Modeling Large-Scale Atmospheric and Oceanic Flows 2
|
|
- Christian Jennings
- 5 years ago
- Views:
Transcription
1 Modeling Large-Scale Atmospheric and Oceanic Flows V. Zeitlin known s of the Laboratoire de Météorologie Dynamique, Univ. P. and M. Curie, Paris Mathematics of the Oceans, Fields Institute, Toronto, 3 jet
2 Plan known s of the jet of dry and moist instabilities known s of the jet
3 General problematics Importance of moisture in the atmosphere: obvious. Influences large-scale dynamics via the latent heat release, due to condensation and precipitation. Atmospheric circulation ing: equation of state of the moist air extremely complex. Discretization/averaging: problematic. Current parametrizations of precipitations and latent heat release: relaxation to the equilibrium (saturation) profile of humidity threshold effect essential nonlinearity Consequences: no linear limit; linear thinking: modal decomposition, linear stability analysis, etc impossible problems in quantifying predictability of moist - convective dynamical systems. known s of the jet
4 Aims and method I Aim: Understanding the influence of condensation and latent heat release upon large-scale dynamical processes Reminder: Simplest for large-scale motions: rotating shallow water. Link with primitive equations: vertical averaging Baroclinic effects: (or more) layers. Problem with this approach for moist air: averaging of essentially nonlinear equation of state. known s of the jet
5 Aims and method II Our approach Combine (standard) vertical averaging of primitive equations between the isobaric surfaces with that of Lagrangian conservation of moist enthalpy Allow for convective fluxes (extra vertical velocity) across the isobars Link these fluxes to condensation Use relaxation parametrization in terms of bulk moisture in the layer for the condensation/precipitation known s of the jet
6 Aims and method III Advantages: Simplicity, qualitative analysis of basic phenomena straightforward Fully nonlinear in the hydrodynamic sector Well-adapted for studying discontinuities, in particular precipitation s Efficient numerical tools available (finite-volume codes for shallow water) Various limits giving known s Inclusion of topography (gentle or steep) straightforward known s of the jet
7 Primitive equations in pseudo-height coordinates d dt v + f k v = φ d dt θ = v + z w = known s of the z φ = g θ θ v = (u, v) and w - horizontal and vertical velocities, d dt = t + v + w z, f - Coriolis parameter, θ - potential temperature, φ - geopotential. jet
8 Moisture and moist enthalpy Condensation turned off: conservation of specific humidity of the air parcel: d dt q =. Condensation turned on: θ and q equations acquire source and sink. Yet the moist enthalpy θ + L c p q, where L - latent heat release, c p - specific heat, is conserved for any air parcel on isobaric surfaces: d dt ( θ + L c p q ) =, known s of the jet
9 Vertical averaging with convective fluxes 3 material surfaces: w = dz dt, w = dz + W, w = dz + W. dt dt W known s z of the θ θ W z z jet Mean-field + constant mean θ
10 Averaged momentum and mass conservation equations: { t v + (v )v + f k v = φ(z ) + g θ θ z, t v + (v )v + f k v = φ(z ) + g θ { t h + (h v ) = W, t h + (h v ) = +W W, known s of the θ z + v v h W, jet
11 Linking convective fluxes to precipitation I Bulk humidity: Q i = z i z i qdz. Precipitation sink: t Q i + (Q i v i ) = P i. In precipitating regions (P i > ), moisture is saturated q(z i ) = q s (z i ) and the temperature of the air-mass W i dtdxdy convected due to the latent heat release θ(z i ) + L c p q s (z i ), is the one of the upper layer: θ i+. We assume "dry" stable background stratification: θ i+ = θ(z i ) + L c p q(z i ) θ i + L c p q(z i ) > θ i, with constant θ(z i ) and q(z i ). known s of the jet
12 Integrating the moist enthalpy we get W i = β i P i with a positive-definite coefficient β i = L c p (θ i+ θ i ) q(z i ) >. Last step: relaxation formula with relaxation time τ. known s of the P i = Q i Q s i τ H(Q i Q s i ) where H(.) is the Heaviside (step) function. jet
13 -layer with a dry upper layer Vertical boundary conditions: upper surface isobaric z = const, geopotential at the bottom constant (ground) φ(z ) = const, Q =, Q = Q: t v + (v )v + f k v = g (h + h ), t v + (v )v + f k v = g (h + αh ) + v v h βp, t h + (h v ) = βp, t h + (h v ) = +βp, t Q + (Qv ) = P, P = Q Qs τ H(Q Q s ) α = θ θ - stratification parameter. known s of the jet
14 Sketch of the θ W h known s of the θ P> h jet
15 Immediate relaxation limit τ, P = Q s v (Gill, 98), and t v + (v )v + f k v = g (h + h ), t v + (v )v + f k v = g (h + αh ) v v h βq s v, t h + (h v ) = +βq s v, t h + (h v ) = βq s v, humidity staying at the saturation value: Q = Q s. known s of the jet
16 Baroclinic reduction Rewriting the in terms of and barotropic velocities: v bt = h v + h v h + h, v bc = v v, and linearizing in the hydrodynamic sector gives: t v bc + f k v bc = g e η, t η + H e v bc = βp, t Q + Q e v bc = P, where g e = g(α ), Q e = He H Q s, η - perturbation of the interface, H e - equivalent height. Model first proposed by Gill (98) and studied by Majda et al (4, 6, 8)., known s of the jet
