 Disposition of Solar Radiation: Total absorbed solar radiation = S 0 1 a p π r p 2 a p planetary albedo ( 30%) Total surface area = 4π r 2 p Absorption per unit area = S 0 1 a 4 p Absorption by clouds, atmosphere, and surface
6 Terrestrial Radiation: Effective emission temperature: σt 4 S 0 1 a e 4 p Earth: T = 255K = e 18 C Observed average surface temperature = 288 K = 15 C
7 Highly Reduced Model Transparent to solar radiation Opaque to infrared radiation Blackbody emission from surface and each layer
8 Radiative Equilibrium: Top of Atmosphere: S 4 σt = a = σt A 4 p e T A = T e Surface: σt s 4 = σt A 4 + S 1 4 T = 2 4 T s e 0 ( 1 a p ) = 2σT e 4 = 303 K
9 Surface temperature too large because: Real atmosphere is not opaque Heat transported by convection as well as by radiation
10 Extended Layer Models TOA : σt 2 4 = σt e 4 T 2 = T e Middle Layer : 2σT 1 4 = σt 2 4 +σt s 4 = σt e 4 +σt s 4 Surface : σt s 4 = σt e 4 +σt T s = 3 4 T e T 1 = 2 4 T e
11 Effects of emissivity<1 Surface : 2ε σt 4 = ε σ T 4 + ε σ T 4 A A A 1 A s ) 1 4 A e s T = ( 5 T 321K < T 2 Stratosphere : 2εσT 4 = ε σ T 4 t t A 2 ) 1 4 t e e T = ( 1 T 214K < T 2
12 Full calculation of radiative equilibrium:
13 Problems with radiative equilibrium solution: Too hot at and near surface Too cold at a near tropopause Lapse rate of temperature too large in the troposphere (But stratosphere temperature close to observed)
14 Missing ingredient: Convection As important as radiation in transporting enthalpy in the vertical Also controls distribution of water vapor and clouds, the two most important constituents in radiative transfer
15 When is a fluid unstable to convection? Pressure and hydrostatic equilibrium Buoyancy Stability
16 Hydrostatic equilibrium: Weight : gρδxδ yδz Pressure : pδ δ x y ( p +δ p ) δ xδ y F = MA: ρδx δy δ z dw = gρδxδyδ z δ pδxδy dt dw p 1 dt = g α z, α = = specific volume ρ
17 Pressure distribution in atmosphere at rest: RT R * Ideal gas : α =, R p m Hydrostatic : 1 p ln( p) g = = p z z RT Isothermal case : p = p e z H, H RT = "scale height " 0 g Earth: H~ 8 Km
18 Buoyancy: Weight g ρ δ x δy δz : b Pressure : pδxδ y ( p + δ p) δxδ y dw F = MA : ρ bδxδyδ z = gρ b δ xδyδ z δ pδxδ y dt dw p p = g α but = g b dt z z α e dw = g α b α e B dt α e
19 Buoyancy and Entropy Specific Volume: α = 1 ρ Specific Entropy: s α T Maxwell : α =α( ps, s = p p s B = g (δα ) α T = p δ s = δ s s p p s (δα ) p g T = δ s = α α p s T z s δ s Γ δ s
20 The adiabatic lapse rate: First Law of Thermodynamics : Q ds rev dt dα = T = c v + p dt dt dt dt d (α p) dp = c v + α dt dt dt = (c + R) dt α dp v dt dt = c dt α dp p dt dt Adiabatic : c p dt αdp = 0 Hydrostatic : c dt + gdz = 0 p ( dt dz) s = g cp Γ d
21 Γ= g c p Earth s atmosphere: Γ= 1 K 100 m
22 Model Aircraft Measurements (Renno and Williams, 1995)
23 Radiative equilibrium is unstable in the troposphere Re-calculate equilibrium assuming that tropospheric stability is rendered neutral by convection: Radiative-Convective Equilibrium
24 Better, but still too hot at surface, too cold at tropopause
25 Above a thin boundary layer, most atmospheric convection involved phase change of water: Moist Convection
26 Moist Convection Significant heating owing to phase changes of water Redistribution of water vapor most important greenhouse gas Significant contributor to stratiform cloudiness albedo and longwave trapping
27 Stability Assessment using Tephigrams: Pressure (mb) Temperature (C)
28 Stability Assessment using Tephigrams: Convective Available Potential Energy (CAPE): p CAPE i (α α i p n p e )dp p = i R d (T ρ T )d ln ( ) p p ρ e p
