Chapter 3. Fundamentals of Atmospheric Modeling

Size: px
Start display at page:

Download "Chapter 3. Fundamentals of Atmospheric Modeling"

Transcription

1 Overhead Slides for Chapter 3 of Fundamentals of Atmospheric Modeling by Mark Z. Jacobson Department of Civil & Environmental Engineering Stanford University Stanford, CA January 30, 00

2 Wind Velocity and Speed Velocity Rate at which the position of a body changes with time Velocity vector v = iu+ jv+ kw (3.) Horizontal velocity vector vh = iu+ jv (3.) Scalar components of wind velocity u x = d v y = d w z = d (3.) Wind speed Magnitude of the velocity vector v = u + v + w (3.3) Horizontal wind speed v h = u + v (3.3)

3 Zonally-/Monthly-Averaged Winds (m/s) Figure 3. a January Altitude (km) Latitude

4 Zonally-/Monthly-Averaged Winds (m/s) Figure 3. b July Altitude (km) Latitude

5 Local and Total Differentiation Expansion of total derivative with chain rule d = dx t + x = t +u x (3.4) Total derivative. Time rate of change along a trajectory d Local derivative. Time rate of change at a fixed point t Transport term. Time rate of change due to transport u x Eulerian frame of reference Frame of reference of a fixed point in space t + u x Lagrangian frame of reference Frame of reference of a moving parcel d

6 Example Example 3.. Balloon traveling with the wind from east to west d x = 0 8 molec cm -3 s - = 0 0 molec cm -3 km - u = -0 m s - Find time rate of change in concentration at fixed point A t = d t u d x = 0 8 molec. m molec. km 0 00 = 0 8 molec. 3 cm s s 3. cm km m 3 cm s

7 Gradient Operator Gradient operator in Cartesian / altitude coordinates = i + j + k x y z (3.6) Dot product of velocity vector with gradient operator v = ( iu+ jv+ kw) i + j + k = u + v + w x y z x y z (3.7) i i i = j j=, k k = j= 0 i k = 0 j k = 0 Dot product of gradient operator with velocity vector Divergence term u v v = i + j + k ( iu+ jv+ kw)= + + x y z x y w z (3.8) Dot product of gradient operator with vector not symmetric v v Dot product of two vectors is symmetric a v = v a

8 Gradient Operator Scalar concentration divergence term u ( v)= + v + x y w z (3.9) Gradient of a scalar variable is a vector = + + = + + x y z i j k i j k x y z (3.0) Apply dot product of velocity and gradient operator to ( v ) = u + v + w = u + v + w x y z x y z (3.) Substitute into total derivative d = + ( v ) (3.) t Generalize and expand total derivative d = u v w t = + v (3.3) x y z t

9 Continuity Equation y Figure 3.. u u z x Accumulation = molecules entering - molecules leaving x y z = u y z t u y z t (3.4) Divide both sides by t and box volume ( x y z) t u u = (3.5) x x --> 0 and t --> 0 --> Flux divergence form of continuity equation t u x = (3.6)

10 Continuity Equation Flux divergence form of continuity equation in three dimensions t u v w = = ( v ) (3.7) x y z Take dot product of gradient operator with v ( v)= ( v)+ ( v ) (3.8) Substitute into (3.7) t = ( v) ( v ) (3.9) From definition of total derivative d ( v ) = t (3.) Substitute into (3.9) and similar equation for density --> Velocity divergence forms of continuity equation d = ( v ) (3.) dρa = ρa v (3.3)

11 Continuity Equation for Mass Mixing Ratio umber concentration as a function of moist-air mass mixing ratio = Aρ a q (3.4) m Substitute (3.4) into (3.9) ρ q a t q + ρ ρ ρ a( v)+ ( v ) a + a = ρa( v ) q (3.5) t Substitute continuity equation for air --> Continuity equation for moist-air mass mixing ratio of a species with no external source or sink terms. q t = ( v q ) (3.6)

12 Compressibility / Incompressibility Compressible fluid (air) Volume of an air parcel changes over time and density varies (thus air is inhomogeneous) u v w v = + + = 0 x y z Incompressible fluid (water) Volume of a water parcel stays constant, but density varies (thus water is also inhomogeneous) u x v w + + = 0 (3.7) y z Substitute water density (ρ w ) and v = 0 into (3.3) Density of incompressible fluid is constant along motion dρ w = 0 (3.8) Substitute water density (ρ w ) and v = 0 into (3.0). At a fixed point in the fluid, water density changes. ρw t = v ρw (3.9)

13 Expanded Continuity Equation Expanded continuity equation t D R n n et = + + = v, (3.30) Substitute = = x y z x y z i j k i j k = + + x y z (3.3) into (3.30) to obtain t u x v y w z D x y z R n n et = =, (3.3)

14 Time and Grid Volume Averaging Precise gas concentration = + (3.33) Time and grid volume averaged concentration = t x y z t+ t t x+ x x y+ y y z+ z z d dy x t z d d (3.34) Precise wind velocity vector v = v+ v (3.36) u = u + u v = v + v w = w + w (3.35) Figure 3.3. Precise, mean, and perturbation components of scalar velocity and gas concentration, respectively. u _ u u' _

15 Continuity Equation Substitute (3.33) and (3.35) into (3.3) + t + u u x v v y w w z + + = ( + ) + + D x y Simplify terms + + z + et, R n n= (3.37) + t = (3.38) + t = = + + t t t + = + = = 0 Simplify again + u + u x ( u + u + u + u ) u u x x = + = (3.39) u = 0 u = 0 u = u

16 Continuity Equation Substitute averaged terms into (3.50) t u x v y w z u v w + + x y z = D + + x y et, + R n z n= (3.40) Turbulent diffusion is much larger than molecular diffusion --> ( u ) ( v ) ( w ), u v w = R n t x y z x y z n= (3.4) Continuity equation for gas in vector notation. et t et, + ( v)+ ( v )= R n n= (3.4) Similar equation for air mass density ρa t + ( vρa)+ ( v ρ a)= 0 (3.43)