17 Quasigeostrophic limit In the small Rossby number limit on the β-plane Lapeyre & Held (4) follows: d () ( ψ + y η ) = βp, dt D D d () ( ψ + y η ) = βp, dt D D Here d () i dt = t + (v () i ), k v () i = ψ i, D i = H i H, and ψ, (geostrophic streamfunctions) are related to the free-surface (η ) and interface (η ) perturbations as: ψ = η + η, ψ = η + αη. known s of the jet
18 -layer moist-convective RSW In the limit H /(H + H ) the reduced-gravity one-layer moist-convective shallow water follows (Bouchut, Lambaerts, Lapeyre & Zeitlin, 9): t v + (v )v + f k v = η, t η + {v ( + η)} = βp, t Q + (Qv ) = P, (Nondimensional equations, η - free-surface perturbation) known s of the jet
19 Horizontal momentum ( t + v )(v h ) + v h v + f k (v h ) = g h gh h v βp, ( t + v )(v h ) + v h v + f k (v h ) = αg h gh h + v βp, Red: moist convection drag. Total momentum: v h + v h is not affected by convection. known s of the jet
20 Energy Energy densities of the layers: { e = h v + g h, e = h v + gh h + αg h, For the total energy E = dxdy(e + e ) we get: t E = dx βp (gh ( α) + (v v ) ). st term: production of PE (for stable stratification); nd term destruction of KE. known s of the jet
21 Potential vorticity ( t + v ) ζ + f h ( t + v ) ζ + f h = ζ + f h = ζ + f h βp, βp + k { ( v v βp h h where ζ i = k ( v i ) = x v i y u i (i =, )- relative vorticity. PV in each layer is not a Lagrangian invariant in precipitating regions. known s )}, of the jet
22 Moist enthalpy and moist PV Moist enthalpy in the lower layer: m = h βq and is always locally conserved: t m + (m v ) =. Conservation of the moist enthalpy in the lower layer allows to derive a new Lagrangian invariant, the moist PV: ( t + v ) ζ + f m =. known s of the jet
23 Quasilinear form and characteristic equations -d reduction: y (...) =, quasilinear system: t f + A(f ) x f = b(f ). Characteristic equation: det(a ci) = "Dry" characteristic equation } } F(c) = {(u c) gh {(u c) αgh gh gh =, "Moist" characteristic equation (τ ) F m (c) = F(c) + ((u u ) (α )gh )gβq s =. known s of the jet
24 Characteristic velocities about the rest state "Dry" characteristics: "Moist" characteristics: Here C = c and C ± = g(h + αh ) ±, C± m = g(h + αh ) ± m. = 4H H (α ) (H + αh ) = (H αh ) + 4H H (H + αh ). m = + 4(α )βqs H (H + αh ). known s of the jet
25 characteristic velocities c m is real for positive moist enthalpy of the lower layer in the state of rest : M = H βq s >, and C m < C < g(h + αh ) < C + < C m +, for < M < H moist internal (mainly ) mode propagates slower than the dry one, consistent with observations. known s of the jet
26 Discontinuities in dependent variables (no rotation) Rankine-Hugoniot (RH) conditions (immediate relaxation): s[v h + v h ] + [u v h + u v h ] =, s[m ] + [m u ] =, s[h ] + [h u + βq s u ] =. s - propagation speed of the discontinuity. Remark: mass conservation moist enthalpy conservation in the lower layer. b Due to lim xs a lim b xs a P =, P does not enter RH conditions for u, v, h. known s of the jet
27 Discontinuities in derivatives RH conditions linearized about the rest state: { (s C + )(s C )[ x u ] = (α )gh gβ[p], (s C m + )(s C m )[ x u ] = s(α )gh gβ[ x Q]. For a configuration where it rains at the right side of the discontinuity, P = and P + = Q s x u + >, there exist five types of precipitation s: known s of the jet
28 Precipitation s. the dry external s, C + < s < C m +,. the dry internal subsonic s, C m < s < C, 3. the moist internal subsonic s, C m < s <, 4. the moist internal supersonic s, C + < s < C, 5. the moist external s, s < C m +. This result confirms previous studies within a linear (Frierson et al, 4). known s of the jet
29 Wave scattering on a moisture : setting Localized internal simple wave centred at x P = and moving eastward: { u (x, ) = σ(x x P ) U + U if σ x x U P otherwise, U =., σ = () Stationary moisture at x M = 5, saturated air at the east, unsaturated at the west: Q(x, ) = Q s { + q tanh(x x M )H( x + x M )}, q =.5. () Strong downflow convergence in the lower layer P > near the moisture. σ, known s of the jet
30 t t Wave scattering on a moisture : velocity and moisture x known s of the u bc x Q x jet
31 t t t t Wave scattering on a moisture : condensation zone I s s r i x r m i x x r i x x Dry and moist internal Riemann invariants. s, - precipitation s (dry subsonic and moist supersonic) r m i x x known s of the jet
32 Characteristics and s in the condensation zone t Q<Qs Q=Qs known s S S3 of the P= P> P= Cd Cm Q<Qs Cq Q=Qs S x jet
33 Evaporation and its parametrizations In the presence of evaporation source E t Q + (Qv ) = E P Hence: t m + (m v ) = βe Simple parametrizations of E (may be combined): Relaxational: E = ˆQ Q τ E H(m ), where ˆQ - equilibrium value. Dynamic: E = α E v H(m ) m should stay positive (plays a role of static stability) known s of the jet
34 Baroclinic Bickley jet Geostrophically balanced upper-layer jet on the f -plane. non-dimensional profiles of velocity and thikness perturbations: ū =, η = α tanh(y), ū = sech (y), η = α tanh(y). No deviation of the free surface: η + η =. Parameters: Ro =., Bu = - typical for atmospheric jets. known s of the jet
35 u i /U η i /H PV i /fh y/r d 3 3 y/r d 3 3 y/r d Bickley jet: zonal velocity ū i, thickness deviation η i and PV anomaly. Lower (upper) layer: solid black (dashed gray). known s of the jet