29 Tropical Soundings: Virtually no CAPE
30 Annual Mean Kapingamoronga
31 Tropical Cyclones: Steady State Physics. Where does the Energy Come From?
32
33 Angular momentum per unit mass M = rv + Ωsin (θ )r 2
34 Energy Production
35 Carnot Theorem: Maximum efficiency results from a particular energy cycle: Isothermal expansion Adiabatic expansion Isothermal compression Adiabatic compression Note: Last leg is not adiabatic in hurricane: Air cools radiatively. But since environmental temperature profile is moist adiabatic, the amount of radiative cooling is the same as if air were saturated and descending moist adiabatically. Maximum rate of working: Ts T W = o Q T s
36
37 Total rate of heat input to hurricane: Q = 2π 0 r 0 ρ C V (k * k ) + C V 3 rdr k 0 D Surface enthalpy flux Dissipative heating In steady state, Work is used to balance frictional dissipation: W = 2π 0 r 0 ρ C D V 3 rdr
38 0 Plug into Carnot equation: r 0 T T ρ V 3 s rdr = r o 0 C ρ C ( * D k V k 0 k) rdr T o 0 If integrals dominated by values of integrands near radius of maximum winds, 2 C k T s T o ( * V k max 0 k ) C D T o
39 Graph of Solution for particular values of coefficients:
40
41
42
43 00 GMT 21 March o N 20 o N 0 o 20 o S 40 o S 0 o 60 o E 120 o E 180 o W 120 o W 60 o W 0 o
44 Numerical simulations
45 Relationship between potential intensity (PI) and intensity of real tropical cyclones
46
47
48 Wind speed (m/s) Potential wind speed (m/s) V (m/s) Time after maximum intensity (hours) 100
49 Evolution with respect to time of maximum intensity
50 Evolution with respect to time of maximum intensity, normalized by peak wind
51 Evolution curve of Atlantic storms whose lifetime maximum intensity is limited by declining potential intensity, but not by landfall
52 Evolution curve of WPAC storms whose lifetime maximum intensity is limited by declining potential intensity, but not by landfall
53 CDF of normalized lifetime maximum wind speeds of North Atlantic tropical cyclones of tropical storm strength (18 m s 1) or greater, for those storms whose lifetime maximum intensity was limited by landfall.
54 CDF of normalized lifetime maximum wind speeds of Northwest Pacific tropical cyclones of tropical storm strength (18 m s 1) or greater, for those storms whose lifetime maximum intensity was limited by landfall.
55 Evolution of Atlantic storms whose lifetime maximum intensity was limited by landfall
56 Evolution of Pacific storms whose lifetime maximum intensity was limited by landfall
57 Composite evolution of landfalling storms
58 MIT OpenCourseWare Science and Policy of Natural Hazards Spring 2010 For information about citing these materials or our Terms of Use, visit:
Radiative Transfer Chapter 3, Hartmann
Radiative Transfer Chapter 3, Hartmann Shortwave Absorption: Clouds, H 2 0, O 3, some CO 2 Shortwave Reflection: Clouds, surface, atmosphere Longwave Absorption: Clouds, H 2 0, CO 2, CH 4, N 2 O Planck
More informationBrief Overview of the Global Atmosphere
Brief Overview of the Global Atmosphere Images on pages 3, 5 through 9, 19, 77 through 80 and 90 are copyrighted by Academic Press, NY, 1999. The images are in a chapter entitled "Quasi-equilibrium thinking"
More informationTropical Cyclones: Steady State Physics
Tropical Cyclones: Steady State Physics Energy Production Carnot Theorem: Maximum efficiency results from a particular energy cycle: Isothermal expansion Adiabatic expansion Isothermal compression Adiabatic