17 Continuity Equation for Mass Mixing Ratio Continuity equation for trace gas in mass mixing ratio units q t + v q = et, R n n= (3.44) Continuity equation for air ρa t = ρa( v) ( v ) ρa (3.0) Sum continuity equations + = ρaq t et, ρavq ρa Rn n= (3.45) Take time and grid volume average of terms in equation --> Species continuity equation q t + ( v ) q + ( ρav q )= ρa et, Rn n= (3.49)

18 Parameterization of Diffusion Eddies Swirling motions of air caused by wind shear and enhanced by buoyancy Turbulence Many eddies of different sizes acting together Turbulent diffusion Subgrid diffusion due to turbulence K-theory Relates turbulent flux of one parameter (e.g. concentration) to gradient of mean value of the parameter Kinematic turbulent flux terms u = Khxx, x v = Khyy, y w = Khzz, z (3.50) Substitute (3.50) into (3.4) t u x v = y + + z K hzz, z w z x K x y K hxx, + hyy, y et, Rn n= (3.5)

19 Continuity Equations for Trace Gases and Air Continuity equation for trace gas number conc. (molec. cm -3 ) t + et, + ( v)= Kh Rn n= (3.5) Expanded continuity equation for a trace gas q t + ( vq)= ( K h ) q (3.56) + Remisg + Rdepg + Rwashg + Rchemg + Rnucg + Rc eg + Rdp sg + Rds eg + Rhrg Continuity equation for air ρa t + ( vρa )= 0 (3.55)

20 Continuity Equations for Particles Continuity equation for particle number conc. (partic. cm -3 ) ni t + ( vni)= K h ni (3.58) + Remisn + Rdepn + Rsedn + Rwashn + Rnucn + Rcoagn Volume concentration versus number concentration and volume vqi, = niυ qi, (3.57) Continuity equation for particle volume concentration (cm 3 cm -3 ) vqi, t + ( vvqi, )=( K h ) vqi, (3.59) + Remisv + Rdepv + Rsedv + Rwashv + Rnucv + Rcoagv R R R R R R cev dpsv dsev eqv aqv hrv

21 Continuity Equations for Water Water vapor qv + ( v ) qv = ( ρakh ) qv (3.6) t ρa + RemisV + RdepV + RchemV + RnucV + Rc ev + Rdp sv Liquid water q Li, + ( v ) qli, = ( ρakh ) ql, i (3.6) t ρa + RemisL + RdepL + RsedL + RnucL + RcoagL + Rc e L + Rf m L Ice q Ii, + ( v ) qii, = ( ρakh ) qi, i t ρa + RdepI + RsedI + RnucI + RcoagI + Rf mi + Rdp s I (3.63) Bulk vs. Size-Resolved Process Size resolved treatment of water B qt = qv + ql, i + qi, i i= (3.60) Bulk treatment of water qt = qv + ql + qi

22 Thermodynamic Energy Equation Energy transfer processes Conduction Advection Forced Convection Free Convection Turbulence Radiative transfer Energy sources / sinks Latent heat release / absorption Solar / infrared emissions / absorption First law of thermodynamics dq = cpd, dtv α adpa (.76) Differentiate, substitute αa = ρa, rearrange --> Thermodynamic energy equation in terms of temperature along the motion of an air parcel dtv dq = + cpd, cpd, ρa dpa (3.64)

23 Thermodynamic Energy Equation κ Differentiate θv Tv 000 pa with respect to time = dθv = dtv κ κ dp θ d Tv κ a v Tv pa p = a p a Tv (3.65) κθv pa dpa Substitute into (3.64) and expand total derivative --> Thermodynamic energy equation dθv θ θ dq = v + ( v ) θ v v = t cpd, Tv (3.66) Multiply (3.66) by c pd, ρ a, continuity equation by c pd, θ v and sum ( cpd, ρaθv) c ρ θ ρ θ + ( v pd, a v)= a v t Tv dq (3.67) Define energy density (J m -3 ) E = c pd, ρ a θ v Substitute into (3.67) E t + ( ve)= ρa θ v Tv dq (3.68)

24 Thermodynamic Energy Equation Decompose terms (assume ρ a << ρa) ρa ρa θv = θv + θ v v = v+ v Substitute into (3.67) + + ρθ a v ρ θ ρ θ ρ θ a v dq av v ( av v)= t cpd, Tv (3.70) Expand and substitute continuity equation θv θ θ ρ θ v dq + ( v ) v + ( av v)= t ρa cpd, Tv (3.7) Subgrid scale turbulent flux divergence terms θ u v = K v θ θ h, xx v θ = K v v h, yy w θ v = Kh, zz x y (3.73) θv z

25 Thermodynamic Energy Equation Substitute v θ v = Kh θv into (3.7), remove overbars θv θ θ ρ θ v dq + ( v ) v = ( akh ) v + t ρa cpd, Tv (3.74) Rewrite diabatic energy source/sink term eh, θv θ θv ρa h θ v dq + ( v ) = n ( K ) v + t ρa cpd, Tv n= (3.76) where eh, dq dqn dqce dq f m dqdp s dq dq = solar ir = n= (3.75)

Chapter 5. Fundamentals of Atmospheric Modeling

Chapter 5. Fundamentals of Atmospheric Modeling Overhead Slides for Chapter 5 of Fundamentals of Atmospheric Modeling by Mark Z. Jacobson Department of Civil & Environmental Engineering Stanford University Stanford, CA 94305-4020 January 30, 2002 Altitude

More information

1 Introduction to Governing Equations 2 1a Methodology... 2

1 Introduction to Governing Equations 2 1a Methodology... 2 Contents 1 Introduction to Governing Equations 2 1a Methodology............................ 2 2 Equation of State 2 2a Mean and Turbulent Parts...................... 3 2b Reynolds Averaging.........................