36 Linear stability diagram c p σ k k Phase velocity (top) and growth rate (bottom) known s of the jet
37 The most unstable mode y/r d y/r d x/r d x/r d Most unstable mode of the upper-layer Bickley jet. Upper(top) and lower (bottom) layer- geostrophic streamfunctions and velocity (arrows) fields. ψ ψ known s of the jet
38 Early stages: evolution of moisture.5 (a) (c) T i T i x (b) (d) T i 3T i Evolution of the moisture anomaly Q Q with superimposed lower-layer velocity. Black contour: condensation zones x known s of the jet
39 Early stages: growth rates σ/ro Dry Moist known s of the t/t i Red: moist, blue: dry simulations. Transient increase in the growth rate due to condensation. jet
40 Cyclone-anticyclone asymmetry <ζ 3 >/<ζ > 3/ <ζ 3 >/<ζ > 3/ t/t i 6 4 UPPER LAYER LOWER LAYER 5 5 t/t i Skewness of relative vorticity. Red: moist, blue: dry simulations. known s of the jet
41 How condensation enhances cyclones: -layer For Ro and Bu O(), close to saturation ψ q << : [ ] ( t + v () ) ψ ψ = βp, (3) [ ] ( t + v () ) q Q s ψ = P, (4) v () = ( y ψ, x ψ) - geostrophic velocity, ψ = η + η, and q is moisture anomaly with respect to Q s. PV of the fluid columns which pass through the precipitating regions increases. For τ q, and: [ ] Q s ( t + v () ) ψ P τ >, (5) increase of geostrophic vorticity in the precipitation regions. known s of the jet
42 Dry vs moist simulations: evolution of relative vorticity (a) Dry (b) Moist (c) T i (d) T i known s of the (e) 5T i (f) 5T i (g) 3T i 35T i (h) 3T i 35T i jet Lower layer: colors, upper layer: contours. Condensation: solid black.
43 Dry vs moist simulations: formation of secondary zonal jets at late stages Dry.5 Moist known s of the 4T i T i jet 8T i T i.5.5.5
44 x Unbalanced (aheostrophic) motions: divergence (a) Dry (b) Moist (c) T i x 3 (d) T i known s of the 5T i 5T i (e) (f) (g) 3T i (h) 3T i 35T i 35T i jet
45 Moist in Nature known s of the jet
46 The Physically and mathematically consistent Simple, physics transparent Efficient high-resolution numerical schemes available Benchmarks: good known s of the jet
47 local enhancement of the growth rate of the moist-convective at the precipitation onset, significant increase in intensity of ageostrophic motions during the evolution of the moist, substantial cyclone - anticyclone asymmetry, which develops due to the moist convection effects. substantial differences in the structure of zonal jets resulting at the late stage of saturation. known s of the jet
48 References Presentation based on: Lambaerts J.; Lapeyre G.; Zeitlin V. and Bouchut F. "Simplified two-layer s of precipitating atmosphere and their properties" Phys. Fluids 3, 4663,. Lambaerts J.; Lapeyre G. and Zeitlin V. "Moist versus Dry Baroclinic Instability in a Simplified Two-Layer Atmospheric Model with Condensation and Latent Heat Release" J. Atmos. Sci. 69, 45-46,. known s of the jet
Influence of condensation and latent heat release upon barotropic and baroclinic instabilities of vortices in a rotating shallow water f-plane model
Influence of condensation and latent heat release upon barotropic and baroclinic instabilities of vortices in a rotating shallow water f-plane model Masoud Rostami, Vladimir Zeitlin To cite this version:
More informationUnderstanding inertial instability on the f-plane with complete Coriolis force
Understanding inertial instability on the f-plane with complete Coriolis force Abstract Vladimir Zeitlin Laboratory of Dynamical Meteorology, University P. and M. Curie and Ecole Normale Supérieure, Paris,
More informationAsymmetric inertial instability
Asymmetric inertial instability V. Zeitlin Institut Universitaire de France 2 Laboratory of Dynamical Meteorology, University P. and M. Curie, Paris, France UCL, December 2 Instabilities of jets Motivations,
More informationAtmospheric dynamics and meteorology
Atmospheric dynamics and meteorology B. Legras, http://www.lmd.ens.fr/legras III Frontogenesis (pre requisite: quasi-geostrophic equation, baroclinic instability in the Eady and Phillips models ) Recommended
More information8/21/08. Modeling the General Circulation of the Atmosphere. Topic 4: Equatorial Wave Dynamics. Moisture and Equatorial Waves
Modeling the General Circulation of the Atmosphere. Topic 4: Equatorial Wave Dynamics D A R G A N M. W. F R I E R S O N U N I V E R S I T Y O F W A S H I N G T O N, D E P A R T M E N T O F A T M O S P
More informationDynamics 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 informationGeophysics 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 informationLecture 10a: The Hadley Cell
Lecture 10a: The Hadley Cell Geoff Vallis; notes by Jim Thomas and Geoff J. Stanley June 27 In this short lecture we take a look at the general circulation of the atmosphere, and in particular the Hadley
More informationIn two-dimensional barotropic flow, there is an exact relationship between mass
19. Baroclinic Instability In two-dimensional barotropic flow, there is an exact relationship between mass streamfunction ψ and the conserved quantity, vorticity (η) given by η = 2 ψ.the evolution of the
More information6 Two-layer shallow water theory.
