A New Basic 1-Dimension 1-Layer Model Obtains Excellent Agreement With the Observed Earth Temperature

Similar documents
1. Weather and climate.

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

- matter-energy interactions. - global radiation balance. Further Reading: Chapter 04 of the text book. Outline. - shortwave radiation balance

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?

Radiation, Sensible Heat Flux and Evapotranspiration

Lecture 9: Climate Sensitivity and Feedback Mechanisms

Global Climate Change

On the Meaning of Feedback Parameter, Transient Climate Response, and the Greenhouse Effect: Basic Considerations and the Discussion of Uncertainties

Climate Change: some basic physical concepts and simple models. David Andrews

Climate Dynamics Simple Climate Models

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

Let s make a simple climate model for Earth.

PTYS 214 Spring Announcements. Midterm 3 next Thursday!

Equation for Global Warming

Atmospheric "greenhouse effect" - How the presence of an atmosphere makes Earth's surface warmer

Lecture 2 Global and Zonal-mean Energy Balance

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

Earth Systems Science Chapter 3

Planetary Atmospheres

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

The Energy Balance Model

Planetary Atmospheres

THE EXOSPHERIC HEAT BUDGET

Lecture 4: Global Energy Balance

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

Parameterization for Atmospheric Radiation: Some New Perspectives

Lecture 7: The Monash Simple Climate

Fundamentals of Atmospheric Radiation and its Parameterization

Radiation from planets

Radiation in climate models.

Atmospheric "greenhouse effect" - How the presence of an atmosphere makes Earth's surface warmer

Stefan-Boltzmann law for the Earth as a black body (or perfect radiator) gives:

COURSE CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION

Klimaänderung. Robert Sausen Deutsches Zentrum für Luft- und Raumfahrt Institut für Physik der Atmosphäre Oberpfaffenhofen

Course Outline CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION. 1. Current climate. 2. Changing climate. 3. Future climate change

COMPUTER METHODS AND MODELING IN GEOLOGY MODELING EARTH'S TEMPERATURE

Global Energy Balance Climate Model. Dr. Robert M. MacKay Clark College Physics & Meteorology

ATMO 551a Intro to Optical Depth Fall τ υ,z. dz = di υ. B[ v,t(z) ]e

Earth s Radiation Budget & Climate

Radiation in the atmosphere

Lecture 3: Global Energy Cycle

Glaciology HEAT BUDGET AND RADIATION

Earth: the Goldilocks Planet

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

2. Illustration of Atmospheric Greenhouse Effect with Simple Models

Deducing Earth s Global Energy Flows from a Simple Greenhouse Model

Radiation Conduction Convection

2/18/2013 Estimating Climate Sensitivity From Past Climates Outline

The Structure and Motion of the Atmosphere OCEA 101

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

Energy Balance and Temperature

Key Feedbacks in the Climate System

FOLLOW THE ENERGY! EARTH S DYNAMIC CLIMATE SYSTEM

Understanding the Greenhouse Effect

2. Meridional atmospheric structure; heat and water transport. Recall that the most primitive equilibrium climate model can be written

Lecture 10: Climate Sensitivity and Feedback

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

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

Radiation and the atmosphere

Satellite Observations and Climate Modeling: What They Can and Cannot Reveal About Future Climate

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

Chapter 6: Modeling the Atmosphere-Ocean System

Lecture 3a: Surface Energy Balance

Outline. Stock Flow and temperature. Earth as a black body. Equation models for earth s temperature. Balancing earth s energy flows.

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

EAS270, The Atmosphere 2 nd Mid-term Exam 2 Nov. 2016

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

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

A Derivation of Radiative Equilibrium Model Equations

Chapter 1 INTRODUCTION AND BASIC CONCEPTS

Lecture 3: Atmospheric Radiative Transfer and Climate

Teaching Energy Balance using Round Numbers: A Quantitative Approach to the Greenhouse Effect and Global Warming

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

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

Friday 8 September, :00-4:00 Class#05

NOTES AND CORRESPONDENCE. On the Radiative and Dynamical Feedbacks over the Equatorial Pacific Cold Tongue

ATMOS 5140 Lecture 7 Chapter 6

Weather Forecasts and Climate AOSC 200 Tim Canty. Class Web Site: Lecture 27 Dec

Thursday, November 1st.