More information

1/18/2011. Conservation of Momentum Conservation of Mass Conservation of Energy Scaling Analysis ESS227 Prof. Jin-Yi Yu

1/18/2011. Conservation of Momentum Conservation of Mass Conservation of Energy Scaling Analysis ESS227 Prof. Jin-Yi Yu Lecture 2: Basic Conservation Laws Conservation Law of Momentum Newton s 2 nd Law of Momentum = absolute velocity viewed in an inertial system = rate of change of Ua following the motion in an inertial

More information

1/3/2011. This course discusses the physical laws that govern atmosphere/ocean motions.

1/3/2011. This course discusses the physical laws that govern atmosphere/ocean motions. Lecture 1: Introduction and Review Dynamics and Kinematics Kinematics: The term kinematics means motion. Kinematics is the study of motion without regard for the cause. Dynamics: On the other hand, dynamics

More information

Conservation of Mass Conservation of Energy Scaling Analysis. ESS227 Prof. Jin-Yi Yu

Conservation of Mass Conservation of Energy Scaling Analysis. ESS227 Prof. Jin-Yi Yu Lecture 2: Basic Conservation Laws Conservation of Momentum Conservation of Mass Conservation of Energy Scaling Analysis Conservation Law of Momentum Newton s 2 nd Law of Momentum = absolute velocity viewed

More information

Project 3 Convection and Atmospheric Thermodynamics

Project 3 Convection and Atmospheric Thermodynamics 12.818 Project 3 Convection and Atmospheric Thermodynamics Lodovica Illari 1 Background The Earth is bathed in radiation from the Sun whose intensity peaks in the visible. In order to maintain energy balance

More information

Daniel J. Jacob, Models of Atmospheric Transport and Chemistry, 2007.

Daniel J. Jacob, Models of Atmospheric Transport and Chemistry, 2007. 1 0. CHEMICAL TRACER MODELS: AN INTRODUCTION Concentrations of chemicals in the atmosphere are affected by four general types of processes: transport, chemistry, emissions, and deposition. 3-D numerical

More information

Control Volume. Dynamics and Kinematics. Basic Conservation Laws. Lecture 1: Introduction and Review 1/24/2017

Control Volume. Dynamics and Kinematics. Basic Conservation Laws. Lecture 1: Introduction and Review 1/24/2017 Lecture 1: Introduction and Review Dynamics and Kinematics Kinematics: The term kinematics means motion. Kinematics is the study of motion without regard for the cause. Dynamics: On the other hand, dynamics

More information

Lecture 1: Introduction and Review

Lecture 1: Introduction and Review Lecture 1: Introduction and Review Review of fundamental mathematical tools Fundamental and apparent forces Dynamics and Kinematics Kinematics: The term kinematics means motion. Kinematics is the study

More information

Getting started: CFD notation

Getting started: CFD notation PDE of p-th order Getting started: CFD notation f ( u,x, t, u x 1,..., u x n, u, 2 u x 1 x 2,..., p u p ) = 0 scalar unknowns u = u(x, t), x R n, t R, n = 1,2,3 vector unknowns v = v(x, t), v R m, m =

More information

Lecture 3. Turbulent fluxes and TKE budgets (Garratt, Ch 2)

Lecture 3. Turbulent fluxes and TKE budgets (Garratt, Ch 2) Lecture 3. Turbulent fluxes and TKE budgets (Garratt, Ch 2) The ABL, though turbulent, is not homogeneous, and a critical role of turbulence is transport and mixing of air properties, especially in the

More information

PALM - Cloud Physics. Contents. PALM group. last update: Monday 21 st September, 2015

PALM - Cloud Physics. Contents. PALM group. last update: Monday 21 st September, 2015 PALM - Cloud Physics PALM group Institute of Meteorology and Climatology, Leibniz Universität Hannover last update: Monday 21 st September, 2015 PALM group PALM Seminar 1 / 16 Contents Motivation Approach

More information

Needs work : define boundary conditions and fluxes before, change slides Useful definitions and conservation equations

Needs work : define boundary conditions and fluxes before, change slides Useful definitions and conservation equations Needs work : define boundary conditions and fluxes before, change slides 1-2-3 Useful definitions and conservation equations Turbulent Kinetic energy The fluxes are crucial to define our boundary conditions,

More information

APPENDIX B. The primitive equations

APPENDIX B. The primitive equations APPENDIX B The primitive equations The physical and mathematical basis of all methods of dynamical atmospheric prediction lies in the principles of conservation of momentum, mass, and energy. Applied to

More information

Chapter 1. Governing Equations of GFD. 1.1 Mass continuity

Chapter 1. Governing Equations of GFD. 1.1 Mass continuity Chapter 1 Governing Equations of GFD The fluid dynamical governing equations consist of an equation for mass continuity, one for the momentum budget, and one or more additional equations to account for

More information

Chapter 4 Water Vapor

Chapter 4 Water Vapor Chapter 4 Water Vapor Chapter overview: Phases of water Vapor pressure at saturation Moisture variables o Mixing ratio, specific humidity, relative humidity, dew point temperature o Absolute vs. relative

More information

ESCI 485 Air/Sea Interaction Lesson 1 Stresses and Fluxes Dr. DeCaria

ESCI 485 Air/Sea Interaction Lesson 1 Stresses and Fluxes Dr. DeCaria ESCI 485 Air/Sea Interaction Lesson 1 Stresses and Fluxes Dr DeCaria References: An Introduction to Dynamic Meteorology, Holton MOMENTUM EQUATIONS The momentum equations governing the ocean or atmosphere

More information

Chapter 9: Differential Analysis

Chapter 9: Differential Analysis 9-1 Introduction 9-2 Conservation of Mass 9-3 The Stream Function 9-4 Conservation of Linear Momentum 9-5 Navier Stokes Equation 9-6 Differential Analysis Problems Recall 9-1 Introduction (1) Chap 5: Control

More information

P = 1 3 (σ xx + σ yy + σ zz ) = F A. It is created by the bombardment of the surface by molecules of fluid.

