Earth s flattening : which impact for meteorology and climatology?
|
|
- Buddy Wade
- 5 years ago
- Views:
Transcription
1 Earth s flattening : which impact for meteorology and climatology? Pierre Bénard Météo-France CNRM/GMAP CNRS Aug. 2014, Montreal P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 1 / 27
2 INTRODUCTION Need of a model of the Earth To write governing equations, one needs (namely): - the shape of the Earth - the shape of Centrifugal forces - the shape of gravity field -... = Hence one needs to first define/choose the assumed shape of the gravity (or geopotential) field P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 2 / 27
3 INTRODUCTION First of all: terminology What is gravity and geopotential, etc., in Meteorology - Gravity : g = the apparent gravity felt by a resting object in the rotating frame (e.g. lying on the floor) - Vertical line = line along apparent gravity (plumb) - Geopotential : g = φ - Horizontal surface = to vertical = iso-geopotential (spirit level) = CONSEQUENCES: - Gravity contains Newtonian and Centrifugal components: g = g N +g C - All surfaces/lines have complicated shapes - Since g = φ, the intensity of gravity is inversely to the vertical separation of geopotentials, locally. P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 3 / 27
4 INTRODUCTION Ω Vertical line ( // to g ) g bigger g smaller Horizontal line ( iso geopotential ) P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 4 / 27
5 INTRODUCTION Currently the model is: Spherical Geopotential Approximation (SGA) - Earth s shape = spherical - All geopotential surfaces = spherical = - Vertical lines are straight radial lines - Vertical separation of geopotentials : uniform - Surface gravity : uniform (g 0 = , some average) Underlying hypothesis This is equivalent to neglect almost all centrifugal effects of earth s rotation P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 5 / 27
6 INTRODUCTION REALITY - Non spherical Earth: Departure best sphere : ±10 km, best ellipsoid : ±100 m Ellipticity ǫ = (a c)/a 0.3% geometrical errors z - Non uniform Gravity : Meridional variations Pole : g P 9.83, Eq. : g E 9.78 Departure mean gravity : ±0.2% gravity errors a 2. a c x P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 6 / 27
7 INTRODUCTION Why relaxing SGA? - Authors claim : systematic and cumulative errors impact on long and climate forecasts? when do they stop to be neglectible? - Also, modelling giant planets atmospheres :... for time being, still considered spherical!! - Thus, it is not useless to prepare and try to evaluate. P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 7 / 27
8 OUTLINE Introduction Consistent Formulations Geometric and gravity errors Estimation of errors in a shallow-water model Estimation of gravity errors in a 3D NWP model Conclusions P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 8 / 27
9 CONSISTENT FORMULATIONS Dynamical Consistency - Definition Definition : Formal respect of conservation principles for axial angular momentum, energy and potential vorticity Dynamically-consistent formulation of gov. equations lead to constraints (cannot write anything which looks good ). Example: bluntly setting g = g(ϕ) in SGA (to better mimic reality) is inconsistent. in SGA, g must be meridionally constant. P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 9 / 27
10 CONSISTENT FORMULATIONS Dynamical Consistency - Theory Big work ( ) mostly UKMO, and also French (LMD, M-F) teams, to better understand non-spherical dynamically-consistent systems Find Governing Equations systems which ensure dynamical consistency (with proofs...) Find appropriate curvilinear coordinate systems for a concretely tractable mathematical description and use. Derivation from Hamiltonian Mechanics formalism helps a lot. Shallow-water, 3D shallow-atmosphere, and 3D deep-atmosphere variants... if interested, look for Staniforth, White, Bénard (Q.J.R. Meteor. Soc), Dubos (JAS), mostly 2014, and refs therein P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 10 / 27
11 CONSISTENT FORMULATIONS Dynamical Consistency - EGA In practice: Ellipsoidal Geopotential Approximation (EGA) instead of SGA all geopotentials are assumed to be ellipsoids (no obvious need to go to actual irregular geoid geometry) EGA allows reasonably tractable equations P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 11 / 27