Climate Feedbacks from ERBE Data

Wednesday, September 8, 2010 Infrared Trapping the Greenhouse Effect

Lecture 3a: Surface Energy Balance

Earth s Energy Balance and the Atmosphere

Temperature Change. Heat (Q) Latent Heat. Latent Heat. Heat Fluxes Transfer of heat in/out of the ocean Flux = Quantity/(Area Time) Latent heat

Hand in Question sheets with answer booklets Calculators allowed Mobile telephones or other devices not allowed

Lecture 5: Greenhouse Effect

Course Outline. About Me. Today s Outline CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION. 1. Current climate. 2.

Introduction to Climate ~ Part I ~

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

Atmospheric Radiation

4. Zero-dimensional Model of Earth s Temperature

Lecture 5: Greenhouse Effect

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

Greenhouse Effect & Habitable Zones Lab # 7

Climate 1: The Climate System

Paper No. : 04 Paper Title: Unit Operations in Food Processing Module-07: Heat Transfer 3: Heat Radiation

The Atmosphere. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems

INTRODUCTION Radiation differs from conduction and convection in that it does not require the presence of a material medium to take place.

Changes in Earth s Albedo Measured by satellite

Transcription:

A New Basic 1-Dimension 1-Layer Model Obtains Excellent Agreement With the Observed Earth Temperature Rainer Link and Horst-Joachim Lüdecke EIKE, European Institute for Climate and Energy, PO.Box 11011, 07722 Jena, GERMANY info@cfact-europe.org rainer.link@gmx.info moluedecke@aol.com Electronic version of an article published in International Journal of Modern Physics, Vol. 22, No. 5 (2011) 449-455, DOI: 10.1142/S0129183111016361, copyright World Scientific Publishing Company, www.worldscinet.com Abstract. The Earth radiation and energy budget is calculated by a manifold of rather complex Global Circulation Models. Their outcome mostly cannot identify radiation in the atmosphere or energy budget relations. Therefore it is reasonable to look at more basic models to identify the main aspects of the model results. The simplest one of all of those is a 1-dimensional 1-layer model. However, most of these models - two are discussed here - suffer the drawback that they do not include essential contributions and relations between the atmospheric layer and the Earth. The 1-dimensional 1-layer model presented here integrates sensible and latent heat, the absorption of solar radiation in the atmosphere and the direct emission of the long wave radiation to space in addition to the standard correlations. For the atmospheric layer two different long wave fluxes are included, top of atmosphere to space and bulk emission to Earth. The reflections of long wave radiations are taken into account. It is shown that this basic model is in excellent agreement with the observed integrated global energy budget. Key words: : Earth energy budget; 1-dimensional 1-layer model; sensible and latent heat; long wave radiation 1 Introduction The Earth radiation and energy budget is calculated by a manifold of Global Circulation Models [1]. These are very complex and their results mostly cannot be plainly identified to understand the integral radiation or energy budget relations. Therefore it is reasonable to look at basic models to identify the main