6 Two-layer shallow water theory. Wewillnowgoontolookatashallowwatersystemthathastwolayersofdifferent density. This is the next level of complexity and a simple starting point for understanding the behaviour
More information2. Baroclinic Instability and Midlatitude Dynamics
2. Baroclinic Instability and Midlatitude Dynamics Midlatitude Jet Stream Climatology (Atlantic and Pacific) Copyright 26 Emily Shuckburgh, University of Cambridge. Not to be quoted or reproduced without
More informationGravity Waves. Lecture 5: Waves in Atmosphere. Waves in the Atmosphere and Oceans. Internal Gravity (Buoyancy) Waves 2/9/2017
Lecture 5: Waves in Atmosphere Perturbation Method Properties of Wave Shallow Water Model Gravity Waves Rossby Waves Waves in the Atmosphere and Oceans Restoring Force Conservation of potential temperature
More informationThe equation we worked with for waves and geostrophic adjustment of a 1-layer fluid is η tt
GEOPHYSICAL FLUID DYNAMICS-I OC512/AS509 2015 P.Rhines LECTUREs 11-12 week 6 9-14 Geostrophic adjustment and overturning circulations with continuous stratification. The equation we worked with for waves
More informationQuasi-equilibrium Theory of Small Perturbations to Radiative- Convective Equilibrium States
Quasi-equilibrium Theory of Small Perturbations to Radiative- Convective Equilibrium States See CalTech 2005 paper on course web site Free troposphere assumed to have moist adiabatic lapse rate (s* does
More informationTransformed Eulerian Mean
Chapter 15 Transformed Eulerian Mean In the last few lectures we introduced some fundamental ideas on 1) the properties of turbulent flows in rotating stratified environments, like the ocean and the atmosphere,
More informationBALANCED FLOW: EXAMPLES (PHH lecture 3) Potential Vorticity in the real atmosphere. Potential temperature θ. Rossby Ertel potential vorticity
BALANCED FLOW: EXAMPLES (PHH lecture 3) Potential Vorticity in the real atmosphere Need to introduce a new measure of the buoyancy Potential temperature θ In a compressible fluid, the relevant measure
More informationPAPER 333 FLUID DYNAMICS OF CLIMATE
MATHEMATICAL TRIPOS Part III Wednesday, 1 June, 2016 1:30 pm to 4:30 pm Draft 21 June, 2016 PAPER 333 FLUID DYNAMICS OF CLIMATE Attempt no more than THREE questions. There are FOUR questions in total.
More informationBoundary layer controls on extratropical cyclone development
Boundary layer controls on extratropical cyclone development R. S. Plant (With thanks to: I. A. Boutle and S. E. Belcher) 28th May 2010 University of East Anglia Outline Introduction and background Baroclinic
More informationRotating stratified turbulence in the Earth s atmosphere
Rotating stratified turbulence in the Earth s atmosphere Peter Haynes, Centre for Atmospheric Science, DAMTP, University of Cambridge. Outline 1. Introduction 2. Momentum transport in the atmosphere 3.
More informationThe general circulation: midlatitude storms
The general circulation: midlatitude storms Motivation for this class Provide understanding basic motions of the atmosphere: Ability to diagnose individual weather systems, and predict how they will change
More informationAgeostrophic instabilities of a front in a stratified rotating fluid
8 ème Congrès Français de Mécanique Grenoble, 27-3 août 27 Ageostrophic instabilities of a front in a stratified rotating fluid J. Gula, R. Plougonven & V. Zeitlin Laboratoire de Météorologie Dynamique
More informationOn the effect of forward shear and reversed shear baroclinic flows for polar low developments. Thor Erik Nordeng Norwegian Meteorological Institute
On the effect of forward shear and reversed shear baroclinic flows for polar low developments Thor Erik Nordeng Norwegian Meteorological Institute Outline Baroclinic growth a) Normal mode solution b) Initial
More informationDynamics of the Extratropical Response to Tropical Heating
Regional and Local Climate Modeling and Analysis Research Group R e L o C l i m Dynamics of the Extratropical Response to Tropical Heating (1) Wegener Center for Climate and Global Change (WegCenter) and
More informationDynamics of the Atmosphere. Large-scale flow with rotation and stratification
12.810 Dynamics of the Atmosphere Large-scale flow with rotation and stratification Visualization of meandering jet stream Upper level winds from June 10th to July 8th 1988 from MERRA Red shows faster
More information1/27/2010. With this method, all filed variables are separated into. from the basic state: Assumptions 1: : the basic state variables must
Lecture 5: Waves in Atmosphere Perturbation Method With this method, all filed variables are separated into two parts: (a) a basic state part and (b) a deviation from the basic state: Perturbation Method