12 CONSISTENT FORMULATIONS - EGA why reasonably? For families of concentric geopotential ellipsoids respecting the correct ratio g Pole /g Eq = 9.83/9.78, vertical lines have no direct analytical expressions (recall: these lines are simple straight lines in SGA) Spheroidal coordinates (λ,ϕ,r) where r = r(φ) (preferred in order to avoid projection of g on horizontal components). orthogonal horizontal/vertical curvilinear coordinates system. Computation of metrics OK. BUT transformation from Cartesian coordinates non-analytic Requires either polynomial approximation or numerical solution. (not considered as a big problem, though) P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 12 / 27
13 ILLUSTRATION Shallow-Water system in geodetic latitude ϕ, no orog. ( ) du R dt a 2 cosϕ u +2Ω R v sinϕ+ a 2 cosϕ g(ϕ) H λ = 0 ( ) dv R dt + a 2 cosϕ u +2Ω R 3 usinϕ+ a 2 c 2 cosϕ ϕ [g(ϕ)h] = 0 ( dh R dt +H u a 2 cosϕ λ + R 3 v a 2 c 2 cosϕ ϕ Rtanϕ ) a 2 v = 0 where : d dt = t + Ru a 2 cosϕ λ + R3 v a 2 c 2 ϕ R = a 2 cos 2 ϕ+c 2 sin 2 ϕ c a P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 13 / 27
14 OUTLINE Introduction Consistent Formulations Geometric and gravity errors Estimation of errors in a shallow-water model Estimation of gravity errors in a 3D NWP model Conclusions P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 14 / 27
15 Geometric and gravity errors Geometric error - Length of Montreal parallel (45 N) on sphere: km - Length of ACTUAL Montreal parallel (45 N) : km - A pressure low travelling eastward at given V is too fast on sphere... Gravity error - g = 9.806m/s 2 on sphere - g = 9.78 to g = 9.83m/s 2 on actual earth - Propagation of a wave sensitive to gravity will be distorted on sphere... separate evaluation - gravity and geometry errors may be assessed separately by setting only correct geometry or correct gravity (Bénard, 2014, Q. J. Roy. Meteor. Soc.) P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 15 / 27
16 OUTLINE Introduction Consistent Formulations Geometric and gravity errors Estimation of errors in a shallow-water model Estimation of gravity errors in a 3D NWP model Conclusions P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 16 / 27
17 Estimation of errors in a shallow-water model Hauriwtz wave (e.g. Thuburn and Li, 2000, Q. J. R. Meteor. Soc.) - Quasi stationary analytical wave for SW - rotation (eastward), vacillations, becomes instable after 30 days P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 17 / 27
18 Estimation of errors in a shallow-water model Longitude Phase (compared to EGA reference) SGA (total error) gravity error geometry error EGA (ref) P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 18 / 27
19 Estimation of errors in a shallow-water model Standard Real case (from Williamson s test set) 10 days forecast, height field at 250 hpa P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 19 / 27
20 Estimation of errors in a shallow-water model Standard Real case (from Williamson s test set) 10 days forecast, height field at 250 hpa: P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 20 / 27
21 Estimation of errors in a shallow-water model Standard Real case (from Williamson s test set) - Longitude phase shift for some features - modified intensity - modified shape - global RMS after 10 days : about 30 m for Z gravity error still dominates P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 21 / 27
22 OUTLINE Introduction Consistent Formulations Geometric and gravity errors Estimation of errors in a shallow-water model Estimation of gravity errors in a 3D NWP model Conclusions P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 22 / 27
23 Estimation of errors in a 3D NWP model estimation of gravity error only: - spherical planet - shallow-atmosphere approximation - but meridionally-variable gravity ( m/s 2 ) Physically consistent (Bénard, 2014, Q. J. R. Meteor. Soc). Allows spherical geometry (at any level), and variable gravity. P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 23 / 27
24 Estimation of errors in a 3D NWP model Forecast scores against TEMP (Radio-soundings) sample : 2 months (April+May 2014) Contour=0.5m Puzzling results?!? weak significance after 72 h P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 24 / 27
25 Estimation of errors in a 3D NWP model Evaluation against verifying analysis shows: - scores/improvements significant only below 72 h differences/score improvements quite weak - at large forecast times, (larger) potential improvements are buried in (much larger) forecasts errors and become unsignificant P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 25 / 27