P = 1 3 (σ xx + σ yy + σ zz ) = F A. It is created by the bombardment of the surface by molecules of fluid. CEE 3310 Thermodynamic Properties, Aug. 27, 2010 11 1.4 Review A fluid is a substance that can not support a shear stress. Liquids differ from gasses in that liquids that do not completely fill a container

More information

ATS 421/521. Climate Modeling. Spring 2015

ATS 421/521. Climate Modeling. Spring 2015 ATS 421/521 Climate Modeling Spring 2015 Lecture 9 Hadley Circulation (Held and Hou, 1980) General Circulation Models (tetbook chapter 3.2.3; course notes chapter 5.3) The Primitive Equations (tetbook

More information

Chapter 9: Differential Analysis of Fluid Flow

Chapter 9: Differential Analysis of Fluid Flow of Fluid Flow Objectives 1. Understand how the differential equations of mass and momentum conservation are derived. 2. Calculate the stream function and pressure field, and plot streamlines for a known

More information

NWP Equations (Adapted from UCAR/COMET Online Modules)

NWP Equations (Adapted from UCAR/COMET Online Modules) NWP Equations (Adapted from UCAR/COMET Online Modules) Certain physical laws of motion and conservation of energy (for example, Newton's Second Law of Motion and the First Law of Thermodynamics) govern

More information

2 Equations of Motion

2 Equations of Motion 2 Equations of Motion system. In this section, we will derive the six full equations of motion in a non-rotating, Cartesian coordinate 2.1 Six equations of motion (non-rotating, Cartesian coordinates)

More information

Chapter 3- Energy Balance and Temperature

Chapter 3- Energy Balance and Temperature Chapter 3- Energy Balance and Temperature Understanding Weather and Climate Aguado and Burt Influences on Insolation Absorption Reflection/Scattering Transmission 1 Absorption An absorber gains energy

More information

Isentropic flows and monsoonal circulations

Isentropic flows and monsoonal circulations Isentropic flows and monsoonal circulations Olivier Pauluis (NYU) Monsoons- Past, Present and future May 20th, 2015 Caltech, Pasadena Outline Introduction Global monsoon in isentropic coordinates Dry ventilation

More information

From the last time, we ended with an expression for the energy equation. u = ρg u + (τ u) q (9.1)

From the last time, we ended with an expression for the energy equation. u = ρg u + (τ u) q (9.1) Lecture 9 9. Administration None. 9. Continuation of energy equation From the last time, we ended with an expression for the energy equation ρ D (e + ) u = ρg u + (τ u) q (9.) Where ρg u changes in potential

More information

Fundamentals of Atmospheric Modelling

Fundamentals of Atmospheric Modelling M.Sc. in Computational Science Fundamentals of Atmospheric Modelling Peter Lynch, Met Éireann Mathematical Computation Laboratory (Opp. Room 30) Dept. of Maths. Physics, UCD, Belfield. January April, 2004.

More information

Prof. Simon Tett, Chair of Earth System Dynamics & Modelling: The University of Edinburgh

Prof. Simon Tett, Chair of Earth System Dynamics & Modelling: The University of Edinburgh SAGES Scottish Alliance for Geoscience, Environment & Society Modelling Climate Change Prof. Simon Tett, Chair of Earth System Dynamics & Modelling: The University of Edinburgh Climate Modelling Climate

More information

Introduction to Fluid Dynamics

Introduction to Fluid Dynamics Introduction to Fluid Dynamics Roger K. Smith Skript - auf englisch! Umsonst im Internet http://www.meteo.physik.uni-muenchen.de Wählen: Lehre Manuskripte Download User Name: meteo Password: download Aim

More information

Chapter 17. Fundamentals of Atmospheric Modeling

Chapter 17. Fundamentals of Atmospheric Modeling Overhead Slides for Chapter 17 of Fundamentals of Atmospheric Modeling by Mark Z. Jacobson Department of Civil & Environmental Engineering Stanford University Stanford, CA 94305-4020 August 21, 1998 Mass

More information

Numerical Example An air parcel with mass of 1 kg rises adiabatically from sea level to an altitude of 3 km. What is its temperature change?

Numerical Example An air parcel with mass of 1 kg rises adiabatically from sea level to an altitude of 3 km. What is its temperature change? Numerical Example An air parcel with mass of 1 kg rises adiabatically from sea level to an altitude of 3 km. What is its temperature change? From the 1 st law, T = -g/c p z + Q/m air /c p Here, Q = 0,

More information

Mathematical Concepts & Notation

Mathematical Concepts & Notation Mathematical Concepts & Notation Appendix A: Notation x, δx: a small change in x t : the partial derivative with respect to t holding the other variables fixed d : the time derivative of a quantity that

More information

Dynamics and Kinematics

Dynamics and Kinematics Geophysics Fluid Dynamics () Syllabus Course Time Lectures: Tu, Th 09:30-10:50 Discussion: 3315 Croul Hall Text Book J. R. Holton, "An introduction to Dynamic Meteorology", Academic Press (Ch. 1, 2, 3,

More information

ATMO/OPTI 656b Spring 09. Physical properties of the atmosphere

ATMO/OPTI 656b Spring 09. Physical properties of the atmosphere The vertical structure of the atmosphere. Physical properties of the atmosphere To first order, the gas pressure at the bottom of an atmospheric column balances the downward force of gravity on the column.

More information

Chapter 5. The Differential Forms of the Fundamental Laws

Chapter 5. The Differential Forms of the Fundamental Laws Chapter 5 The Differential Forms of the Fundamental Laws 1 5.1 Introduction Two primary methods in deriving the differential forms of fundamental laws: Gauss s Theorem: Allows area integrals of the equations

More information

z g + F w (2.56) p(x, y, z, t) = p(z) + p (x, y, z, t) (2.120) ρ(x, y, z, t) = ρ(z) + ρ (x, y, z, t), (2.121)

z g + F w (2.56) p(x, y, z, t) = p(z) + p (x, y, z, t) (2.120) ρ(x, y, z, t) = ρ(z) + ρ (x, y, z, t), (2.121) = + dw dt = 1 ρ p z g + F w (.56) Let us describe the total pressure p and density ρ as the sum of a horizontally homogeneous base state pressure and density, and a deviation from this base state, that

More information

ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY. Lecture 19. Learning objectives: develop a physical understanding of ocean thermodynamic processes

ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY. Lecture 19. Learning objectives: develop a physical understanding of ocean thermodynamic processes ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY Lecture 19 Learning objectives: develop a physical understanding of ocean thermodynamic processes 1. Ocean surface heat fluxes; 2. Mixed layer temperature

More information

2. Conservation of Mass

2. Conservation of Mass 2 Conservation of Mass The equation of mass conservation expresses a budget for the addition and removal of mass from a defined region of fluid Consider a fixed, non-deforming volume of fluid, V, called

More information

OCN/ATM/ESS 587. Ocean circulation, dynamics and thermodynamics.

