Patterns in the CERES Global Mean Data, Part 3
|
|
- Herbert Lucas
- 5 years ago
- Views:
Transcription
1 Patterns in the CERES Global Mean Data, Part Wild et al Total Solar Irradiance, Albedo, and Cloud Radiative Effects Miklos Zagoni 31 st CERES Science Team Meeting, May 7 9, 2019, Hampton, VA Instead of the traditional paradigm of properties define processes, study how processes define property Graeme Stephens
2 CERES SYN1deg Ed4A Clear-sky, 2000 Oct 2018 Sept SFC SW down = SFC SW up = SFC SW in = SFC LW in = E(SFC) = SW in + LW in = TOA LW = (TOA LW) = Diff = E(SFC) 2 (TOA LW) = 4.3 Wm -2 TOA Net, unadjusted = 4.3 Wm -2
3 Net balancing SW gain = 1.7 LW gain = 2.5 My best: SFC SW in = = SFC LW in = = E (SW + LW in) = = TOA LW = = TOA LW = = Diff = 4.28 = 0.0
4 CERES SYN1deg Ed4A Clear-sky, 2000 Oct 2018 Sep My best: SFC SW + LW net = = TOA LW = = (TOA LW)/ 2 = = Diff = 0.7 = 0.0
5 CERES SYN1deg Ed4A All-sky, 2000 Oct 2018 Sep E(SFC, SW + LW in) = TOA LW = LWCRE = (TOA LW) + LWCRE = Diff = 2.16
6 CERES EBAF Ed2.8 Clear-sky, CLIM YEAR SFC SW in = SFC LW in = E(SFC, SW + LW in) = TOA LW = x (TOA LW) = DIFF = 2(TOA LW) E(SFC, in) = 0.38 Wm -2
7 CERES EBAF Ed2.8 Clear-sky, CLIM YEAR SH+LH (SW + LW Net) = TOA LW = (TOA LW)/ 2 = DIFF = 0.49 Wm -2 G (SFC LW Up TOA LW) = G = TOA LW = DIFF = 0.20 Wm -2
8 CERES EBAF Ed2.8 All-sky, CLIM YEAR SFC SW in = SFC LW in = E(SFC, in) = TOA LW = (TOA LW) = SFC LWCRE = (TOA LW) + SFC LWCRE = DIFF = 0.42 Wm -2
9 CERES EBAF Ed4.0 Clear-sky, CLIM YEAR SFC SW in = SFC LW in = E(SFC, SW + LW in) = TOA LW = (TOA LW) = DIFF = 8.08 Wm -2
10 CERES EBAF Ed4.0 Clear-sky, CLIM YEAR SH+LH (SFC SW + LW Net) = G (SFC LW Up TOA LW) = DIFF = 0.84
11 CERES EBAF Ed4.0 All-sky, CLIM YEAR SFC SW in = = SFC LW in = = E(SFC, SW + LW in) = = TOA LW = = (TOA LW) = = SFC LWCRE = = (TOA LW) + LWCRE = = DIFF = 1.75
12 Why is this important? Mars: E(SFC) << 2OLR Venus: E(SFC) >> 2OLR Earth: E(SFC, clear) = 2OLR(clear) Earth: E(SFC, all) = 2OLR(all) + LWCRE
13 Why is this soooo important? Mars: E(SFC) << 2OLR E(SFC) = (SW + LW) in = 123 Wm -2 2OLR = 2 110; WIN = 97 Wm -2 ; E(SFC) = 2OLR WIN No clouds, leaky greenhouse: WIN is lost without compensation Venus: E(SFC) >> 2OLR E(SFC) = 2OLR + k SFC LWCRE Multiple-closed cloud layers, WIN = 0 Earth: E(SFC, clear) = 2OLR(clear) = Wm -2 E(SFC, clear) = 2ASR(clear) WIN(clear) + LWCRE E(SFC, clear) = EXACT! Earth: E(SFC, all) = 2OLR(all) + LWCRE Leaky greenhouse + partial cloud cover: Atmospheric window closed by the blanketing effect of clouds
14 = 66 W m -2 g
15 Mars: WIN is lost without compensation OLR = WIN + ATM
16 Earth: WIN is closed by LWCRE Effectively closed shell, number of free paths:τ = 2
17 Schwarzschild E. A. Milne (1922) Radiative equilibrium: the insolation of an atmospehere. Phil Mag 44
18 Some simplifications do not hold well, still Inner boundary : Effective temp : Outer boundary = SFC LW up : OLR : ATM LW up = 3/2 : 1 : 3/4
19 SFC Temp Discontinuity = OLR/2 Goody and Yung (1989) independent of τ
20 Goody s greenhouse solution for atmospheres in radiative equilibrium With = 2 we have Discontinuity at the groud = OLR/2
21 Temp discontinuity at the ground = OLR/2 (= convective flux) E(SFC, τ = 2) = 2OLR
22 SYN1deg and EBAF got it right. There is a set of constraints. For some reason, Earth works on that limiting state. SW + LW net = OLR/2 E(SFC) = 2 OLR ULW = 3 OLR/2 ATM = 3 OLR/4 WIN G = OLR/4 = OLR/2
23 Exxxact! Clear-sky: WIN G SW + LW net ATM LW up TOA LW SFC LW up E(SFC) SW + LW in (TOA LW)