26 OUTLINE Introduction Consistent Formulations Geometric and gravity errors Estimation of errors in a shallow-water model Estimation of gravity errors in a 3D NWP model Conclusions P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 26 / 27
27 CONCLUSION Governing Equations are now obtained in various frameworks Allows an estimation of errors in SGA and benefits from EGA Gravity errors seems to slightly dominate 3D shows immediate (but weak) score improvement at short ranges At medium/long range (larger) improvements seem to be buried in (much larger) forecast errors and become not significant. Seemingly no panics with SGA, but reasonably need to prepare the set for future NWP in EGA... P. Bénard (Météo-France) Earth s flattening : which impact? 16/21 Aug 2014, Montreal 27 / 27
( u,v). For simplicity, the density is considered to be a constant, denoted by ρ 0
! Revised Friday, April 19, 2013! 1 Inertial Stability and Instability David Randall Introduction Inertial stability and instability are relevant to the atmosphere and ocean, and also in other contexts
More informationHeight systems. Rüdiger Gens
Rüdiger Gens 2 Outline! Why bother about height systems?! Relevant terms! Coordinate systems! Reference surfaces! Geopotential number! Why bother about height systems?! give a meaning to a value defined
More informationHeight systems. Rudi Gens Alaska Satellite Facility
Rudi Gens Alaska Satellite Facility Outline Why bother about height systems? Relevant terms Coordinate systems Reference surfaces Geopotential number 2 Why bother about height systems? give a meaning to
More informationd v 2 v = d v d t i n where "in" and "rot" denote the inertial (absolute) and rotating frames. Equation of motion F =
Governing equations of fluid dynamics under the influence of Earth rotation (Navier-Stokes Equations in rotating frame) Recap: From kinematic consideration, d v i n d t i n = d v rot d t r o t 2 v rot
More information+ ω = 0, (1) (b) In geometric height coordinates in the rotating frame of the Earth, momentum balance for an inviscid fluid is given by
Problem Sheet 1: Due Thurs 3rd Feb 1. Primitive equations in different coordinate systems (a) Using Lagrangian considerations and starting from an infinitesimal mass element in cartesian coordinates (x,y,z)
More informationEATS Notes 1. Some course material will be online at
EATS 3040-2015 Notes 1 14 Aug 2015 Some course material will be online at http://www.yorku.ca/pat/esse3040/ HH = Holton and Hakim. An Introduction to Dynamic Meteorology, 5th Edition. Most of the images
More informationLecture 2. Lecture 1. Forces on a rotating planet. We will describe the atmosphere and ocean in terms of their:
Lecture 2 Lecture 1 Forces on a rotating planet We will describe the atmosphere and ocean in terms of their: velocity u = (u,v,w) pressure P density ρ temperature T salinity S up For convenience, we will
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 informationControl 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 informationLecture 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 information3 Space curvilinear motion, motion in non-inertial frames
3 Space curvilinear motion, motion in non-inertial frames 3.1 In-class problem A rocket of initial mass m i is fired vertically up from earth and accelerates until its fuel is exhausted. The residual mass
More information1/3/2011. 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 informationThe Hydrostatic Approximation. - Euler Equations in Spherical Coordinates. - The Approximation and the Equations
OUTLINE: The Hydrostatic Approximation - Euler Equations in Spherical Coordinates - The Approximation and the Equations - Critique of Hydrostatic Approximation Inertial Instability - The Phenomenon - The
More informationNOTES AND CORRESPONDENCE. Comments on The Roles of the Horizontal Component of the Earth s Angular Velocity in Nonhydrostatic Linear Models
198 JOURNAL OF THE ATMOSPHERIC SCIENCES NOTES AND CORRESPONDENCE Comments on The Roles of the Horizontal Component of the Earth s Angular elocity in Nonhydrostatic Linear Models DALE R. DURRAN AND CHRISTOPHER
More informationAttractor of a Shallow Water Equations Model
Thai Journal of Mathematics Volume 5(2007) Number 2 : 299 307 www.math.science.cmu.ac.th/thaijournal Attractor of a Shallow Water Equations Model S. Sornsanam and D. Sukawat Abstract : In this research,
More informationDynamic Meteorology - Introduction
Dynamic Meteorology - Introduction Atmospheric dynamics the study of atmospheric motions that are associated with weather and climate We will consider the atmosphere to be a continuous fluid medium, or