OCN/ATM/ESS 587. Ocean circulation, dynamics and thermodynamics. OCN/ATM/ESS 587 Ocean circulation, dynamics and thermodynamics. Equation of state for seawater General T/S properties of the upper ocean Heat balance of the upper ocean Upper ocean circulation Deep circulation

More information

Mathematical Theory of Non-Newtonian Fluid

Mathematical Theory of Non-Newtonian Fluid Mathematical Theory of Non-Newtonian Fluid 1. Derivation of the Incompressible Fluid Dynamics 2. Existence of Non-Newtonian Flow and its Dynamics 3. Existence in the Domain with Boundary Hyeong Ohk Bae

More information

Parcel Model. Atmospheric Sciences September 30, 2012

Parcel Model. Atmospheric Sciences September 30, 2012 Parcel Model Atmospheric Sciences 6150 September 30, 2012 1 Governing Equations for Precipitating Convection For precipitating convection, we have the following set of equations for potential temperature,

More information

Atmospheric Sciences 321. Science of Climate. Lecture 13: Surface Energy Balance Chapter 4

Atmospheric Sciences 321. Science of Climate. Lecture 13: Surface Energy Balance Chapter 4 Atmospheric Sciences 321 Science of Climate Lecture 13: Surface Energy Balance Chapter 4 Community Business Check the assignments HW #4 due Wednesday Quiz #2 Wednesday Mid Term is Wednesday May 6 Practice

More information

wavelength (nm)

wavelength (nm) Blackbody radiation Everything with a temperature above absolute zero emits electromagnetic radiation. This phenomenon is called blackbody radiation. The intensity and the peak wavelength of the radiation

More information

The perturbation pressure, p, can be represented as the sum of a hydrostatic pressure perturbation p h and a nonhydrostatic pressure perturbation p nh

The perturbation pressure, p, can be represented as the sum of a hydrostatic pressure perturbation p h and a nonhydrostatic pressure perturbation p nh z = The perturbation pressure, p, can be represented as the sum of a hydrostatic pressure perturbation p h and a nonhydrostatic pressure perturbation p nh, that is, p = p h + p nh. (.1) The former arises

More information

1. The vertical structure of the atmosphere. Temperature profile.

1. The vertical structure of the atmosphere. Temperature profile. Lecture 4. The structure of the atmosphere. Air in motion. Objectives: 1. The vertical structure of the atmosphere. Temperature profile. 2. Temperature in the lower atmosphere: dry adiabatic lapse rate.

More information

A Simple Turbulence Closure Model

A Simple Turbulence Closure Model A Simple Turbulence Closure Model Atmospheric Sciences 6150 1 Cartesian Tensor Notation Reynolds decomposition of velocity: Mean velocity: Turbulent velocity: Gradient operator: Advection operator: V =

More information

Fluid dynamics and moist thermodynamics

Fluid dynamics and moist thermodynamics Chapter 1 Fluid dynamics and moist thermodynamics In this chapter we review the equations that represent the physical laws governing atmospheric motion. Rigorous derivations of the equations may be found

More information

τ xz = τ measured close to the the surface (often at z=5m) these three scales represent inner unit or near wall normalization

τ xz = τ measured close to the the surface (often at z=5m) these three scales represent inner unit or near wall normalization τ xz = τ measured close to the the surface (often at z=5m) these three scales represent inner unit or near wall normalization Note that w *3 /z i is used to normalized the TKE equation in case of free

More information

A Simple Turbulence Closure Model. Atmospheric Sciences 6150

A Simple Turbulence Closure Model. Atmospheric Sciences 6150 A Simple Turbulence Closure Model Atmospheric Sciences 6150 1 Cartesian Tensor Notation Reynolds decomposition of velocity: V = V + v V = U i + u i Mean velocity: V = Ui + V j + W k =(U, V, W ) U i =(U

More information

Geophysics Fluid Dynamics (ESS228)

Geophysics Fluid Dynamics (ESS228) Geophysics Fluid Dynamics (ESS228) Course Time Lectures: Tu, Th 09:30-10:50 Discussion: 3315 Croul Hall Text Book J. R. Holton, "An introduction to Dynamic Meteorology", Academic Press (Ch. 1, 2, 3, 4,

More information

Chapter 7: Thermodynamics

Chapter 7: Thermodynamics Chapter 7: Thermodynamics 7.1 Sea surface heat budget In Chapter 5, we have introduced the oceanic planetary boundary layer-the Ekman layer. The observed T and S in this layer are almost uniform vertically,

More information

Advection, Conservation, Conserved Physical Quantities, Wave Equations

Advection, Conservation, Conserved Physical Quantities, Wave Equations EP711 Supplementary Material Thursday, September 4, 2014 Advection, Conservation, Conserved Physical Quantities, Wave Equations Jonathan B. Snively!Embry-Riddle Aeronautical University Contents EP711 Supplementary

More information

Today s Lecture: Atmosphere finish primitive equations, mostly thermodynamics

Today s Lecture: Atmosphere finish primitive equations, mostly thermodynamics Today s Lecture: Atmosphere finish primitive equations, mostly thermodynamics Reference Peixoto and Oort, Sec. 3.1, 3.2, 3.4, 3.5 (but skip the discussion of oceans until next week); Ch. 10 Thermodynamic

More information

Reynolds Averaging. We separate the dynamical fields into slowly varying mean fields and rapidly varying turbulent components.