2 Rainer Link and Horst-Joachim Lüdecke aspects. Kiel and Trenberth [2], [6] used a 1-dimensional 3-layer model with different top of atmospheric layer fluxes and those from the bulk atmospheric layer for the evaluation of the measured data. The results for their integral global energy budget are widely accepted as a reference. A quite elementary model is the 1-dimensional 1-layer model presented by Schneider and Mass [5], and from other authors following the approach from Liou [4]. Schneider and Mass did not take into account the absorption of solar radiation by the atmosphere nor the sensible and latent heat. Their model used only one temperature for the top of atmosphere and for the long wave radiation to the Earth, and their equation for thermal equilibrium was expressed by the basic formula R dt E /dt = (1 a) S 0 /4 + ε E F IR F IR (1) The problems associated with this oversimplification are thoroughly discussed by Kramm and Dlugi [3]. These authors correctly criticized Eq. (1) because the absorption of solar radiation in the atmosphere and/or the sensible and latent heat emitted by Earth are completely neglected. They finally improved the model of Schneider and Mass by including the sensible and latent heat and the absorption of solar radiation by the atmosphere. However, also this corrected model [3] shows substantial drawbacks. Kramm and Dlugi used only one temperature T and one integral emissivity ε A for the lower and upper part of the atmospheric layer (Eqs. A19, A20 in Ref. 3). This is not feasible because of the big difference between the long-wave radiation from the top of the atmosphere and the down-welling infrared radiation to the Earth from the lower atmosphere [2], [6]. Furthermore, the direct emission of the long wave radiation from Earth to space was wrongly taken into account by a term (1 ε a ) ε E TE 4 (p. 152 and Eq. A18 in Ref. 3) that disappears for ε a = 1. This was the reason why Kramm and Dlugi for the mean Earth temperature obtained T E = 268 K (Figure 15 in Ref. 3). This disagrees with the observed value T E = 288 K. Kramm and Dlugi calculated the mean temperature of the atmosphere T A = 255 K. In their paper this value is independent of the integral absorbtivity of the atmosphere with respect to solar radiation (A a in Figure 15 of Ref. 3), which seems rather odd. Furthermore Kramm and Dlugi used the same latent and sensible heat of 92 W/m 2 for the whole temperature range of TE down to the freezing temperature of 268 K 5 0 C. This is not feasible as is demonstrated in Figure 3 where we show the temperature dependence of Q on T A. Kramm and Dlugi used the incompatibility of their model results with observed values as an argument that their model (the improved model of Schneider et al.) reveals no evidence for the existence of the so-called atmospheric greenhouse effect, if realistic empirical data are used. 2 Applied methods A basic 1-dimensional 1-layer model with different atmospheric and top of atmosphere long wave radiation fluxes and temperatures, including the reflections

A New Basic One-Dimension One-Layer Model 3 of the long wave radiation at the surface of the Earth and atmosphere can correctly reproduce the observed global average surface temperatures and radiation fluxes, if all emission and absorption processes are accurately introduced into the model. The model and the interrelations of the model presented here are shown schematically in the following Figure 1: Fig. 1. Fluxes applied in the 1-dimensional 1-layer model of this paper. The abbreviations are for short wave: S 0 - Incident solar flux (1365 W/m 2 ), S R - Total reflected flux, S RA- Reflected by atmosphere, S A -Absorbed by atmosphere, S ER -Reflected by Earth, S E - Absorbed by Earth. For long wave: L T oa- Emitted from top of atmosphere, L Ed - Directly emitted from Earth, L EA - Emitted by Earth and absorbed by atmosphere, L rea - Emitted by Earth and reflected by atmosphere, L A - Emitted by atmosphere and absorbed by Earth, L ra - Emitted by atmosphere and reflected by Earth, L O - Outgoing long wave radiation, Q S, Q L: Sensitive and latent heat, Q = Q S + Q L The model depicted in Figure 1 is a 1-dimensional 1-layer model which integrates sensible and latent heat, the absorption of solar radiation and the direct emission of the long wave radiation to space. The reflection of long wave radiation from the surface and atmosphere is taken into account. For the atmospheric layer two different long wave fluxes are included, from top of atmosphere to space and bulk emission to Earth. Direct emission to space of the reflected atmospheric back radiation to Earth is not considered, because it is assumed that the reflected spectrum fits completely into the absorption bands of the greenhouse gases. The following relations hold as they can be deducted from Figure 1: 0 = S 0 /4 S R L T oa L Ed (2) 0 = S A L A + L ra L T oa + L EA L rea + Q (3)

