Patterns in the CERES Global Mean Data, Part 3

Size: px
Start display at page:

Download "Patterns in the CERES Global Mean Data, Part 3"

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. 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 information

Patterns in the CERES Global Mean Data

Patterns 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 information

Deducing Earth s Global Energy Flows from a Simple Greenhouse Model

Deducing 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 information

Interannual variability of top-ofatmosphere. CERES instruments

Interannual 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 information

A new diagram of Earth s global energy budget

A 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 information

History of Earth Radiation Budget Measurements With results from a recent assessment

History 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 information

Seeking 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 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 information

Atmospheric "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 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 information

Radiation in climate models.

Radiation 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 information

Understanding the Greenhouse Effect

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

More information

Lecture 3. Background materials. Planetary radiative equilibrium TOA outgoing radiation = TOA incoming radiation Figure 3.1

Lecture 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 information

Lecture 4: Global Energy Balance

Lecture 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 information

Lecture 4: Global Energy Balance. Global Energy Balance. Solar Flux and Flux Density. Blackbody Radiation Layer Model.

Lecture 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 information

Variability in Global Top-of-Atmosphere Shortwave Radiation Between 2000 And 2005

Variability 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 information

Earth Systems Science Chapter 3

Earth 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 information

and Atmospheric Science, University of Miami, 4600 Rickenbacker Causeway, Miami, FL 33149, USA.

and 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 information

Global Energy and Water Budgets

Global 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 information

Is the Earth s climate system constrained?*+

Is 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 information

Constraints 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. 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 information

Lecture # 04 January 27, 2010, Wednesday Energy & Radiation

Lecture # 04 January 27, 2010, Wednesday Energy & Radiation Lecture # 04 January 27, 2010, Wednesday Energy & Radiation Kinds of energy Energy transfer mechanisms Radiation: electromagnetic spectrum, properties & principles Solar constant Atmospheric influence

More information

Atmospheric "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 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 information

Data and formulas at the end. Exam would be Weds. May 8, 2008

Data 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

Mon Oct 20. Today: radiation and temperature (cont) sun-earth geometry energy balance >> conceptual model of climate change Tues:

Mon 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 information

Changes in Earth s Albedo Measured by satellite

Changes 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 information

9/5/16. Section 3-4: Radiation, Energy, Climate. Common Forms of Energy Transfer in Climate. Electromagnetic radiation.

9/5/16. 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 information

Data and formulas at the end. Real exam is Wednesday May 8, 2002

Data 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 information

Climate Dynamics Simple Climate Models

Climate 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 information

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

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

More information

Habitable Planets. Much of it stolen from. Yutaka ABE University of Tokyo

Habitable 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 information

Solar Insolation and Earth Radiation Budget Measurements

Solar 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 information

Aerosol 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 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 information

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

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

More information

Influence 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 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 information

Radiation in the atmosphere

Radiation 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 information

Lecture 3: Global Energy Cycle

Lecture 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 information

Heat, temperature and gravity Emil Junvik

Heat, 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 information

How good are our models?

How 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 information

Do climate models over-estimate cloud feedbacks?

Do 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 information

Planetary Atmospheres

Planetary 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 information

2. Illustration of Atmospheric Greenhouse Effect with Simple Models

2. 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 information

Spectrum of Radiation. Importance of Radiation Transfer. Radiation Intensity and Wavelength. Lecture 3: Atmospheric Radiative Transfer and Climate

Spectrum of Radiation. Importance of Radiation Transfer. Radiation Intensity and Wavelength. Lecture 3: Atmospheric Radiative Transfer and Climate Lecture 3: Atmospheric Radiative Transfer and Climate Radiation Intensity and Wavelength frequency Planck s constant Solar and infrared radiation selective absorption and emission Selective absorption

More information

Lecture 3: Atmospheric Radiative Transfer and Climate

Lecture 3: Atmospheric Radiative Transfer and Climate Lecture 3: Atmospheric Radiative Transfer and Climate Solar and infrared radiation selective absorption and emission Selective absorption and emission Cloud and radiation Radiative-convective equilibrium

More information

Lecture 2 Global and Zonal-mean Energy Balance

Lecture 2 Global and Zonal-mean Energy Balance Lecture 2 Global and Zonal-mean Energy Balance A zero-dimensional view of the planet s energy balance RADIATIVE BALANCE Roughly 70% of the radiation received from the Sun at the top of Earth s atmosphere

More information

P607 Climate and Energy (Dr. H. Coe)

P607 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 information

Lecture 3a: Surface Energy Balance

Lecture 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 information

The 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 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 information

Lecture 3a: Surface Energy Balance

Lecture 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 information

Complexity 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 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 information

Planetary Atmospheres

Planetary 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 information

Monday 9 September, :30-11:30 Class#03

Monday 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 information

IDŐJÁRÁS 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 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 information

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.

