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Introduction to Climate Modeling

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Presentation on theme: "Introduction to Climate Modeling"— Presentation transcript:

1 Introduction to Climate Modeling
Zhengyu Liu

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3 Why we need a Climate Model?
Quantitative Assessment of Complex System Numerical Laboratory, especially important for geophysical field Most credible strategy for prediction

4 Outline Part I: A Conceptual Climate Model Radiative Equilibrium Model Prognostic Coupled Ocean-Atmosphere Model Part II: Challenges in Numerical Climate Model Numerical Stability Parameterization Interaction

5 Part I: Global mean model (0-D) Why the Earth surface temperature is about 15oC (288K)?
Equilibrium Model Prognostic Model

6 Radiative Equilibrium Model
S Cloud S (1-)S TS4 (1-)S GHG T4 T4 S=342Wm2 Qs = S -  T4 =0 T = (S/ )1/4 , T =279oK=6oC, Too cold! , Qs = (1-a)S -  T4 =0 T = [(1-a)S/ ]1/4 T =255oK= -18oC Even colder QTOA = (1-a)S -  T4 = 0 Qs = (1-a)S +  T4 -  TS4 =0 T= ((1-a)S/ )1/4 TS =21/4T=288oK=15oC About right… b=dT/dS ~ 1/(4 T 3) Climate Sensitivity

7 Climate Sensitivity To explain the ice age, Arrhenius estimated that halving of CO2 would decrease temperatures by 4 - 5 °C (Celsius) and a doubling of CO2 would cause a temperature rise of 5 - 6 °C. In his 1906 publication, Arrhenius adjusted the value downwards to 1.6 °C (including water vapour feedback: 2.1 °C). Recent (2007) estimates from IPCC say this value (the Climate sensitivity) is likely to be between 2 and 4.5 °C. Arrhenius expected CO2 doubling to take about 3000 years; it is now estimated in most scenarios to take about a century. Svante Arrhenius

8 Prognostic Coupled Climate System
To4 Atmosphere Ocean Equilibrium Model

9 in Numerical Climate Modeling
Part II: Challenges in Numerical Climate Modeling C1. Numerical Stability C2. Physical Parameterization C3. Interaction Among Components

10 C1: Numerical Stability I: Temporal Descritization
tn tn+1 Tn Tn+1 Stability Condition  time step limit Implications: too large time step leads to model “blow up” (also poor model accuracy: 2) Very small time step is needed to simulate faster process (large a) e.g. atmosphere, and even more, small scale clouds…..

11 Implication to Coupled Climate System
Atmosphere Ocean Equilibrium Model Full Model Intermediate Model Expensive!

12 A Numerical Demonstration

13 3-D Climate model

14 Atmospheric General Circulation

15 The Coupled Ocean-Atmosphere System
EQ Transient Eddies Stationary Waves S. Pole N. Pole N. Atlantic THC ~ decadal-centennial Southern Ocean THC ~ millennial Thermocline circulation ~ decadal Hadley Cell The Coupled Ocean-Atmosphere System

16 General Circulation Model (GCM): Equations
Momentum Equations Mass Equation Heat Equation Equation of State where

17 General Circulation Model: Spatial Descritization
atmosphere ocean

18 C1: Numerical Stability II: Spatial- Descritization
Energy balance model Stability Condition Implication Double resolution requires quadrupling temporal resolution! So, the computation is increased 2(dy)*4(dt)=8 ~ 10 times ( for 3-D model, x, y, z… , 2(dx)*2(dy)*2(dz)*4(dt)=32 times !) Conclusion Very expensive for high resolution modeling!

19 C2: Physics Parameterization: Subgrid-scale physics
Current Climate Model General circulation (resolved) Synoptic storms (resolved) Clouds (parameterized) Droplets (….) Condensation nucli (…) ……….

20 Computational Implication on parameterization
S T4 To4 Atmosphere Ocean Coupled Climate System Full Model Intermediate Model parameterization

21 C3: Interdisciplinary Interaction:
Land 3.8° Atmosphere Sea Ice x3° Ocean C3: Interdisciplinary Interaction: Earth System Modeling Earth System Model

22 Tropical Bias Observation Model (original) Model
(solar penetration parameterization)

23 Model-Data Comparison of Last Glaical Maximum Climate
LGM Climate Obs SST CLIMAP SST Model SST Model SST Model Tair Model Tair 1) CO2 vs. ice sheet 2) Proxy uncertainty vs. model uncertainty Liu et al., 2002, GRL

24 C3: Earth System Model Physical Model +Ecological Model
+Biogeochemical Model +……. No perfect model! A model for a purpose!

25 The End

26 Radiative Equilibrium Model
S Qsurf = S -  T4 =0 T c= (S/ )1/4 , S=342 Wm2  T c =279oK=6oC, Too cold! ,

27 Cloud Albedo Effect: Radiative Equilibrium Model
S Cloud S (1-)S Qsurf = (1-a)S -  T4 =0 T cc= [(1-a)S/ ]1/4 ,  T cc =255oK= -18oC Even colder

28 Greenhouse Effect Qsurf = (1-a)S +  Tg4 -  T4 =0
glass Tg4 Qsurf = (1-a)S +  Tg4 -  T4 =0 QTOA = (1-a)S -  Tg4 = 0 Tg= ((1-a)S/ )1/4 = Tcc=255K ,  Tcg =21/4Tg=288oK=15oC About right…

29 How does the climate respond to global warming forcing?
CO2 induced Radiative Forcing Climate Sensitivity

30 CO2 induced Radiative Forcing
RF= 5.25 ln (CO2) W/m (S. Arrhenius, 1900) Examples: Present relative to 1850 (CO2 =250ppm) RF=5.25 *ln (385 / 250 ppm) = ~2.5 W/m2 Doubliing CO2 RF=5.25 *ln (500 / 250 ppm) = ~4 W/m2 Climate Sensitivity ΔT=b*RF b = climate sensitivity! = increase in temperature per unit increase in radiative forcing

31 Climate Sesnsitivity and Global Warming Response
RF(CO2) T4 S Global warming prediction: Qsurf = S +RF-  T4 =0 T = [(S+RF)/ ]1/4 ~= (S/ )1/4 +b*RF = Tc +b*RF, here RF<<S or global warming ΔT= T- Tc = b*RF Climate sensitivity: b=d (S/ )1/4 /dS = 1/(4 Tc 3)=0.2 K / Wm-2 Double CO2 : ΔT = b*RF = 0.2 * 4 = 0.8oK, small??

32 The Role of Climate Model
Quantitative Assessment of Complex System Numerical Laboratory, especially important for geophysical field Most credible strategy for prediction

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