More information8 Mechanisms for tropical rainfall responses to equatorial
8 Mechanisms for tropical rainfall responses to equatorial heating More reading: 1. Hamouda, M. and Kucharski, F. (2019) Ekman pumping Mechanism driving Precipitation anomalies in Response to Equatorial
More informationSEVERE AND UNUSUAL WEATHER
SEVERE AND UNUSUAL WEATHER Basic Meteorological Terminology Adiabatic - Referring to a process without the addition or removal of heat. A temperature change may come about as a result of a change in the
More informationSynoptic-Dynamic Meteorology in Midlatitudes
Synoptic-Dynamic Meteorology in Midlatitudes VOLUME II Observations and Theory of Weather Systems HOWARD B. BLUESTEIN New York Oxford OXFORD UNIVERSITY PRESS 1993 Contents 1. THE BEHAVIOR OF SYNOPTIC-SCALE,
More informationModeling the atmosphere of Jupiter
Modeling the atmosphere of Jupiter Bruce Turkington UMass Amherst Collaborators: Richard S. Ellis (UMass Professor) Andrew Majda (NYU Professor) Mark DiBattista (NYU Postdoc) Kyle Haven (UMass PhD Student)
More information3. Midlatitude Storm Tracks and the North Atlantic Oscillation
3. Midlatitude Storm Tracks and the North Atlantic Oscillation Copyright 2006 Emily Shuckburgh, University of Cambridge. Not to be quoted or reproduced without permission. EFS 3/1 Review of key results
More informationGoals of this Chapter
Waves in the Atmosphere and Oceans Restoring Force Conservation of potential temperature in the presence of positive static stability internal gravity waves Conservation of potential vorticity in the presence
More informationt tendency advection convergence twisting baroclinicity
RELATIVE VORTICITY EQUATION Newton s law in a rotating frame in z-coordinate (frictionless): U + U U = 2Ω U Φ α p U + U U 2 + ( U) U = 2Ω U Φ α p Applying to both sides, and noting ω U and using identities
More information2.5 Shallow water equations, quasigeostrophic filtering, and filtering of inertia-gravity waves
Chapter. The continuous equations φ=gh Φ=gH φ s =gh s Fig..5: Schematic of the shallow water model, a hydrostatic, incompressible fluid with a rigid bottom h s (x,y), a free surface h(x,y,t), and horizontal
More informationThe Effect of Moist Convection on the Tropospheric Response to Tropical and Subtropical Zonally Asymmetric Torques
DECEMBER 2013 B O O S A N D S H A W 4089 The Effect of Moist Convection on the Tropospheric Response to Tropical and Subtropical Zonally Asymmetric Torques WILLIAM R. BOOS Department of Geology and Geophysics,
More informationClouds 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 informationEliassen-Palm Theory
Eliassen-Palm Theory David Painemal MPO611 April 2007 I. Introduction The separation of the flow into its zonal average and the deviations therefrom has been a dominant paradigm for analyses of the general
More informationResonant excitation of trapped coastal waves by free inertia-gravity waves
Resonant excitation of trapped coastal waves by free inertia-gravity waves V. Zeitlin 1 Institut Universitaire de France 2 Laboratory of Dynamical Meteorology, University P. and M. Curie, Paris, France
More informationUsing simplified vorticity equation,* by assumption 1 above: *Metr 430 handout on Circulation and Vorticity. Equations (4) and (5) on that handout
Rossby Wave Equation A. Assumptions 1. Non-divergence 2. Initially, zonal flow, or nearly zonal flow in which u>>v>>w. 3. Initial westerly wind is geostrophic and does not vary along the x-axis and equations
More informationLecture #2 Planetary Wave Models. Charles McLandress (Banff Summer School 7-13 May 2005)
Lecture #2 Planetary Wave Models Charles McLandress (Banff Summer School 7-13 May 2005) 1 Outline of Lecture 1. Observational motivation 2. Forced planetary waves in the stratosphere 3. Traveling planetary
More informationModel equations for planetary and synoptic scale atmospheric motions associated with different background stratification
Model equations for planetary and synoptic scale atmospheric motions associated with different background stratification Stamen Dolaptchiev & Rupert Klein Potsdam Institute for Climate Impact Research
More informationA new theory for moist convection in statistical equilibrium
A new theory for moist convection in statistical equilibrium A. Parodi(1), K. Emanuel(2) (2) CIMA Research Foundation,Savona, Italy (3) EAPS, MIT, Boston, USA True dynamics: turbulent, moist, non-boussinesq,
More informationWind Gyres. curl[τ s τ b ]. (1) We choose the simple, linear bottom stress law derived by linear Ekman theory with constant κ v, viz.
Wind Gyres Here we derive the simplest (and oldest; Stommel, 1948) theory to explain western boundary currents like the Gulf Stream, and then discuss the relation of the theory to more realistic gyres.