More informationAdiabatic expansion Isothermal compression Adiabatic compression
Tropical Cyclones: Steady State Physics 1 Energy Production 2 Carnot Theorem: Maximum efficiency results from a pa rticular energy e cycle: Isothermal expansion Adiabatic expansion Isothermal compression
More informationLecture 3: Convective Heat Transfer I
Lecture 3: Convective Heat Transfer I Kerry Emanuel; notes by Paige Martin and Daniel Mukiibi June 18 1 Introduction In the first lecture, we discussed radiative transfer in the climate system. Here, we
More informationRadiative equilibrium Some thermodynamics review Radiative-convective equilibrium. Goal: Develop a 1D description of the [tropical] atmosphere
Radiative equilibrium Some thermodynamics review Radiative-convective equilibrium Goal: Develop a 1D description of the [tropical] atmosphere Vertical temperature profile Total atmospheric mass: ~5.15x10
More informationRadiative-Convective Instability. Kerry Emanuel Massachusetts Institute of Technology
Radiative-Convective Instability Kerry Emanuel Massachusetts Institute of Technology Program Basic radiative-convective equilibrium Macro-instability of the RC state Some consequences Radiative Equilibrium
More informationProject 3 Convection and Atmospheric Thermodynamics
12.818 Project 3 Convection and Atmospheric Thermodynamics Lodovica Illari 1 Background The Earth is bathed in radiation from the Sun whose intensity peaks in the visible. In order to maintain energy balance
More informationRadiative Equilibrium Models. Solar radiation reflected by the earth back to space. Solar radiation absorbed by the earth
I. The arth as a Whole (Atmosphere and Surface Treated as One Layer) Longwave infrared (LWIR) radiation earth to space by the earth back to space Incoming solar radiation Top of the Solar radiation absorbed
More informationAnnual Number of Peer Reviewed Articles with Hurricane or Tropical Cyclone in their Titles, according to Meteorological and Geoastrophysical
Hurricanes and Climate Kerry Emanuel Program in Atmospheres, Oceans, and Climate MIT Program Potential Intensity Role of potential ti li intensity it in storm intensity it Role of potential intensity in
More informationHurricanes are intense vortical (rotational) storms that develop over the tropical oceans in regions of very warm surface water.
Hurricanes: Observations and Dynamics Houze Section 10.1. Holton Section 9.7. Emanuel, K. A., 1988: Toward a general theory of hurricanes. American Scientist, 76, 371-379 (web link). http://ww2010.atmos.uiuc.edu/(gh)/guides/mtr/hurr/home.rxml
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 informationPlanetary Atmospheres
Planetary Atmospheres Structure Composition Clouds Meteorology Photochemistry Atmospheric Escape EAS 4803/8803 - CP 17:1 Structure Generalized Hydrostatic Equilibrium P( z) = P( 0)e z # ( ) " dr / H r
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 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 informationPlanetary Atmospheres
Planetary Atmospheres Structure Composition Clouds Meteorology Photochemistry Atmospheric Escape EAS 4803/8803 - CP 11:1 Structure Generalized Hydrostatic Equilibrium P( z) = P( 0)e z # ( ) " dr / H r
More information1. The vertical structure of the atmosphere. Temperature profile.
Lecture 4. The structure of the atmosphere. Air in motion. Objectives: 1. The vertical structure of the atmosphere. Temperature profile. 2. Temperature in the lower atmosphere: dry adiabatic lapse rate.