Reynolds Averaging. We separate the dynamical fields into slowly varying mean fields and rapidly varying turbulent components. Reynolds Averaging Reynolds Averaging We separate the dynamical fields into sloly varying mean fields and rapidly varying turbulent components. Reynolds Averaging We separate the dynamical fields into

More information

OCEAN MODELING II. Parameterizations

OCEAN MODELING II. Parameterizations OCEAN MODELING II Parameterizations Gokhan Danabasoglu Oceanography Section Climate and Global Dynamics Division National Center for Atmospheric Research NCAR is sponsored by the National Science Foundation

More information

CHAPTER 8 NUMERICAL SIMULATIONS OF THE ITCZ OVER THE INDIAN OCEAN AND INDONESIA DURING A NORMAL YEAR AND DURING AN ENSO YEAR

CHAPTER 8 NUMERICAL SIMULATIONS OF THE ITCZ OVER THE INDIAN OCEAN AND INDONESIA DURING A NORMAL YEAR AND DURING AN ENSO YEAR CHAPTER 8 NUMERICAL SIMULATIONS OF THE ITCZ OVER THE INDIAN OCEAN AND INDONESIA DURING A NORMAL YEAR AND DURING AN ENSO YEAR In this chapter, comparisons between the model-produced and analyzed streamlines,

More information

Multi-Scale Modeling of Turbulence and Microphysics in Clouds. Steven K. Krueger University of Utah

Multi-Scale Modeling of Turbulence and Microphysics in Clouds. Steven K. Krueger University of Utah Multi-Scale Modeling of Turbulence and Microphysics in Clouds Steven K. Krueger University of Utah 10,000 km Scales of Atmospheric Motion 1000 km 100 km 10 km 1 km 100 m 10 m 1 m 100 mm 10 mm 1 mm Planetary

More information

Scale analysis of the vertical equation of motion:

Scale analysis of the vertical equation of motion: Scale analysis of the vertical equation of motion: As we did with the hz eqns, we do for the vertical to estimate the order of magnitude of Dw/ we take the largest of the terms, Dw -- W/T h UW/L W 2 /H

More information

A Discussion on The Effect of Mesh Resolution on Convective Boundary Layer Statistics and Structures Generated by Large-Eddy Simulation by Sullivan

A Discussion on The Effect of Mesh Resolution on Convective Boundary Layer Statistics and Structures Generated by Large-Eddy Simulation by Sullivan 耶鲁 - 南京信息工程大学大气环境中心 Yale-NUIST Center on Atmospheric Environment A Discussion on The Effect of Mesh Resolution on Convective Boundary Layer Statistics and Structures Generated by Large-Eddy Simulation

More information

CAM-SE: Lecture I. Peter Hjort Lauritzen

CAM-SE: Lecture I. Peter Hjort Lauritzen CAM-SE: Lecture I Peter Hjort Lauritzen Atmospheric Modeling and Predictability Section Climate and Global Dynamics Laboratory National Center for Atmospheric Research 2nd WCRP Summer School on Climate

More information

Chapter 4: Fluid Kinematics

Chapter 4: Fluid Kinematics Overview Fluid kinematics deals with the motion of fluids without considering the forces and moments which create the motion. Items discussed in this Chapter. Material derivative and its relationship to

More information

ρ x + fv f 'w + F x ρ y fu + F y Fundamental Equation in z coordinate p = ρrt or pα = RT Du uv tanφ Dv Dt + u2 tanφ + vw a a = 1 p Dw Dt u2 + v 2

ρ x + fv f 'w + F x ρ y fu + F y Fundamental Equation in z coordinate p = ρrt or pα = RT Du uv tanφ Dv Dt + u2 tanφ + vw a a = 1 p Dw Dt u2 + v 2 Fundamental Equation in z coordinate p = ρrt or pα = RT Du uv tanφ + uw Dt a a = 1 p ρ x + fv f 'w + F x Dv Dt + u2 tanφ + vw a a = 1 p ρ y fu + F y Dw Dt u2 + v 2 = 1 p a ρ z g + f 'u + F z Dρ Dt + ρ

More information

AA210A Fundamentals of Compressible Flow. Chapter 1 - Introduction to fluid flow

AA210A Fundamentals of Compressible Flow. Chapter 1 - Introduction to fluid flow AA210A Fundamentals of Compressible Flow Chapter 1 - Introduction to fluid flow 1 1.2 Conservation of mass Mass flux in the x-direction [ ρu ] = M L 3 L T = M L 2 T Momentum per unit volume Mass per unit

More information

ATMO 551a Fall The Carnot Cycle

ATMO 551a Fall The Carnot Cycle What is a arnot ycle and Why do we care The arnot ycle arnot was a French engineer who was trying to understand how to extract usable mechanical work from a heat engine, that is an engine where a gas or

More information

5. General Circulation Models

5. General Circulation Models 5. General Circulation Models I. 3-D Climate Models (General Circulation Models) To include the full three-dimensional aspect of climate, including the calculation of the dynamical transports, requires

More information

PDE Solvers for Fluid Flow

PDE Solvers for Fluid Flow PDE Solvers for Fluid Flow issues and algorithms for the Streaming Supercomputer Eran Guendelman February 5, 2002 Topics Equations for incompressible fluid flow 3 model PDEs: Hyperbolic, Elliptic, Parabolic

More information

Math background. Physics. Simulation. Related phenomena. Frontiers in graphics. Rigid fluids

Math background. Physics. Simulation. Related phenomena. Frontiers in graphics. Rigid fluids Fluid dynamics Math background Physics Simulation Related phenomena Frontiers in graphics Rigid fluids Fields Domain Ω R2 Scalar field f :Ω R Vector field f : Ω R2 Types of derivatives Derivatives measure

More information

References: Parcel Theory. Vertical Force Balance. ESCI Cloud Physics and Precipitation Processes Lesson 3 - Stability and Buoyancy Dr.