More informationIntroduction to Isentropic Coordinates: a new view of mean meridional & eddy circulations. Cristiana Stan
Introduction to Isentropic Coordinates: a new view of mean meridional & eddy circulations Cristiana Stan School and Conference on the General Circulation of the Atmosphere and Oceans: a Modern Perspective
More informationESCI 343 Atmospheric Dynamics II Lesson 11 - Rossby Waves
ESCI 343 Atmospheric Dynamics II Lesson 11 - Rossby Waves Reference: An Introduction to Dynamic Meteorology (4 rd edition), J.R. Holton Atmosphere-Ocean Dynamics, A.E. Gill Fundamentals of Atmospheric
More informationClass exercises Chapter 3. Elementary Applications of the Basic Equations
Class exercises Chapter 3. Elementary Applications of the Basic Equations Section 3.1 Basic Equations in Isobaric Coordinates 3.1 For some (in fact many) applications we assume that the change of the Coriolis
More informationParameterizing large-scale dynamics using the weak temperature gradient approximation
Parameterizing large-scale dynamics using the weak temperature gradient approximation Adam Sobel Columbia University NCAR IMAGe Workshop, Nov. 3 2005 In the tropics, our picture of the dynamics should
More informationNonlinear baroclinic dynamics of surface cyclones crossing a zonal jet
Nonlinear baroclinic dynamics of surface cyclones crossing a zonal jet Jean-Baptiste GILET, Matthieu Plu and Gwendal Rivière CNRM/GAME (Météo-France, CNRS) 3rd THORPEX International Science Symposium Monterey,
More informationGFD II: Balance Dynamics ATM S 542
GFD II: Balance Dynamics ATM S 542 DARGAN M. W. FRIERSON UNIVERSITY OF WASHINGTON, DEPARTMENT OF ATMOSPHERIC SCIENCES WEEK 8 SLIDES Eady Model Growth rates (imaginary part of frequency) Stable for large
More informationThe Shallow Water Equations
If you have not already done so, you are strongly encouraged to read the companion file on the non-divergent barotropic vorticity equation, before proceeding to this shallow water case. We do not repeat
More information196 7 atmospheric oscillations:
196 7 atmospheric oscillations: 7.4 INTERNAL GRAVITY (BUOYANCY) WAVES We now consider the nature of gravity wave propagation in the atmosphere. Atmospheric gravity waves can only exist when the atmosphere
More informationCan a Simple Two-Layer Model Capture the Structure of Easterly Waves?
Can a Simple Two-Layer Model Capture the Structure of Easterly Waves? Cheryl L. Lacotta 1 Introduction Most tropical storms in the Atlantic, and even many in the eastern Pacific, are due to disturbances
More informationSpherical Shallow Water Turbulence: Cyclone-Anticyclone Asymmetry, Potential Vorticity Homogenisation and Jet Formation
Spherical Shallow Water Turbulence: Cyclone-Anticyclone Asymmetry, Potential Vorticity Homogenisation and Jet Formation Jemma Shipton Department of Atmospheric, Oceanic and Planetary Physics, University
More informationScales of Linear Baroclinic Instability and Macroturbulence in Dry Atmospheres
JUNE 2009 M E R L I S A N D S C H N E I D E R 1821 Scales of Linear Baroclinic Instability and Macroturbulence in Dry Atmospheres TIMOTHY M. MERLIS AND TAPIO SCHNEIDER California Institute of Technology,
More informationLARGE SCALE DYNAMICS OF PRECIPITATION FRONTS IN THE TROPICAL ATMOSPHERE: A NOVEL RELAXATION LIMIT
COMM. MATH. SCI. Vol., No., pp. 591 c International Press LARGE SCALE DYNAMICS OF PRECIPITATION FRONTS IN THE TROPICAL ATMOSPHERE: A NOVEL RELAXATION LIMIT DARGAN M. W. FRIERSON, ANDREW J. MAJDA, AND OLIVIER
More informationEquatorial Superrotation on Tidally Locked Exoplanets
Equatorial Superrotation on Tidally Locked Exoplanets Adam P. Showman University of Arizona Lorenzo M. Polvani Columbia University Synopsis Most 3D atmospheric circulation models of tidally locked exoplanets
More informationModeling the General Circulation of the Atmosphere. Topic 2: Tropical General Circulation
Modeling the General Circulation of the Atmosphere. Topic 2: Tropical General Circulation DARGAN M. W. FRIERSON UNIVERSITY OF WASHINGTON, DEPARTMENT OF ATMOSPHERIC SCIENCES 1-28-16 Today What determines
More informationContents. Parti Fundamentals. 1. Introduction. 2. The Coriolis Force. Preface Preface of the First Edition
Foreword Preface Preface of the First Edition xiii xv xvii Parti Fundamentals 1. Introduction 1.1 Objective 3 1.2 Importance of Geophysical Fluid Dynamics 4 1.3 Distinguishing Attributes of Geophysical
More informationSYNOPTIC RESPONSES TO BREAKING MOUNTAIN GRAVITY WAVES MOMENTUM DEPOSIT AT TURNING CRITICAL LEVELS. 2 Model
P. SYNOPTIC RESPONSES TO BREAKING MOUNTAIN GRAVITY WAVES MOMENTUM DEPOSIT AT TURNING CRITICAL LEVELS Armel MARTIN and François LOTT Ecole Normale Superieure, Paris, France Abstract The synoptic scale responses
More informationSymmetric Instability and Rossby Waves
Chapter 8 Symmetric Instability and Rossby Waves We are now in a position to begin investigating more complex disturbances in a rotating, stratified environment. Most of the disturbances of interest are
More informationA Truncated Model for Finite Amplitude Baroclinic Waves in a Channel
A Truncated Model for Finite Amplitude Baroclinic Waves in a Channel Zhiming Kuang 1 Introduction To date, studies of finite amplitude baroclinic waves have been mostly numerical. The numerical models,
More informationModel description of AGCM5 of GFD-Dennou-Club edition. SWAMP project, GFD-Dennou-Club
Model description of AGCM5 of GFD-Dennou-Club edition SWAMP project, GFD-Dennou-Club Mar 01, 2006 AGCM5 of the GFD-DENNOU CLUB edition is a three-dimensional primitive system on a sphere (Swamp Project,
More informationMesoscale Atmospheric Systems. Surface fronts and frontogenesis. 06 March 2018 Heini Wernli. 06 March 2018 H. Wernli 1
Mesoscale Atmospheric Systems Surface fronts and frontogenesis 06 March 2018 Heini Wernli 06 March 2018 H. Wernli 1 Temperature (degc) Frontal passage in Mainz on 26 March 2010 06 March 2018 H. Wernli
More informationBy convention, C > 0 for counterclockwise flow, hence the contour must be counterclockwise.