More information1) The energy balance at the TOA is: 4 (1 α) = σt (1 0.3) = ( ) 4. (1 α) 4σ = ( S 0 = 255 T 1
EAS488/B8800 Climate & Climate Change Homework 2: Atmospheric Radiation and Climate, surface energy balance, and atmospheric general circulation Posted: 3/12/18; due: 3/26/18 Answer keys 1. (10 points)
More informationAtmospheric Thermodynamics
Atmospheric Thermodynamics R. Wordsworth February 12, 2015 1 Objectives Derive hydrostatic equation Derive dry and moist adiabats Understand how the theory relates to observed properties of real atmospheres
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 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 informationEnergy 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 information4. Atmospheric transport. Daniel J. Jacob, Atmospheric Chemistry, Harvard University, Spring 2017
4. Atmospheric transport Daniel J. Jacob, Atmospheric Chemistry, Harvard University, Spring 2017 Forces in the atmosphere: Gravity g Pressure-gradient ap = ( 1/ ρ ) dp / dx for x-direction (also y, z directions)
More informationThermodynamics Review [?] Entropy & thermodynamic potentials Hydrostatic equilibrium & buoyancy Stability [dry & moist adiabatic]
Thermodynamics Review [?] Entropy & thermodynamic potentials Hydrostatic equilibrium & buoyancy Stability [dry & moist adiabatic] Entropy 1. (Thermodynamics) a thermodynamic quantity that changes in a
More informationSpectrum 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 informationLecture 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 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 informationHurricanes: Their physics and relationship to climate. Kerry Emanuel Massachusetts Institute of Technology
Hurricanes: Their physics and relationship to climate Kerry Emanuel Massachusetts Institute of Technology Topics Overview of Tropical Cyclones Tropical Cyclone Physics What have TCs been like in the past,
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 information1 Thermodynamics: some Preliminaries
1 Thermodynamics: some Preliminaries Beforewebegintoconsider thetransfer ofradiation through an atmosphere, let s consider the structure of an atmosphere with a little thermodynamics. This material hopefully
More informationLecture 4: Global Energy Balance
Lecture : Global Energy Balance S/ * (1-A) T A T S T A Blackbody Radiation Layer Model Greenhouse Effect Global Energy Balance terrestrial radiation cooling Solar radiation warming Global Temperature atmosphere
More informationLecture 4: Global Energy Balance. Global Energy Balance. Solar Flux and Flux Density. Blackbody Radiation Layer Model.
Lecture : Global Energy Balance Global Energy Balance S/ * (1-A) terrestrial radiation cooling Solar radiation warming T S Global Temperature Blackbody Radiation ocean land Layer Model energy, water, and
More informationOutline. Stock Flow and temperature. Earth as a black body. Equation models for earth s temperature. Balancing earth s energy flows.
Outline Stock Flow and temperature Earth as a black body Equation models for earth s temperature { { Albedo effect Greenhouse effect Balancing earth s energy flows Exam questions How does earth maintain
More informationDynamics and Kinematics
Geophysics Fluid Dynamics () Syllabus Course Time Lectures: Tu, Th 09:30-10:50 Discussion: 3315 Croul Hall Text Book J. R. Holton, "An introduction to Dynamic Meteorology", Academic Press (Ch. 1, 2, 3,
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 informationPresentation A simple model of multiple climate regimes
A simple model of multiple climate regimes Kerry Emanuel March 21, 2012 Overview 1. Introduction 2. Essential Climate Feedback Processes Ocean s Thermohaline Circulation, Large-Scale Circulation of the
More informationFriday 8 September, :00-4:00 Class#05
Friday 8 September, 2017 3:00-4:00 Class#05 Topics for the hour Global Energy Budget, schematic view Solar Radiation Blackbody Radiation http://www2.gi.alaska.edu/~bhatt/teaching/atm694.fall2017/ notes.html
More informationdf dz = dp dt Essentially, this is just a statement of the first law in one of the forms we derived earlier (expressed here in W m 3 ) dq p dt dp
A problem with using entropy as a variable is that it is not a particularly intuitive concept. The mechanics of using entropy for evaluating system evolution is well developed, but it sometimes feels a
More informationRadiative-Convective Instability