24 g ATM LW up = 3OLR/4 = OLR WIN = OLR/4 SFC LW up = 3OLR/2 SH+LH = OLR/2 E(SFC) = 2OLR
25 Direct consequence Below clouds: cavity Waves in a cavity: quantized F = N UNIT UNIT: the smallest flux component: LWCRE UNIT = LWCRE = TSI/51 = / 51 = Wm -2
26 Wave propagation in a closed box: F = N UNIT, N = 1, 2, 3, 4, 5,
27 Earth s energy flows: quantized, N is related to Total Solar Irradiance TSI = 51 Diff Wm-2 LWCRE = 1 Incoming Solar Radiation = 51/4 0.0 TOA SW Up (all) = 15/4 0.8 ASR(all) = OLR(all) = 36/4 0.0 TOA SW Up (clear) = 8/4 0.0 ASR(clear) = 43/4 0.0 OLR(clear) = 40/4 1.3 WIN(clear) = 10/4 0.2 LWQ = 28/4 0.2 SFC SW down (clear) = 37/4 0.2 SFC SW up (clear) = 5/4 0.3 Planetary albedo = 5/17 = SFC albedo = 5/37 = Exact!
28 LWQ 183 Wild et al. 2015
29 Surface observations justify Wild et al. 2018
30 The complete solution TSI = 51 Wild et al. 2018
Patterns in the CERES Global Mean Data, Part 3. Cloud Area Fraction, Atmospheric Energy Budgets, DLR Update. Miklos Zagoni
Patterns in the CERES Global Mean Data, Part 3. Cloud Area Fraction, Atmospheric Energy Budgets, DLR Update β eff eff = β obs ε obs ε IR IR Miklos Zagoni miklos.zagoni@t-online.hu 2018 Earth Radiation
More informationPatterns in the CERES Global Mean Data
Patterns in the CERES Global Mean Data Miklos Zagoni Fall 2017 CERES Science Team Meeting, September 27, NASA GSFC, Greenbelt, MD. "To search for something though it be mushrooms or some pattern is impossible,
More informationDeducing Earth s Global Energy Flows from a Simple Greenhouse Model
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 Article Deducing Earth s Global Energy Flows from a Simple Greenhouse Model
More informationInterannual variability of top-ofatmosphere. CERES instruments
Interannual variability of top-ofatmosphere albedo observed by CERES instruments Seiji Kato NASA Langley Research Center Hampton, VA SORCE Science team meeting, Sedona, Arizona, Sep. 13-16, 2011 TOA irradiance
More informationA new diagram of Earth s global energy budget
Acta Geod Geophys (2016) 51:481 492 DOI 10.1007/s40328-015-0138-0 A new diagram of Earth s global energy budget Miklos Zagoni 1 Received: 26 November 2014 / Accepted: 23 July 2015 / Published online: 19
More informationHistory of Earth Radiation Budget Measurements With results from a recent assessment
History of Earth Radiation Budget Measurements With results from a recent assessment Ehrhard Raschke and Stefan Kinne Institute of Meteorology, University Hamburg MPI Meteorology, Hamburg, Germany Centenary
More informationSeeking a consistent view of energy and water flows through the climate system
Seeking a consistent view of energy and water flows through the climate system Robert Pincus University of Colorado and NOAA/Earth System Research Lab Atmospheric Energy Balance [Wm -2 ] 340.1±0.1 97-101
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 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 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 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: 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 informationVariability in Global Top-of-Atmosphere Shortwave Radiation Between 2000 And 2005
Variability in Global Top-of-Atmosphere Shortwave Radiation Between 2000 And 2005 Norman G. Loeb NASA Langley Research Center Hampton, VA Collaborators: B.A. Wielicki, F.G. Rose, D.R. Doelling February
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 informationand Atmospheric Science, University of Miami, 4600 Rickenbacker Causeway, Miami, FL 33149, USA.