References: Parcel Theory. Vertical Force Balance. ESCI Cloud Physics and Precipitation Processes Lesson 3 - Stability and Buoyancy Dr. References: ESCI 340 - Cloud Physics and Precipitation Processes Lesson 3 - Stability and Buoyancy Dr. DeCaria Glossary of Meteorology, 2nd ed., American Meteorological Society A Short Course in Cloud

More information

Meteorology 6150 Cloud System Modeling

Meteorology 6150 Cloud System Modeling Meteorology 6150 Cloud System Modeling Steve Krueger Spring 2009 1 Fundamental Equations 1.1 The Basic Equations 1.1.1 Equation of motion The movement of air in the atmosphere is governed by Newton s Second

More information

Lecture 3: 1. Lecture 3.

Lecture 3: 1. Lecture 3. Lecture 3: 1 Lecture 3. Lecture 3: 2 Plan for today Summary of the key points of the last lecture. Review of vector and tensor products : the dot product (or inner product ) and the cross product (or vector

More information

Chapter 2. Quasi-Geostrophic Theory: Formulation (review) ε =U f o L <<1, β = 2Ω cosθ o R. 2.1 Introduction

Chapter 2. Quasi-Geostrophic Theory: Formulation (review) ε =U f o L <<1, β = 2Ω cosθ o R. 2.1 Introduction Chapter 2. Quasi-Geostrophic Theory: Formulation (review) 2.1 Introduction For most of the course we will be concerned with instabilities that an be analyzed by the quasi-geostrophic equations. These are

More information

2. Conservation laws and basic equations

2. Conservation laws and basic equations 2. Conservation laws and basic equations Equatorial region is mapped well by cylindrical (Mercator) projection: eastward, northward, upward (local Cartesian) coordinates:,, velocity vector:,,,, material

More information

Lagrangian description from the perspective of a parcel moving within the flow. Streamline Eulerian, tangent line to instantaneous velocity field.

Lagrangian description from the perspective of a parcel moving within the flow. Streamline Eulerian, tangent line to instantaneous velocity field. Chapter 2 Hydrostatics 2.1 Review Eulerian description from the perspective of fixed points within a reference frame. Lagrangian description from the perspective of a parcel moving within the flow. Streamline

More information

Convection and buoyancy oscillation

Convection and buoyancy oscillation Convection and buoyancy oscillation Recap: We analyzed the static stability of a vertical profile by the "parcel method"; For a given environmental profile (of T 0, p 0, θ 0, etc.), if the density of an

More information

Course , General Circulation of the Earth's Atmosphere Prof. Peter Stone Section 4: Water Vapor Budget

Course , General Circulation of the Earth's Atmosphere Prof. Peter Stone Section 4: Water Vapor Budget Course 12.812, General Circulation of the Earth's Atmosphere Prof. Peter Stone Section 4: Water Vapor Budget Water Vapor Distribution First let us look at the distribution of specific humidity, q. The

More information

A Global Atmospheric Model. Joe Tribbia NCAR Turbulence Summer School July 2008

A Global Atmospheric Model. Joe Tribbia NCAR Turbulence Summer School July 2008 A Global Atmospheric Model Joe Tribbia NCAR Turbulence Summer School July 2008 Outline Broad overview of what is in a global climate/weather model of the atmosphere Spectral dynamical core Some results-climate

More information

Governing Equations and Scaling in the Tropics

Governing Equations and Scaling in the Tropics Governing Equations and Scaling in the Tropics M 1 ( ) e R ε er Tropical v Midlatitude Meteorology Why is the general circulation and synoptic weather systems in the tropics different to the those in the

More information

Atmospheric Thermodynamics

Atmospheric Thermodynamics Atmospheric Thermodynamics Atmospheric Composition What is the composition of the Earth s atmosphere? Gaseous Constituents of the Earth s atmosphere (dry air) Constituent Molecular Weight Fractional Concentration

More information

Introduction to Partial Differential Equations

Introduction to Partial Differential Equations Introduction to Partial Differential Equations Philippe B. Laval KSU Current Semester Philippe B. Laval (KSU) 1D Heat Equation: Derivation Current Semester 1 / 19 Introduction The derivation of the heat

More information

Lecture 3: Light and Temperature

Lecture 3: Light and Temperature Lecture 3: Light and Temperature terrestrial radiative cooling Solar radiative warming (Light) Global Temperature atmosphere ocean land Light Temperature Different forms of energy Energy conservation energy,

More information

2σ e s (r,t) = e s (T)exp( rr v ρ l T ) = exp( ) 2σ R v ρ l Tln(e/e s (T)) e s (f H2 O,r,T) = f H2 O

2σ e s (r,t) = e s (T)exp( rr v ρ l T ) = exp( ) 2σ R v ρ l Tln(e/e s (T)) e s (f H2 O,r,T) = f H2 O Formulas/Constants, Physics/Oceanography 4510/5510 B Atmospheric Physics II N A = 6.02 10 23 molecules/mole (Avogadro s number) 1 mb = 100 Pa 1 Pa = 1 N/m 2 Γ d = 9.8 o C/km (dry adiabatic lapse rate)

More information

Thermodynamics Review [?] Entropy & thermodynamic potentials Hydrostatic equilibrium & buoyancy Stability [dry & moist adiabatic]

Thermodynamics Review [?] Entropy & thermodynamic potentials Hydrostatic equilibrium & buoyancy Stability [dry & moist adiabatic] Thermodynamics Review [?] Entropy & thermodynamic potentials Hydrostatic equilibrium & buoyancy Stability [dry & moist adiabatic] Entropy 1. (Thermodynamics) a thermodynamic quantity that changes in a

More information

Chapter 1. Continuum mechanics review. 1.1 Definitions and nomenclature

Chapter 1. Continuum mechanics review. 1.1 Definitions and nomenclature Chapter 1 Continuum mechanics review We will assume some familiarity with continuum mechanics as discussed in the context of an introductory geodynamics course; a good reference for such problems is Turcotte

More information

Candidates must show on each answer book the type of calculator used. Log Tables, Statistical Tables and Graph Paper are available on request.