Radiative-Convective Instability Kerry Emanuel, Allison Wing, and Emmanuel Vincent Massachusetts Institute of Technology Self-Aggregation of Deep Moist Convection Cloud Clusters Tropical Cyclone Genesis
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 informationEART164: PLANETARY ATMOSPHERES
EART16: PLANETARY ATMOSPHERES Francis Nimmo Last Week How do planets form? They accrete from the solar nebula (dust+gas) They may subsequently migrate Where do atmospheres come from? Primary, secondary,
More informationGeophysics Fluid Dynamics (ESS228)
Geophysics Fluid Dynamics (ESS228) Course Time Lectures: Tu, Th 09:30-10:50 Discussion: 3315 Croul Hall Text Book J. R. Holton, "An introduction to Dynamic Meteorology", Academic Press (Ch. 1, 2, 3, 4,
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 informationATMO 551a Fall The Carnot Cycle
What is a arnot ycle and Why do we care The arnot ycle arnot was a French engineer who was trying to understand how to extract usable mechanical work from a heat engine, that is an engine where a gas or
More informationAtmosphere, Ocean and Climate Dynamics Fall 2008
MIT OpenCourseWare http://ocw.mit.edu 12.003 Atmosphere, Ocean and Climate Dynamics Fall 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. Contents
More informationDynamics of the Zonal-Mean, Time-Mean Tropical Circulation
Dynamics of the Zonal-Mean, Time-Mean Tropical Circulation First consider a hypothetical planet like Earth, but with no continents and no seasons and for which the only friction acting on the atmosphere
More informationMeteorology 6150 Cloud System Modeling
Meteorology 6150 Cloud System Modeling Steve Krueger Spring 2009 1 Fundamental Equations 1.1 The Basic Equations 1.1.1 Equation of motion The movement of air in the atmosphere is governed by Newton s Second
More informationHurricane Science Tutorial. Kerry Emanuel Lorenz Center, MIT
Hurricane Science Tutorial Kerry Emanuel Lorenz Center, MIT Why Should You Care? Forecasting Much progress in social science of response to warnings, requests to evacuate, etc. Forecasters are ambassadors
More informationLecture # 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 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 informationATMS 321: Sci. of Climate Final Examination Study Guide Page 1 of 4
ATMS 321: Sci. of Climate Final Examination Study Guide Page 1 of 4 Atmospheric Sciences 321: Final Examination Study Guide The final examination will consist of similar questions Science of Climate Multiple
More informationGlobal Energy Balance: Greenhouse Effect
Global Energy Balance: Greenhouse Effect Atmospheric Composition & Structure Physical Causes of Greenhouse Effects Chapter 3: 44 48. Atmospheric Composition Why does water vapor vary so much? Saturation
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 informationFundamentals of Weather and Climate
Fundamentals of Weather and Climate ROBIN McILVEEN Environmental Science Division Institute of Environmental and Biological Sciences Lancaster University CHAPMAN & HALL London Glasgow Weinheim New York
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 informationLecture 11: Meridonal structure of the atmosphere
Lecture 11: Meridonal structure of the atmosphere September 28, 2003 1 Meridional structure of the atmosphere In previous lectures we have focussed on the vertical structure of the atmosphere. Today, we
More informationTropical Meteorology. Kerry Emanuel Program in Atmospheres, Oceans, and Climate Massachusetts Institute of Technology Cambridge, MA 02139, USA
Tropical Meteorology Kerry Emanuel Program in Atmospheres, Oceans, and Climate Massachusetts Institute of Technology Cambridge, MA 02139, USA October 5, 1999 Introduction 1 Radiative-Convective Equilibrium
More informationQuasi-equilibrium Theory of Small Perturbations to Radiative- Convective Equilibrium States
Quasi-equilibrium Theory of Small Perturbations to Radiative- Convective Equilibrium States See CalTech 2005 paper on course web site Free troposphere assumed to have moist adiabatic lapse rate (s* does
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 informationPhysical Fundamentals of Global Change Processes
University of Applied Sciences Eberswalde Master Study Program Global Change Management Manfred Stock Potsdam Institute for Climate Impact Research Module: Physical Fundamentals of Global Change Processes
More informationToday s Lecture: Atmosphere finish primitive equations, mostly thermodynamics