Observed changes in top-of-the-atmosphere radiation and upper-ocean heating consistent within uncertainty. Steady accumulation of heat by Earth since 2000 according to satellite and ocean data Norman G.
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 informationIs the Earth s climate system constrained?*+
Is the Earth s climate system constrained?*+ Graeme Stephens, Denis O Brien, Peter Webster,Peter Pilewskie,Seiji Kato,Juilin Li *Stephens et al., 2014;The albedo of Earth, Rev Geophys, + Stephens and L
More informationConstraints on the Interannual Variation of Global and Regional Topof-Atmosphere. Inferred from MISR Measurements. Roger Davies
Constraints on the Interannual Variation of Global and Regional Topof-Atmosphere Radiation Budgets Inferred from MISR Measurements Roger Davies Physics Department University of Auckland Background: basic
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 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 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 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 informationChanges in Earth s Albedo Measured by satellite
Changes in Earth s Albedo Measured by satellite Bruce A. Wielicki, Takmeng Wong, Norman Loeb, Patrick Minnis, Kory Priestley, Robert Kandel Presented by Yunsoo Choi Earth s albedo Earth s albedo The climate
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 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 informationClimate Dynamics Simple Climate Models
Climate Dynamics Simple Climate Models John Shepherd School of Ocean & Earth Science Southampton Oceanography Centre 1) Basic facts and findings Overview : 4 Lectures The global energy balance Zero-dimensional
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 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 informationSolar Insolation and Earth Radiation Budget Measurements
Week 13: November 19-23 Solar Insolation and Earth Radiation Budget Measurements Topics: 1. Daily solar insolation calculations 2. Orbital variations effect on insolation 3. Total solar irradiance measurements
More informationAerosol Radiative Forcing DEPARTMENT OF PHYSICS The AeroCom Prescribed Experiment: Towards the Quantification of Host Model Errors
Aerosol Radiative Forcing DEPARTMENT OF PHYSICS The AeroCom Prescribed Experiment: Towards the Quantification of Host Model Errors AeroCom Meeting, Reykjavik, Island 10/10/2008 Philip Stier Atmospheric,
More informationMon 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 informationInfluence of Clouds and Aerosols on the Earth s Radiation Budget Using Clouds and the Earth s Radiant Energy System (CERES) Measurements
Influence of Clouds and Aerosols on the Earth s Radiation Budget Using Clouds and the Earth s Radiant Energy System (CERES) Measurements Norman G. Loeb Hampton University/NASA Langley Research Center Bruce
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 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 informationHeat, temperature and gravity Emil Junvik
Heat, temperature and gravity Emil Junvik emil.junvik@gmail.com 018-03-17 Abstract A simple analysis of planetary temperatures and the relationship between heat flow and gravity in spherical shells. It
More informationHow good are our models?
direct Estimates of regional and global forcing: ^ How good are our models? Bill Collins with Andrew Conley, David Fillmore, and Phil Rasch National Center for Atmospheric Research Boulder, Colorado Models
More informationDo climate models over-estimate cloud feedbacks?