Candidates must show on each answer book the type of calculator used. Log Tables, Statistical Tables and Graph Paper are available on request. UNIVERSITY OF EAST ANGLIA School of Mathematics Spring Semester Examination 2004 FLUID DYNAMICS Time allowed: 3 hours Attempt Question 1 and FOUR other questions. Candidates must show on each answer book

More information

Open boundary conditions in numerical simulations of unsteady incompressible flow

Open boundary conditions in numerical simulations of unsteady incompressible flow Open boundary conditions in numerical simulations of unsteady incompressible flow M. P. Kirkpatrick S. W. Armfield Abstract In numerical simulations of unsteady incompressible flow, mass conservation can

More information

Convection. forced convection when the flow is caused by external means, such as by a fan, a pump, or atmospheric winds.

Convection. forced convection when the flow is caused by external means, such as by a fan, a pump, or atmospheric winds. Convection The convection heat transfer mode is comprised of two mechanisms. In addition to energy transfer due to random molecular motion (diffusion), energy is also transferred by the bulk, or macroscopic,

More information

Chapter 5. Sound Waves and Vortices. 5.1 Sound waves

Chapter 5. Sound Waves and Vortices. 5.1 Sound waves Chapter 5 Sound Waves and Vortices In this chapter we explore a set of characteristic solutions to the uid equations with the goal of familiarizing the reader with typical behaviors in uid dynamics. Sound

More information

TURBULENT KINETIC ENERGY

TURBULENT KINETIC ENERGY TURBULENT KINETIC ENERGY THE CLOSURE PROBLEM Prognostic Moment Equation Number Number of Ea. fg[i Q! Ilial.!.IokoQlI!!ol Ui au. First = at au.'u.' '_J_ ax j 3 6 ui'u/ au.'u.' a u.'u.'u k ' Second ' J =

More information

ATMOSPHERIC AND OCEANIC FLUID DYNAMICS

ATMOSPHERIC AND OCEANIC FLUID DYNAMICS ATMOSPHERIC AND OCEANIC FLUID DYNAMICS Fundamentals and Large-scale Circulation G E O F F R E Y K. V A L L I S Princeton University, New Jersey CAMBRIDGE UNIVERSITY PRESS An asterisk indicates more advanced

More information

Løsningsforslag: oppgavesett kap. 9 (2 av 3) GEF2200

Løsningsforslag: oppgavesett kap. 9 (2 av 3) GEF2200 Løsningsforslag: oppgavesett kap. 9 (2 av 3) GEF2200 s.m.blichner@geo.uio.no Oppgave 1 a) The turbulent vertical flux of sensible heat (Q H ) in the atmospheric boundary layer often takes place through

More information

Principles of Convection

Principles of Convection Principles of Convection Point Conduction & convection are similar both require the presence of a material medium. But convection requires the presence of fluid motion. Heat transfer through the: Solid

More information

Overview of fundamental atmospheric concepts

Overview of fundamental atmospheric concepts Fundamentals of Earth s Atmosphere AOSC 433/633 & CHEM 433/633 Tim Canty Class Web Site: http://www.atmos.umd.edu/~rjs/class/spr2013 Notes: Ross, Tim, & Allison co-teach this class; please include all

More information

Convective Fluxes: Sensible and Latent Heat Convective Fluxes Convective fluxes require Vertical gradient of temperature / water AND Turbulence ( mixing ) Vertical gradient, but no turbulence: only very

More information

1. Composition and Structure

1. Composition and Structure Atmospheric sciences focuses on understanding the atmosphere of the earth and other planets. The motivations for studying atmospheric sciences are largely: weather forecasting, climate studies, atmospheric

More information

Using Cloud-Resolving Models for Parameterization Development

Using Cloud-Resolving Models for Parameterization Development Using Cloud-Resolving Models for Parameterization Development Steven K. Krueger University of Utah! 16th CMMAP Team Meeting January 7-9, 2014 What is are CRMs and why do we need them? Range of scales diagram

More information

where p oo is a reference level constant pressure (often 10 5 Pa). Since θ is conserved for adiabatic motions, a prognostic temperature equation is:

where p oo is a reference level constant pressure (often 10 5 Pa). Since θ is conserved for adiabatic motions, a prognostic temperature equation is: 1 Appendix C Useful Equations Purposes: Provide foundation equations and sketch some derivations. These equations are used as starting places for discussions in various parts of the book. C.1. Thermodynamic

More information

Soft Bodies. Good approximation for hard ones. approximation breaks when objects break, or deform. Generalization: soft (deformable) bodies

Soft Bodies. Good approximation for hard ones. approximation breaks when objects break, or deform. Generalization: soft (deformable) bodies Soft-Body Physics Soft Bodies Realistic objects are not purely rigid. Good approximation for hard ones. approximation breaks when objects break, or deform. Generalization: soft (deformable) bodies Deformed

More information

Clouds and turbulent moist convection

Clouds and turbulent moist convection Clouds and turbulent moist convection Lecture 2: Cloud formation and Physics Caroline Muller Les Houches summer school Lectures Outline : Cloud fundamentals - global distribution, types, visualization

More information

f self = 1/T self (b) With revolution, rotaton period T rot in second and the frequency Ω rot are T yr T yr + T day T rot = T self > f self

f self = 1/T self (b) With revolution, rotaton period T rot in second and the frequency Ω rot are T yr T yr + T day T rot = T self > f self Problem : Units : Q-a Mathematically exress the relationshi between the different units of the hysical variables: i) Temerature: ) Fahrenheit and Celsius; 2) Fahrenheit and Kelvin ii) Length: ) foot and

More information

Quick Recapitulation of Fluid Mechanics

Quick Recapitulation of Fluid Mechanics Quick Recapitulation of Fluid Mechanics Amey Joshi 07-Feb-018 1 Equations of ideal fluids onsider a volume element of a fluid of density ρ. If there are no sources or sinks in, the mass in it will change

More information