Chapter 4 4.1 The Circulation Theorem Circulation is a measure of rotation. It is calculated for a closed contour by taking the line integral of the velocity component tangent to the contour evaluated
More informationDynamics of Upper-Level Waves
Dynamics of Upper-Level Waves Atmos 5110 Synoptic Dynamic Meteorology I Instructor: Jim Steenburgh jim.steenburgh@utah.edu 801-581-8727 Suite 480/Office 488 INSCC Suggested reading: Lackman (2011) section
More informationCHAPTER 4. THE HADLEY CIRCULATION 59 smaller than that in midlatitudes. This is illustrated in Fig. 4.2 which shows the departures from zonal symmetry
Chapter 4 THE HADLEY CIRCULATION The early work on the mean meridional circulation of the tropics was motivated by observations of the trade winds. Halley (1686) and Hadley (1735) concluded that the trade
More informationAtmosphere, Ocean and Climate Dynamics Fall 2008
MIT OpenCourseWare http://ocw.mit.edu 12.003 Atmosphere, Ocean and Climate Dynamics Fall 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. Contents
More information8 3D transport formulation
8 3D transport formulation 8.1 The QG case We consider the average (x; y; z; t) of a 3D, QG system 1. The important distinction from the zonal mean case is that the mean now varies with x, or (more generally)
More information( ) = 1005 J kg 1 K 1 ;
Problem Set 3 1. A parcel of water is added to the ocean surface that is denser (heavier) than any of the waters in the ocean. Suppose the parcel sinks to the ocean bottom; estimate the change in temperature
More informationGoverning 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 information4. Atmospheric transport. Daniel J. Jacob, Atmospheric Chemistry, Harvard University, Spring 2017
4. Atmospheric transport Daniel J. Jacob, Atmospheric Chemistry, Harvard University, Spring 2017 Forces in the atmosphere: Gravity g Pressure-gradient ap = ( 1/ ρ ) dp / dx for x-direction (also y, z directions)
More informationIsentropic Analysis. Much of this presentation is due to Jim Moore, SLU
Isentropic Analysis Much of this presentation is due to Jim Moore, SLU Utility of Isentropic Analysis Diagnose and visualize vertical motion - through advection of pressure and system-relative flow Depict
More information2 Transport of heat, momentum and potential vorticity
Transport of heat, momentum and potential vorticity. Conventional mean momentum equation We ll write the inviscid equation of onal motion (we ll here be using log-pressure coordinates with = H ln p=p,
More informationThe general circulation of the atmosphere
Lecture Summer term 2015 The general circulation of the atmosphere Prof. Dr. Volkmar Wirth, Zi. 426, Tel.: 39-22868, vwirth@uni-mainz.de Lecture: 2 Stunden pro Woche Recommended reading Hartmann, D. L.,
More informationNonlinear Balance on an Equatorial Beta Plane
Nonlinear Balance on an Equatorial Beta Plane David J. Raymond Physics Department and Geophysical Research Center New Mexico Tech Socorro, NM 87801 April 26, 2009 Summary Extension of the nonlinear balance
More information7 Balanced Motion. 7.1 Return of the...scale analysis for hydrostatic balance! CSU ATS601 Fall 2015
7 Balanced Motion We previously discussed the concept of balance earlier, in the context of hydrostatic balance. Recall that the balanced condition means no accelerations (balance of forces). That is,
More information2. Meridional atmospheric structure; heat and water transport. Recall that the most primitive equilibrium climate model can be written
2. Meridional atmospheric structure; heat and water transport The equator-to-pole temperature difference DT was stronger during the last glacial maximum, with polar temperatures down by at least twice
More informationPV Generation in the Boundary Layer
1 PV Generation in the Boundary Layer Robert Plant 18th February 2003 (With thanks to S. Belcher) 2 Introduction How does the boundary layer modify the behaviour of weather systems? Often regarded as a
More informationFixed Rossby Waves: Quasigeostrophic Explanations and Conservation of Potential Vorticity
Fixed Rossby Waves: Quasigeostrophic Explanations and Conservation of Potential Vorticity 1. Observed Planetary Wave Patterns After upper air observations became routine, it became easy to produce contour
More informationScience Olympiad Meteorology Quiz #1 Page 1 of 7
1) What is generally true about the stratosphere: a) Has turbulent updrafts and downdrafts. b) Has either a stable or increasing temperature profile with altitude. c) Where the auroras occur. d) Both a)
More informationQ.1 The most abundant gas in the atmosphere among inert gases is (A) Helium (B) Argon (C) Neon (D) Krypton
Q. 1 Q. 9 carry one mark each & Q. 10 Q. 22 carry two marks each. Q.1 The most abundant gas in the atmosphere among inert gases is (A) Helium (B) Argon (C) Neon (D) Krypton Q.2 The pair of variables that
More informationEffective Depth of Ekman Layer.