4 Rainer Link and Horst-Joachim Lüdecke 0 = S E S ER L EA + L rea L Ed + L A L ra Q (4) Additionally the following connections are evident: L E = L EA + L Ed (5) S R = S RA + S ER (6) α = (S RA + S ER )/(S 0 /4) (7) α A = S A /(S 0 /4) (8) S E = S 0 /4 S RA S ER S A = S 0 /4 (1 α α A ) (9) d = L Ed /L E (10) L 0 = L T oa + L Ed = L T oa + d L E (11) r EA = L rea /L EA (12) r A = L ra /L A (13) The following relations result 0 = (1 α) S 0 /4 L O (14) 0 = α A S 0 /4 L A (1 r A ) L T oa + L EA (1 r EA ) + Q (15) 0 = (1 α α A ) S 0 /4 L E (1 r EA d r EA ) + L A (1 r A ) Q (16) From ERBE (Earth Radiation Budget Experiment) data [2] and [6] and references cited therein, a value for L 0 = 241 W/m 2 and L T oa = 199 W/m 2 was evaluated. As it can be seen in the above relations, we connect the long wave radiation fluxes. As a consequence, the equations are independent of absorption and emission coefficients. From Eq. (2), Eq.(5), Eq. (6), Eq.(7), Eq. (15), and Eq. (16), one obtains (see also Figure 1) L E = ((1 α) S 0 /4 L T oa )/d (17) L A = [L E (1 r EA (1 + d)) (1 α α A ) S 0 /4 + Q]/(1 r A ) (18) The dependence of L E in Eq. (17) and L A in Eq. (18) on the fraction d = L ED /L E is shown in Figure 2. For the calculation of L A it is assumed that r EA = (1 ε A ) = 0 and r A = (1 ε E ) = 0, which is in agreement with the energy and radiation balance scheme of Kiel and Trenberth [2], [6], who neglected the reflexion of long wave radiation from the surface of the Earth and from the atmosphere. For the absorption values we also followed Trenberth [6] with α A = 0.23 and α = 0.3.

A New Basic One-Dimension One-Layer Model 5 Fig. 2. The long-wave flux L A (red) emitted by the atmosphere and absorbed by the Earth (back radiation, see Figure 1) and L E = L EA + L Ed (blue) as a function of d = L Ed / L E. The vertical line marks the value of d = 0.101, which corresponds to the observed values of Trenberth [6] The corresponding temperatures are calculated according to Stephan-Boltzmann and assuming a gray body for Earth and atmosphere ( ε - emission coefficients, σ - Stephan-Boltzmann constant): ε A σ T 4 A = L A (19) ε E σ T 4 E = L E (20) ε T oa σ T 4 T oa = L T oa (21) With the values (see Ref. 6) Q = 97 W/m 2, L T oa = 199 W/m 2, α A = 0.23, and d = 0.101 the mean global temperature T E, L A and L E are reproduced with r EA = (1 ε A ) = 0, (ε A =1), r A = (1 ε E ) = 0, (ε E =1). This is evident, as Kiel and Trenberth [2], [6] did not take into account the reflexion of long wave radiation from the Earth and atmosphere. Our model of course is capable of calculating these values with non zero reflexions of long wave radiation to atmosphere or surface. L A = 333 W/m 2 (see Figure 2) L E = 396 W/m 2 (see Figure 2)