More informationExtension of the 1981 Arakawa and Lamb Scheme to Arbitrary Grids
Extension of the 1981 Arakawa and Lamb Scheme to Arbitrary Grids Department of Atmospheric Science Colorado State University May 7th, 2015 Intro Introduction Introduction Key Principles of Numerical Modeling
More informationGEOID UNDULATIONS OF SUDAN USING ORTHOMETRIC HEIGHTS COMPARED WITH THE EGM96 ANG EGM2008
GEOID UNDULATIONS OF SUDAN USING ORTHOMETRIC HEIGHTS COMPARED Dr. Abdelrahim Elgizouli Mohamed Ahmed* WITH THE EGM96 ANG EGM2008 Abstract: Positioning by satellite system determine the normal height above
More informationAssimilation Experiments of One-dimensional Variational Analyses with GPS/MET Refractivity
Assimilation Experiments of One-dimensional Variational Analyses with GPS/MET Refractivity Paul Poli 1,3 and Joanna Joiner 2 1 Joint Center for Earth Systems Technology (JCET), University of Maryland Baltimore
More informationNumerical Investigation on Spherical Harmonic Synthesis and Analysis
Numerical Investigation on Spherical Harmonic Synthesis and Analysis Johnny Bärlund Master of Science Thesis in Geodesy No. 3137 TRITA-GIT EX 15-006 School of Architecture and the Built Environment Royal
More informationOverview of the Numerics of the ECMWF. Atmospheric Forecast Model
Overview of the Numerics of the Atmospheric Forecast Model M. Hortal Seminar 6 Sept 2004 Slide 1 Characteristics of the model Hydrostatic shallow-atmosphere approimation Pressure-based hybrid vertical
More information1/28/16. EGM101 Skills Toolbox. Oblate spheroid. The shape of the earth Co-ordinate systems Map projections. Geoid
EGM101 Skills Toolbox Oblate spheroid The shape of the earth Co-ordinate systems Map projections The geoid is the shape that the surface of the oceans would take under the influence of Earth's gravitation
More informationMountain Torques Caused by Normal-Mode Global Rossby Waves, and the Impact on Atmospheric Angular Momentum
1045 Mountain Torques Caused by Normal-Mode Global Rossby Waves, and the Impact on Atmospheric Angular Momentum HARALD LEJENÄS Department of Meteorology, Stockholm University, Stockholm, Sweden ROLAND
More informationThe Equations of Motion in a Rotating Coordinate System. Chapter 3
The Equations of Motion in a Rotating Coordinate System Chapter 3 Since the earth is rotating about its axis and since it is convenient to adopt a frame of reference fixed in the earth, we need to study
More informationMap projections. Rüdiger Gens
Rüdiger Gens Coordinate systems Geographic coordinates f a: semi-major axis b: semi-minor axis Geographic latitude b Geodetic latitude a f: flattening = (a-b)/a Expresses as a fraction 1/f = about 300
More informationChapter 5. Shallow Water Equations. 5.1 Derivation of shallow water equations
Chapter 5 Shallow Water Equations So far we have concentrated on the dynamics of small-scale disturbances in the atmosphere and ocean with relatively simple background flows. In these analyses we have
More informationA study of the moist Entropy in Meteorology.
Workshop on the Atmospheric Modelling 8-10 February, 2011.Toulouse, France. A study of the moist Entropy in Meteorology. Pascal MARQUET (Météo-France. DPrévi / LABO) Contents 1) Motivations : to study
More informationMeteorology 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 informationDynamics Rotating Tank
Institute for Atmospheric and Climate Science - IACETH Atmospheric Physics Lab Work Dynamics Rotating Tank Large scale flows on different latitudes of the rotating Earth Abstract The large scale atmospheric
More informationLecture 12: Angular Momentum and the Hadley Circulation
Lecture 12: Angular Momentum and the Hadley Circulation September 30, 2003 We learnt last time that there is a planetary radiative drive net warming in the tropics, cooling over the pole which induces
More informationEART164: PLANETARY ATMOSPHERES
EART164: PLANETARY ATMOSPHERES Francis Nimmo Last Week Radiative Transfer Black body radiation, Planck function, Wien s law Absorption, emission, opacity, optical depth Intensity, flux Radiative diffusion,
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 informationChapter 4: Fundamental Forces
Chapter 4: Fundamental Forces Newton s Second Law: F=ma In atmospheric science it is typical to consider the force per unit mass acting on the atmosphere: Force mass = a In order to understand atmospheric
More informationChapter 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 informationOn the Tides' paradox.