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. 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 information

Very Dynamic! Energy in the Earth s Atmosphere. How Does it Get Here? All Objects Radiate Energy!

Very 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 information

Take away concepts. What is Energy? Solar Radiation Emission and Absorption. Energy: The ability to do work

Take 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 information

Earth s Radiation Budget & Climate

Earth 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 information

1) The energy balance at the TOA is: 4 (1 α) = σt (1 0.3) = ( ) 4. (1 α) 4σ = ( S 0 = 255 T 1

1) 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 information

ATMOS 5140 Lecture 7 Chapter 6

ATMOS 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 information

Earth s Energy Budget: How Is the Temperature of Earth Controlled?

Earth s Energy Budget: How Is the Temperature of Earth Controlled? 1 NAME Investigation 2 Earth s Energy Budget: How Is the Temperature of Earth Controlled? Introduction As you learned from the reading, the balance between incoming energy from the sun and outgoing energy

More information

Name(s) Period Date. Earth s Energy Budget: How Is the Temperature of Earth Controlled?

Name(s) Period Date. Earth s Energy Budget: How Is the Temperature of Earth Controlled? Name(s) Period Date 1 Introduction Earth s Energy Budget: How Is the Temperature of Earth Controlled? As you learned from the reading, the balance between incoming energy from the sun and outgoing energy

More information

Radiative Equilibrium Models. Solar radiation reflected by the earth back to space. Solar radiation absorbed by the earth

Radiative 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 information

ATMS 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 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 information

1. Weather and climate.

1. 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 information

How Accurate is the GFDL GCM Radiation Code? David Paynter,

How 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 information

Key Feedbacks in the Climate System

Key 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 information

Earth: A Dynamic Planet A. Solar and terrestrial radiation

Earth: 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 information

Surface Radiation Budget from ARM Satellite Retrievals

Surface 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 information

Overview of the Unified Radiation Package for NCEP models

Overview 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 information

MNFFY 221/SIF 4082 Energy and Environmental Physics. 2002

MNFFY 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 information

Satellite-based estimate of global aerosol-cloud radiative forcing by marine warm clouds

Satellite-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 information

Radiative Balance and the Faint Young Sun Paradox

Radiative 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 information

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Physics Problem Solving 10: The Greenhouse Effect. Section Table and Group

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Physics Problem Solving 10: The Greenhouse Effect. Section Table and Group MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Physics 8.02 Problem Solving 10: The Greenhouse Effect Section Table and Group Names Hand in one copy per group at the end of the Friday Problem Solving

More information

8. Clouds and Climate

8. 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 information

Radiation, Sensible Heat Flux and Evapotranspiration

Radiation, 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

- 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 information

Astron 104 Laboratory #10 Solar Energy and the Habitable Zone

Astron 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 information

Dependence of Radiative Forcing on Mineralogy in the Community Atmosphere Model

Dependence 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 information

CERES_EBAF-Surface_Ed2.7 Data Quality Summary (June 7, 2013)

CERES_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 information

CLIMATE 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 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 information

Lecture 1b: Global Energy Balance. Instructor: Prof. Johnny Luo

Lecture 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 information

Global 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 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 information

Greenhouse Effect & Venusian Atmospheric Balance. Evan Anders

Greenhouse 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 information

Greenhouse Effect & Habitable Zones Lab # 7

Greenhouse 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 information

Assessing 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 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 information

Introduction to Climate ~ Part I ~

Introduction 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 information

Climate Feedbacks from ERBE Data

Climate 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 information

atmospheric influences on insolation & the fate of solar radiation interaction of terrestrial radiation with atmospheric gases

atmospheric 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 information

An 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 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 information

More on Diabatic Processes

More 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 information

Radiation Conduction Convection

Radiation 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 information

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

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

More information

Energy Balance and Temperature

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

More information

On 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 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 information

Radiation balance of the Earth. 6. Earth radiation balance under present day conditions. Top of Atmosphere (TOA) Radiation balance

Radiation 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 information

Which picture shows the larger flux of blue circles?

Which 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 information

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

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

More information

Radiation from planets

Radiation 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 information

Lecture 2: Energy Balance and the Troposphere

Lecture 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 information

THE EXOSPHERIC HEAT BUDGET

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

More information

Earth: the Goldilocks Planet

Earth: the Goldilocks Planet Earth: the Goldilocks Planet Not too hot (460 C) Fig. 3-1 Not too cold (-55 C) Wave properties: Wavelength, velocity, and? Fig. 3-2 Reviewing units: Wavelength = distance (meters or nanometers, etc.) Velocity

More information

Exam Physics of Climate

Exam 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