6 Rainer Link and Horst-Joachim Lüdecke T E 289 K (Eq. (20)) T A 277 K (Eq. (19)) In addition, if we assume ε T oa =1, T T oa 243 K results. The mean atmospheric temperature T A as a function of α A can be evaluated from Eqs. (18) and (19). In very good approximation the function is linear T A = 75.04 α A + 257 K (22) Obviously the value for T A is strongly dependent on α A in disagreement with the results from Kramm and Dlugi [3], who calculated the mean temperature of the atmosphere as T A = 255 K, independent of the integral absorption of the atmosphere with respect to the short wave radiation of the sun. Figure 3 shows the T E temperature dependence of Q = Q S + Q L (sensible and latent heat) and of the mean atmospheric temperatur T A with α = 0.3, α A = 0.23, r EA =r A =0, d = 0.101, evaluated with the Eqs. (17) - (20). The Albedo of clouds and surface of the Earth have not been changed as function of temperature, although a strong dependence must be expected as well. Unfortunately there exists no detailed calculation or any Ansatz from more complex global circulation models. Fig. 3. Temperature dependence of Q = Q S + Q L (sensible and latent heat) and of the mean atmospheric temperatur T A with α = 0.3, α A = 0.23, r EA=r A=0, d = 0.101. It was assumed that the temperature dependence of Q is proportional to the absolute humidity resulting in Q = 7 W/m 2 and T A = 227 K for an Earth temperature of T E = 271 K.

A New Basic One-Dimension One-Layer Model 7 Within our model the effect of a radiative forcing can be deduced. From the values given by Trenberth [6] the ratio L Ed /L 0 = 0.167 (23) is determined. Assuming an additional radiative forcing RF = L 0 as described by IPCC AR4 and a corresponding partition of RF after readjustment to radiative equilibrum as in Eq. (23) L Ed L 0 holds. Eq. (10) with d = 0.101 can be written as = L Ed L 0 = 0.167 (24) L Ed / L E = 0.101 (25) For a doubling of CO 2 the IPCC asumes RF = 3.7 W/m 2. RF = L 0 together with Eq. (24) and Eq. (25) yield L E = (0.167/0.101) RF = 6.12 W/m 2 (26) The unturbed state is L E = 396 W/m 2. This and Eq. (20) result in T 289.1 K. The perturbed state, however, is L E + L E = 402.12 W/m 2 that yields T 290.2 K. As a result, the change of the surface temperature of the Earth induced by 3.7 W/m 2 radiative forcing (doubling of CO 2 ) is T 1.1 K, which is in good agreement with the IPCC value [1] without feedback. 3 Conclusion This paper demonstrates that a basic 1-dimensional 1-layer model with different atmospheric and top of atmosphere long wave radiation fluxes and temperatures, and including the reflections of the long wave radiation at the surface of the Earth and atmosphere can reproduce with excellent agreement the observed global average surface temperatures and radiation fluxes. This requires that all emission and absorption processes are correctly introduced into the model. In particular the direct emission of long wave radiation from Earth to space and the temperature dependence of latent and sensible heat have to be taken into account. Our model yields a change in the surface temperature of the Earth of roughly 1.1 o C for an additional radiative forcing of 3.7 W/m 2 - caused for instance by a hypothetical doubling of the present CO 2 concentration in the atmosphere -, which is in good agreement with the appropriate IPCC value, if no feedback amplification (or attenuation) is considered. References 1. AR4, IPCC (2007), http://www.ipcc.ch/publications and data/ar4/wg1/en/contents.html

8 Rainer Link and Horst-Joachim Lüdecke 2. J. T. Kiehl and K. E. Trenberth, Earths Annual Global Mean Energy Budget, Bulletin of the American Meteorological Society 78, No. 2 (1997) 3. G. Kramm and R. Dlugi, On the Meaning of Feedback Parameter, Transient Climate Response, and the Greenhouse Effect: Basic Considerations and the Discussion of Uncertainties, The Open Atmospheric Science Journal 4 (2010) 4. K. N. Liou, An introduction to atmospheric radiation - 2nd edn., Academic Press (2002) 5. S. H. Schneider and C. Mass, Volcanic dust, sunspots, and temperature trends, Science 190, 741 (1975) 6. K. E. Trenberth, J. T. Fasullo and J. T. Kiehl, Earths Global Energy Budget, American Meteorological Society (BAMS), March 2009