On the Tides' paradox. T. De ees - thierrydemees @ pandora.be Abstract In this paper I analyse the paradox of tides, that claims that the oon and not the Sun is responsible for them, although the Sun's
More informationNavigation Mathematics: Kinematics (Earth Surface & Gravity Models) EE 570: Location and Navigation
Lecture Navigation Mathematics: Kinematics (Earth Surface & ) EE 570: Location and Navigation Lecture Notes Update on March 10, 2016 Aly El-Osery and Kevin Wedeward, Electrical Engineering Dept., New Mexico
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 informationOrbital Motion in Schwarzschild Geometry
Physics 4 Lecture 29 Orbital Motion in Schwarzschild Geometry Lecture 29 Physics 4 Classical Mechanics II November 9th, 2007 We have seen, through the study of the weak field solutions of Einstein s equation
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 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 informationSpherical Harmonics and Related Topics. David Randall 2 S = 0, r 2 r r S 2. S = r n Y n
! Revised April 10, 2017 1:32 PM! 1 Spherical Harmonics and Related Topics David Randall The spherical surface harmonics are convenient functions for representing the distribution of geophysical quantities
More informationLast week we obtained a general solution: 1 cos αdv
GRAVITY II Surface Gravity Anomalies Due to Buried Bodies Simple analytical solution may be derived for bodies with uniform density contrast simple shape, such as: Sphere Horizontal/vertical cylinders
More informationThe dynamics of high and low pressure systems
The dynamics of high and low pressure systems Newton s second law for a parcel of air in an inertial coordinate system (a coordinate system in which the coordinate axes do not change direction and are
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 informationThe Mathematics of Maps Lecture 4. Dennis The The Mathematics of Maps Lecture 4 1/29
The Mathematics of Maps Lecture 4 Dennis The The Mathematics of Maps Lecture 4 1/29 Mercator projection Dennis The The Mathematics of Maps Lecture 4 2/29 The Mercator projection (1569) Dennis The The Mathematics
More informationAstronomy 6570 Physics of the Planets
Astronomy 6570 Physics of the Planets Planetary Rotation, Figures, and Gravity Fields Topics to be covered: 1. Rotational distortion & oblateness 2. Gravity field of an oblate planet 3. Free & forced planetary
More informationIntroduction to Geographic Information Science. Updates/News. Last Lecture. Geography 4103 / Map Projections and Coordinate Systems
Geography 4103 / 5103 Introduction to Geographic Information Science Map Projections and Coordinate Systems Updates/News Thursday s lecture Reading discussion 1 find the readings online open questions,
More informationcarroll/notes/ has a lot of good notes on GR and links to other pages. General Relativity Philosophy of general
http://pancake.uchicago.edu/ carroll/notes/ has a lot of good notes on GR and links to other pages. General Relativity Philosophy of general relativity. As with any major theory in physics, GR has been
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 informationAn Optimal Control Problem Formulation for. the Atmospheric Large-Scale Wave Dynamics
pplied Mathematical Sciences, Vol. 9, 5, no. 8, 875-884 HIKRI Ltd, www.m-hikari.com http://dx.doi.org/.988/ams.5.448 n Optimal Control Problem Formulation for the tmospheric Large-Scale Wave Dynamics Sergei
More information9 Rossby Waves. 9.1 Non-divergent barotropic vorticity equation. CSU ATS601 Fall (Holton Chapter 7, Vallis Chapter 5)
9 Rossby Waves (Holton Chapter 7, Vallis Chapter 5) 9.1 Non-divergent barotropic vorticity equation We are now at a point that we can discuss our first fundamental application of the equations of motion:
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 informationg (z) = 1 (1 + z/a) = 1