5.5: Ekman Pumping Effective Depth of Ekman Layer. 2 Effective Depth of Ekman Layer. Defining γ = f/2k, we derived the solution u = u g (1 e γz cos γz) v = u g e γz sin γz corresponding to the Ekman spiral.
More informationCHAPTER 2 - ATMOSPHERIC CIRCULATION & AIR/SEA INTERACTION
Chapter 2 - pg. 1 CHAPTER 2 - ATMOSPHERIC CIRCULATION & AIR/SEA INTERACTION The atmosphere is driven by the variations of solar heating with latitude. The heat is transferred to the air by direct absorption
More informationJet Formation in the Equatorial Oceans Through Barotropic and Inertial Instabilities. Mark Fruman
p. 1/24 Jet Formation in the Equatorial Oceans Through Barotropic and Inertial Instabilities Mark Fruman Bach Lien Hua, Richard Schopp, Marc d Orgeville, Claire Ménesguen LPO IFREMER, Brest, France IAU
More information10 Shallow Water Models
10 Shallow Water Models So far, we have studied the effects due to rotation and stratification in isolation. We then looked at the effects of rotation in a barotropic model, but what about if we add stratification
More informationWave Mean-Flow Interactions in Moist Baroclinic Life Cycles
JULY 2017 Y A M A D A A N D P A U L U I S 2143 Wave Mean-Flow Interactions in Moist Baroclinic Life Cycles RAY YAMADA Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of
More informationPrototype Instabilities
Prototype Instabilities David Randall Introduction Broadly speaking, a growing atmospheric disturbance can draw its kinetic energy from two possible sources: the kinetic and available potential energies
More informationInertial, barotropic and baroclinic instabilities of the Bickley jet in two - layer rotating shallow water model
Inertial, barotropic and baroclinic instabilities of the Bickley jet in two - layer rotating shallow water model François Bouchut Laboratoire d Analyse et de Mathématiques Appliquées, Université Paris-Est/CNRS,
More informationNeeds 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 informationATS 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 informationOn the role of planetary-scale waves in the abrupt seasonal. transition of the Northern Hemisphere general circulation. Tiffany A.
Generated using version 3.2 of the official AMS L A TEX template 1 On the role of planetary-scale waves in the abrupt seasonal 2 transition of the Northern Hemisphere general circulation 3 Tiffany A. Shaw
More informationHurricanes are intense vortical (rotational) storms that develop over the tropical oceans in regions of very warm surface water.
Hurricanes: Observations and Dynamics Houze Section 10.1. Holton Section 9.7. Emanuel, K. A., 1988: Toward a general theory of hurricanes. American Scientist, 76, 371-379 (web link). http://ww2010.atmos.uiuc.edu/(gh)/guides/mtr/hurr/home.rxml
More informationNote that Rossby waves are tranverse waves, that is the particles move perpendicular to the direction of propagation. f up, down (clockwise)
Ocean 423 Rossby waves 1 Rossby waves: Restoring force is the north-south gradient of background potential vorticity (f/h). That gradient can be due to either the variation in f with latitude, or to a
More informationA Uniform PV Framework for Balanced Dynamics
A Uniform PV Framework for Balanced Dynamics vertical structure of the troposphere surface quasigeostrophic models Dave Muraki Simon Fraser University Greg Hakim University of Washington Chris Snyder NCAR
More informationInternal boundary layers in the ocean circulation
Internal boundary layers in the ocean circulation Lecture 9 by Andrew Wells We have so far considered boundary layers adjacent to physical boundaries. However, it is also possible to find boundary layers
More informationTopographic Enhancement of Eddy Efficiency in Baroclinic Equilibration
Topographic Enhancement of Eddy Efficiency in Baroclinic Equilibration JPO, 44 (8), 2107-2126, 2014 by Ryan Abernathey Paola Cessi as told by Navid CASPO theory seminar, 28 May 2016 section 2 what s the
More information7 The General Circulation
7 The General Circulation 7.1 The axisymmetric state At the beginning of the class, we discussed the nonlinear, inviscid, axisymmetric theory of the meridional structure of the atmosphere. The important
More informationVorticity and Potential Vorticity
Chapter 4 Vorticity and Potential Vorticity In this chapter we explore a way of solving the shallow water equations for motions with characteristic time scales longer than the rotation period of the earth.
More informationSUPPLEMENTARY INFORMATION
Figure S1. Summary of the climatic responses to the Gulf Stream. On the offshore flank of the SST front (black dashed curve) of the Gulf Stream (green long arrow), surface wind convergence associated with
More informationEliassen-Palm Cross Sections Edmon et al. (1980)
Eliassen-Palm Cross Sections Edmon et al. (1980) Cecily Keppel November 14 2014 Eliassen-Palm Flux For β-plane Coordinates (y, p) in northward, vertical directions Zonal means F = v u f (y) v θ θ p F will
More informationStability, cyclone-anticyclone asymmetry and frequency selection in rotating shallow-water wakes
Stability, cyclone-anticyclone asymmetry and frequency selection in rotating shallow-water wakes T. Dubos 1, G. Perret 1,2, A. Stegner 1, J.-M. Chomaz 3 and M. Farge 1 1 IPSL/Laboratoire de Meteorologie
More information