Today s Lecture: Atmosphere finish primitive equations, mostly thermodynamics Reference Peixoto and Oort, Sec. 3.1, 3.2, 3.4, 3.5 (but skip the discussion of oceans until next week); Ch. 10 Thermodynamic
More information2. Meridional atmospheric structure; heat and water transport. Recall that the most primitive equilibrium climate model can be written
2. Meridional atmospheric structure; heat and water transport The equator-to-pole temperature difference DT was stronger during the last glacial maximum, with polar temperatures down by at least twice
More informationMon Oct 20. Today: radiation and temperature (cont) sun-earth geometry energy balance >> conceptual model of climate change Tues:
Mon Oct 20 Announcements: bring calculator to class from now on > in-class activities > midterm and final Today: radiation and temperature (cont) sun-earth geometry energy balance >> conceptual model of
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 information2. Illustration of Atmospheric Greenhouse Effect with Simple Models
2. Illustration of Atmospheric Greenhouse Effect with Simple Models In the first lecture, I introduced the concept of global energy balance and talked about the greenhouse effect. Today we will address
More informationOverview of fundamental atmospheric concepts
Fundamentals of Earth s Atmosphere AOSC 433/633 & CHEM 433/633 Tim Canty Class Web Site: http://www.atmos.umd.edu/~rjs/class/spr2013 Notes: Ross, Tim, & Allison co-teach this class; please include all
More informationClimate Dynamics (PCC 587): Clouds and Feedbacks
Climate Dynamics (PCC 587): Clouds and Feedbacks D A R G A N M. W. F R I E R S O N U N I V E R S I T Y O F W A S H I N G T O N, D E P A R T M E N T O F A T M O S P H E R I C S C I E N C E S D A Y 7 : 1
More informationHand in Question sheets with answer booklets Calculators allowed Mobile telephones or other devices not allowed
York University Department of Earth and Space Science and Engineering ESSE 3030 Department of Physics and Astronomy PHYS 3080 Atmospheric Radiation and Thermodynamics Final Examination 2:00 PM 11 December
More informationGreenhouse Effect & Venusian Atmospheric Balance. Evan Anders
Greenhouse Effect & Venusian Atmospheric Balance Evan Anders Greenhouse Effect Strong absorption bands of gases and aerosols trap the heat in the lower atmosphere...raising the surface temperature High
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 informationLecture 2: Global Energy Cycle
Lecture 2: Global Energy Cycle Planetary energy balance Greenhouse Effect Selective absorption Vertical energy balance Solar Flux and Flux Density Solar Luminosity (L) the constant flux of energy put out
More informationSolar Flux and Flux Density. Lecture 2: Global Energy Cycle. Solar Energy Incident On the Earth. Solar Flux Density Reaching Earth
Lecture 2: Global Energy Cycle Solar Flux and Flux Density Planetary energy balance Greenhouse Effect Selective absorption Vertical energy balance Solar Luminosity (L) the constant flux of energy put out
More informationHabitable Planets. Much of it stolen from. Yutaka ABE University of Tokyo
Habitable Planets Much of it stolen from Yutaka ABE University of Tokyo 1. Habitability and Water Why water? Importance of Liquid Gas: highly mobile, but low material density. Solid: high density but very
More informationStefan-Boltzmann law for the Earth as a black body (or perfect radiator) gives:
2. Derivation of IPCC expression ΔF = 5.35 ln (C/C 0 ) 2.1 Derivation One The assumptions we will make allow us to represent the real atmosphere. This remarkably reasonable representation of the real atmosphere
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: 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 information1. Runaway Greenhouse
1. Runaway Greenhouse Making the simple complicated is commonplace; making the complicated simple, awesomely simple, that s creativity. - Charlie Mingus (Jazz Musician) Initially we assume that the radiative
More informationEnergy, 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 informationMASSACHUSETTS 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 informationClimate vs Weather J. J. Hack/A. Gettelman: June 2005
Climate vs Weather J. J. Hack/A. Gettelman: June 2005 What is Climate? J. J. Hack/A. Gettelman: June 2005 Characterizing Climate Climate change and its manifestation in terms of weather (climate extremes)
More information1. Radiative Transfer. 2. Spectrum of Radiation. 3. Definitions