1.4.2 Gravitational Force g is the gravitational force. It always points towards the center of mass, and it is proportional to the inverse square of the distance above the center of mass: g (z) = GM (a
More informationEE 570: Location and Navigation
EE 570: Location and Navigation Navigation Mathematics: Kinematics (Earth Surface & Gravity Models) Aly El-Osery Kevin Wedeward Electrical Engineering Department, New Mexico Tech Socorro, New Mexico, USA
More informationComparison of ensemble and NMC type of background error statistics for the ALADIN/HU model
Comparison of ensemble and NMC type of background error statistics for the ALADIN/HU model Kristian Horvath horvath@cirus.dhz.hr Croatian Meteorological and Hydrological Service supervised by Bölöni Gergely
More information1/18/2011. 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 informationGEF 1100 Klimasystemet. Chapter 7: Balanced flow
GEF1100 Autumn 2016 27.09.2016 GEF 1100 Klimasystemet Chapter 7: Balanced flow Prof. Dr. Kirstin Krüger (MetOs, UiO) 1 Lecture Outline Ch. 7 Ch. 7 Balanced flow 1. Motivation 2. Geostrophic motion 2.1
More informationIntroduction to Physical Oceanography Homework 3 - Solutions. 1. Volume transport in the Gulf Stream and Antarctic Circumpolar current (ACC):
Laure Zanna 10/17/05 Introduction to Physical Oceanography Homework 3 - Solutions 1. Volume transport in the Gulf Stream and Antarctic Circumpolar current (ACC): (a) Looking on the web you can find a lot
More informationModern Navigation. Thomas Herring
12.215 Modern Navigation Thomas Herring Today s Class Latitude and Longitude Simple spherical definitions Geodetic definition: For an ellipsoid Astronomical definition: Based on direction of gravity Relationships
More informationLecture XIX: Particle motion exterior to a spherical star
Lecture XIX: Particle motion exterior to a spherical star Christopher M. Hirata Caltech M/C 350-7, Pasadena CA 95, USA Dated: January 8, 0 I. OVERVIEW Our next objective is to consider the motion of test
More informationContents. I Introduction 1. Preface. xiii
Contents Preface xiii I Introduction 1 1 Continuous matter 3 1.1 Molecules................................ 4 1.2 The continuum approximation.................... 6 1.3 Newtonian mechanics.........................
More informationGEOGRAPHIC COORDINATE SYSTEMS
GEOGRAPHIC COORDINATE SYSTEMS Introduction to GIS Winter 2015 What is Georeferencing? Used to establish a location on the Earth s surface 1 st order polynomial transformation Georeferencing toolbar What
More informationThe hydrostatic and nonhydrostatic global model IFS/ARPEGE: deep-layer model formulation and testing.
7 The hydrostatic and nonhydrostatic global model IFS/ARPEGE: deep-layer model formulation and testing. Karim Yessad 1 and Nils P. Wedi Research Department 1 Centre National de Recherches Météorologiques,
More informationInfluence of Gravity Waves on the Atmospheric Climate
Influence of Gravity Waves on the Atmospheric Climate François Lott, LMD/CNRS, Ecole Normale Supérieure, Paris flott@lmd.ens.fr 1)Dynamical impact of mountains on atmospheric flows 3)Non-orographic gravity
More informationLecture 1 ATS 601. Thomas Birner, CSU. ATS 601 Lecture 1
Lecture 1 ATS 601 Thomas Birner, CSU About your Instructor: Thomas Birner Assistant Professor, joined CSU 10/2008 M.Sc. Physics (Condensed Matter Theory), U of Leipzig, Germany Ph.D. Atmospheric Science
More informationSymmetry methods in dynamic meteorology
Symmetry methods in dynamic meteorology p. 1/12 Symmetry methods in dynamic meteorology Applications of Computer Algebra 2008 Alexander Bihlo alexander.bihlo@univie.ac.at Department of Meteorology and
More information2. 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 informationTraveling planetary-scale Rossby waves in the winter stratosphere: The role of tropospheric baroclinic instability
GEOPHYSICAL RESEARCH LETTERS, VOL.???, XXXX, DOI:.29/, 1 2 Traveling planetary-scale Rossby waves in the winter stratosphere: The role of tropospheric baroclinic instability Daniela I.V. Domeisen, 1 R.