Do climate models over-estimate cloud feedbacks? Sandrine Bony CNRS, LMD/IPSL, Paris with contributions from Jessica Vial (LMD), David Coppin (LMD) Florent Brient (ETH), Tobias Becker (MPI), Kevin Reed
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 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 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 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 informationP607 Climate and Energy (Dr. H. Coe)
P607 Climate and Energy (Dr. H. Coe) Syllabus: The composition of the atmosphere and the atmospheric energy balance; Radiative balance in the atmosphere; Energy flow in the biosphere, atmosphere and ocean;
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 informationThe Cryosphere Radiative Effect in CESM. Justin Perket Mark Flanner CESM Polar Climate Working Group Meeting Wednesday June 19, 2013
The Cryosphere Radiative Effect in CESM Justin Perket Mark Flanner CESM Polar Climate Working Group Meeting Wednesday June 19, 2013 Cryosphere Radiative Effect (CrRE) A new diagnostic feature is available
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 informationComplexity of the climate system: the problem of the time scales. Climate models and planetary habitability
Complexity of the climate system: the problem of the time scales Climate models and planetary habitability Time scales of different components of the climate system Planets and Astrobiology (2016-2017)
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 informationMonday 9 September, :30-11:30 Class#03
Monday 9 September, 2013 10:30-11:30 Class#03 Topics for the hour Solar zenith angle & relationship to albedo Blackbody spectra Stefan-Boltzman Relationship Layer model of atmosphere OLR, Outgoing longwave
More informationIDŐJÁRÁS Quarterly Journal of the Hungarian Meteorological Service Vol. 111, No. 1, January March 2007, pp. 1 40
IDŐJÁRÁS Quarterly Journal of the Hungarian Meteorological Service Vol. 111, No. 1, January March 27, pp. 1 4 Greenhouse effect in semi-transparent planetary atmospheres Ferenc M. Miskolczi Holston Lane
More information9.4. The newly released 5-year Terra-based monthly CERES radiative flux and cloud product. David R. Doelling, D. F. Keyes AS&M, Inc.
9.4 The newly released 5-year Terra-based monthly CERES radiative flux and cloud product David R. Doelling, D. F. Keyes AS&M, Inc., Hampton, VA D. F. Young, B. A. Wielicki, T. Wong NASA Langley Research
More informationVery Dynamic! Energy in the Earth s Atmosphere. How Does it Get Here? All Objects Radiate Energy!