1. Radiative Transfer Virtually all the exchanges of energy between the earth-atmosphere system and the rest of the universe take place by radiative transfer. The earth and its atmosphere are constantly
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 informationData and formulas at the end. Real exam is Wednesday May 8, 2002
ATMS 31: Physical Climatology Practice Mid Term Exam - Spring 001 page 1 Atmospheric Sciences 31 Physical Climatology Practice Mid-Term Examination: Would be Closed Book Data and formulas at the end. Real
More informationRadiation in the atmosphere
Radiation in the atmosphere Flux and intensity Blackbody radiation in a nutshell Solar constant Interaction of radiation with matter Absorption of solar radiation Scattering Radiative transfer Irradiance
More informationClouds and turbulent moist convection
Clouds and turbulent moist convection Lecture 2: Cloud formation and Physics Caroline Muller Les Houches summer school Lectures Outline : Cloud fundamentals - global distribution, types, visualization
More informationClimate Dynamics (PCC 587): Feedbacks & Clouds
Climate Dynamics (PCC 587): Feedbacks & Clouds DARGAN M. W. FRIERSON UNIVERSITY OF WASHINGTON, DEPARTMENT OF ATMOSPHERIC SCIENCES DAY 6: 10-14-13 Feedbacks Climate forcings change global temperatures directly
More informationComposition, Structure and Energy. ATS 351 Lecture 2 September 14, 2009
Composition, Structure and Energy ATS 351 Lecture 2 September 14, 2009 Composition of the Atmosphere Atmospheric Properties Temperature Pressure Wind Moisture (i.e. water vapor) Density Temperature A measure
More informationInner core dynamics: Eyewall Replacement and hot towers
Inner core dynamics: Eyewall Replacement and hot towers FIU Undergraduate Hurricane Internship Lecture 4 8/13/2012 Why inner core dynamics is important? Current TC intensity and structure forecasts contain
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 informationLecture 3a: Surface Energy Balance
Lecture 3a: Surface Energy Balance Instructor: Prof. Johnny Luo http://www.sci.ccny.cuny.edu/~luo Surface Energy Balance 1. Factors affecting surface energy balance 2. Surface heat storage 3. Surface
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 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 informationdi λ ds = ρk λi λ B λ (T ) + ρk λ dz' )= B λ (T(z'))e I λ (z TOA + k λ Longwave radiative transfer Longwave radiative transfer
Radiative transfer applied to the atmosphere: Longwave radiation z In the longwave spectrum (> µm) we have to take into account both absorption and emission, as the atmosphere and Earth surface with temperatures
More informationAtmospheric Circulation
Atmospheric Circulation (WAPE: General Circulation of the Atmosphere and Variability) François Lott, flott@lmd.ens.fr http://web.lmd.jussieu.fr/~flott 1) Mean climatologies and equations of motion a)thermal,
More informationFundamentals of Earth s Atmosphere. AOSC 434/658R & CHEM 434/678A Tim Canty
Fundamentals of Earth s Atmosphere AOSC 434/658R & CHEM 434/678A Tim Canty Class Web Site: http://www.atmos.umd.edu/~rjs/class/spr2011 Notes: Please include both Ross and Tim on any class related email
More informationLecture 3a: Surface Energy Balance
Lecture 3a: Surface Energy Balance Instructor: Prof. Johnny Luo http://www.sci.ccny.cuny.edu/~luo Total: 50 pts Absorption of IR radiation O 3 band ~ 9.6 µm Vibration-rotation interaction of CO 2 ~
More informationUNIVERSITY OF SOUTHAMPTON
UNIVERSITY OF SOUTHAMPTON PHYS1013W1 SEMESTER 2 EXAMINATION 2014-2015 ENERGY AND MATTER Duration: 120 MINS (2 hours) This paper contains 8 questions. Answers to Section A and Section B must be in separate
More informationGlobal Energy and Water Budgets
Global Energy and Water Budgets 1 40 10 30 Pressure (hpa) 100 Pure radiative equilibrium Dry adiabatic adjustment 20 Altitude (km) 6.5 C/km adjustment 10 1000 0 180 220 260 300 340 Temperature (K)
More informationFinal Examination. Part A Answer ONLY TWELVE QUESTIONS in Part A. (Each question is 3 points)
ATS 210 Spring Term 2001 NAME: Final Examination This is a 2 hour, closed-book examination. Calculators may be used. All answers should be written on the examination paper. Use the final sheet for any
More informationData and formulas at the end. Exam would be Weds. May 8, 2008
ATMS 321: Science of Climate Practice Mid Term Exam - Spring 2008 page 1 Atmospheric Sciences 321 Science of Climate Practice Mid-Term Examination: Would be Closed Book Data and formulas at the end. Exam
More information