Energy in the Earth s Atmosphere Unit Essential Question: What are the different features of the atmosphere that characterize our weather. How does the atmosphere influence life and how does life influence
More informationTake away concepts. What is Energy? Solar Radiation Emission and Absorption. Energy: The ability to do work
Solar Radiation Emission and Absorption Take away concepts 1. 2. 3. 4. 5. 6. Conservation of energy. Black body radiation principle Emission wavelength and temperature (Wien s Law). Radiation vs. distance
More informationEarth s Radiation Budget & Climate
Earth s Radiation Budget & Climate Professor Richard Allan University of Reading NERC Advanced Training Course Earth Observations for Weather & Climate Studies 5 9 September 2016 Quantify the main terms
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 informationATMOS 5140 Lecture 7 Chapter 6
ATMOS 5140 Lecture 7 Chapter 6 Thermal Emission Blackbody Radiation Planck s Function Wien s Displacement Law Stefan-Bolzmann Law Emissivity Greybody Approximation Kirchhoff s Law Brightness Temperature
More informationEarth 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 informationName(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 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 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 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 informationHow Accurate is the GFDL GCM Radiation Code? David Paynter,
Radiation Processes in the GFDL GCM: How Accurate is the GFDL GCM Radiation Code? David Paynter, Alexandra Jones Dan Schwarzkopf, Stuart Freidenreich and V.Ramaswamy GFDL, Princeton, New Jersey 13th June
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 informationEarth: A Dynamic Planet A. Solar and terrestrial radiation
Earth: A Dynamic Planet A Aims To understand the basic energy forms and principles of energy transfer To understand the differences between short wave and long wave radiation. To appreciate that the wavelength
More informationSurface Radiation Budget from ARM Satellite Retrievals
Surface Radiation Budget from ARM Satellite Retrievals P. Minnis, D. P. Kratz, and T. P. charlock Atmospheric Sciences National Aeronautics and Space Administration Langley Research Center Hampton, Virginia
More informationOverview of the Unified Radiation Package for NCEP models
Overview of the Unified Radiation Package for NCEP models Yu-Tai Hou Jul 2011 DTC/EMC Workshop Development Objectives:: State of the art technology, Standardized component modules, General plug-in compatibility,
More informationMNFFY 221/SIF 4082 Energy and Environmental Physics. 2002
MNFFY 221/SIF 4082 Energy and Environmental Physics. 2002 Suggested solution to exam Problem 2 a) Show that the energy received from the sun earth is on average equal to the solar constant S given by 1
More informationSatellite-based estimate of global aerosol-cloud radiative forcing by marine warm clouds
SUPPLEMENTARY INFORMATION DOI: 10.1038/NGEO2214 Satellite-based estimate of global aerosol-cloud radiative forcing by marine warm clouds Y.-C. Chen, M. W. Christensen, G. L. Stephens, and J. H. Seinfeld
More informationRadiative Balance and the Faint Young Sun Paradox
Radiative Balance and the Faint Young Sun Paradox Solar Irradiance Inverse Square Law Faint Young Sun Early Atmosphere Earth, Water, and Life 1. Water - essential medium for life. 2. Water - essential
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 information8. Clouds and Climate
8. Clouds and Climate 1. Clouds (along with rain, snow, fog, haze, etc.) are wet atmospheric aerosols. They are made up of tiny spheres of water from 2-100 m which fall with terminal velocities of a few
More informationRadiation, Sensible Heat Flux and Evapotranspiration
Radiation, Sensible Heat Flux and Evapotranspiration Climatological and hydrological field work Figure 1: Estimate of the Earth s annual and global mean energy balance. Over the long term, the incoming
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 informationAstron 104 Laboratory #10 Solar Energy and the Habitable Zone
Name: Date: Section: Astron 104 Laboratory #10 Solar Energy and the Habitable Zone Introduction The Sun provides most of the energy available in the solar system. Sunlight warms the planet and helps create
More informationDependence of Radiative Forcing on Mineralogy in the Community Atmosphere Model
Dependence of Radiative Forcing on Mineralogy in the Community Atmosphere Model Rachel Scanza 1, Natalie Mahowald 1, Jasper Kok 2, Steven Ghan 3, Charles Zender 4, Xiaohong Liu 5, Yan Zhang 6 February
More informationCERES_EBAF-Surface_Ed2.7 Data Quality Summary (June 7, 2013)
CERES_EBAF-Surface_Ed2.7 (June 7, 2013) Investigation: CERES Data Product: EBAF-Surface Data Set: Terra (Instruments: CERES-FM1 or CERES-FM2) Aqua (Instruments: CERES-FM3 or CERES-FM4) Data Set Version:
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 informationLecture 1b: Global Energy Balance. Instructor: Prof. Johnny Luo
Lecture 1b: Global Energy Balance Instructor: Prof. Johnny Luo Daily average insola>on A few points: 1. Solar constant ~ 1361 W m -2. But averaged over a whole day, we get much less. 2. At NYC in Jan,
More informationGlobal Energy Balance Climate Model. Dr. Robert M. MacKay Clark College Physics & Meteorology
Global Energy Balance Climate Model Dr. Robert M. MacKay Clark College Physics & Meteorology rmackay@clark.edu (note: the value of 342 W/m 2 given in this figure is the solar constant divided by 4.0 (1368/4.0).
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 informationGreenhouse Effect & Habitable Zones Lab # 7
Greenhouse Effect & Habitable Zones Lab # 7 Objectives: To model the effect of greenhouse gases on the radiative balance on Earth, and to think about what factors that can affect the habitability of a
More informationAssessing the impact of Arctic sea ice variability on Greenland Ice Sheet surface mass and energy exchange
Assessing the impact of Arctic sea ice variability on Greenland Ice Sheet surface mass and energy exchange J. Stroeve, L. Boisvert, J. Mioduszewski, T. Komayo Enhanced Greenland Melt and Sea Ice Loss R=
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 informationClimate Feedbacks from ERBE Data
Climate Feedbacks from ERBE Data Why Is Lindzen and Choi (2009) Criticized? Zhiyu Wang Department of Atmospheric Sciences University of Utah March 9, 2010 / Earth Climate System Outline 1 Introduction
More informationatmospheric influences on insolation & the fate of solar radiation interaction of terrestrial radiation with atmospheric gases
Goals for today: 19 Sept., 2011 Finish Ch 2 Solar Radiation & the Seasons Start Ch 3 Energy Balance & Temperature Ch 3 will take us through: atmospheric influences on insolation & the fate of solar radiation
More informationAn Observational Study of the Relationship between Cloud, Aerosol and Meteorology in Marine Stratus Regions
An Observational Study of the Relationship between Cloud, Aerosol and Meteorology in Marine Stratus Regions Norman G. Loeb NASA Langley Research Center Hampton, VA Oct 18 th, 2006, AeroCom Meeting (Virginia
More informationMore on Diabatic Processes
More on Diabatic Processes Chapter 3 Write Qtotal = Qrad + Qcond + Qsen total heating radiative heating condensationa l heating sensible heating While diabatic processes drive atmospheric motions, the
More informationRadiation Conduction Convection
Lecture Ch. 3a Types of transfers Radiative transfer and quantum mechanics Kirchoff s law (for gases) Blackbody radiation (simplification for planet/star) Planck s radiation law (fundamental behavior)
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 informationOn the use of satellite remote sensing to determine direct aerosol radiative effect over land : A case study over China
On the use of satellite remote sensing to determine direct aerosol radiative effect over land : A case study over China Anu-Maija Sundström, Antti Arola, Pekka Kolmonen, Gerrit de Leeuw, and Markku Kulmala
More informationRadiation balance of the Earth. 6. Earth radiation balance under present day conditions. Top of Atmosphere (TOA) Radiation balance
Radiation balance of the Earth Top of Atmosphere (TOA) radiation balance 6. Earth radiation balance under present day conditions Atmospheric radiation balance: Difference between TOA and surface radiation
More informationWhich picture shows the larger flux of blue circles?
Which picture shows the larger flux of blue circles? 33% 33% 33% 1. Left 2. Right 3. Neither Left Right Neither This Week: Global Climate Model Pt. 1 Reading: Chapter 3 Another Problem Set Coming Towards
More information2. 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 informationRadiation from planets
Chapter 4 Radiation from planets We consider first basic, mostly photometric radiation parameters for solar system planets which can be easily compared with existing or future observations of extra-solar
More informationLecture 2: Energy Balance and the Troposphere
Lecture 2: Energy Balance and the Troposphere Geoff Vallis; notes by Shineng Hu and Alexis Kaminski June 17 The philosophy throughout these lectures is that in order to understand a complex system we must
More informationTHE 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 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 informationExam Physics of Climate
Exam Physics of Climate Time allowed: 120 minutes You are allowed to use all online class materials, as well as graded problem sets and computer (EdGCM) labs. 1. [50 points] You are the science officer
More information