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 informationMathematical 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 informationDynamics of interacting vortices on trapped Bose-Einstein condensates. Pedro J. Torres University of Granada
Dynamics of interacting vortices on trapped Bose-Einstein condensates Pedro J. Torres University of Granada Joint work with: P.G. Kevrekidis (University of Massachusetts, USA) Ricardo Carretero-González
More information2 General Relativity. 2.1 Curved 2D and 3D space
22 2 General Relativity The general theory of relativity (Einstein 1915) is the theory of gravity. General relativity ( Einstein s theory ) replaced the previous theory of gravity, Newton s theory. The
More informationCONSERVATION LAWS ON THE SPHERE: FROM SHALLOW WATER TO BURGERS. Matania Ben-Artzi
CONSERVATION LAWS ON THE SPHERE: FROM SHALLOW WATER TO BURGERS Matania Ben-Artzi Institute of Mathematics, Hebrew University, Jerusalem, Israel Advances in Applied Mathematics IN MEMORIAM OF PROFESSOR
More informationPotential Theory and the Static Gravity Field of the Earth
TOGP 00054 a0005 3.02 Potential Theory and the Static Gravity Field of the Earth C. Jekeli, The Ohio State University, Columbus, OH, USA ª 2007 Elsevier Ltd. All rights reserved. g0005 g0010 g0015 g0020
More informationChapter 2. The continuous equations
Chapter. The continuous equations Fig. 1.: Schematic of a forecast with slowly varying weather-related variations and superimposed high frequency Lamb waves. Note that even though the forecast of the slow
More informationAn inherently mass-conserving semi-implicit semi-lagrangian discretization of the deep-atmosphere global non-hydrostatic equations
Quarterly Journalof the RoyalMeteorologicalSociety Q. J. R. Meteorol. Soc. : July DOI:./qj. n inherently mass-conserving semi-implicit semi-lagrangian discretization of the deep-atmosphere global non-hydrostatic
More informationDSJRA-55 Product Users Handbook. Climate Prediction Division Global Environment and Marine Department Japan Meteorological Agency July 2017
DSJRA-55 Product Users Handbook Climate Prediction Division Global Environment and Marine Department Japan Meteorological Agency July 2017 Change record Version Date Remarks 1.0 13 July 2017 First version
More informationHEIGHT-LATITUDE STRUCTURE OF PLANETARY WAVES IN THE STRATOSPHERE AND TROPOSPHERE. V. Guryanov, A. Fahrutdinova, S. Yurtaeva
HEIGHT-LATITUDE STRUCTURE OF PLANETARY WAVES IN THE STRATOSPHERE AND TROPOSPHERE INTRODUCTION V. Guryanov, A. Fahrutdinova, S. Yurtaeva Kazan State University, Kazan, Russia When constructing empirical
More informationConservation 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 information1 The satellite altimeter measurement
1 The satellite altimeter measurement In the ideal case, a satellite altimeter measurement is equal to the instantaneous distance between the satellite s geocenter and the ocean surface. However, an altimeter
More informationA mechanistic model study of quasi-stationary wave reflection. D.A. Ortland T.J. Dunkerton NorthWest Research Associates Bellevue WA
A mechanistic model study of quasi-stationary wave reflection D.A. Ortland T.J. Dunkerton ortland@nwra.com NorthWest Research Associates Bellevue WA Quasi-stationary flow Describe in terms of zonal mean
More informationThe atmosphere: A general introduction Niels Woetmann Nielsen Danish Meteorological Institute
The atmosphere: A general introduction Niels Woetmann Nielsen Danish Meteorological Institute Facts about the atmosphere The atmosphere is kept in place on Earth by gravity The Earth-Atmosphere system
More informationMS-GWaves / GWING: Towards UA-ICON A non-hydrostatic global model for studying gravity waves from troposphere to thermosphere
MS-GWaves / GWING: Towards UA-ICON A non-hydrostatic global model for studying gravity waves from troposphere to thermosphere Sebastian Borchert, Günther Zängl, Michael Baldauf (1), Guidi Zhou, Hauke Schmidt,
More informationAstrodynamics (AERO0024)
Astrodynamics (AERO0024) 5. Dominant Perturbations Gaëtan Kerschen Space Structures & Systems Lab (S3L) Motivation Assumption of a two-body system in which the central body acts gravitationally as a point
More informationA5682: Introduction to Cosmology Course Notes. 2. General Relativity
2. General Relativity Reading: Chapter 3 (sections 3.1 and 3.2) Special Relativity Postulates of theory: 1. There is no state of absolute rest. 2. The speed of light in vacuum is constant, independent
More informationNon-hydrostatic sound-proof equations of motion for gravity-dominated compressible fl ows. Thomas Dubos
Non-hydrostatic sound-proof of for gravity-dominated compressible fl ows Thomas Dubos Laboratoire de Météorologie Dynamique/IPSL, École Polytechnique, Palaiseau, France Fabrice Voitus Centre National de
More informationEAS372 Open Book Final Exam 11 April, 2013
EAS372 Open Book Final Exam 11 April, 2013 Professor: J.D. Wilson Time available: 2 hours Value: 30% Please check the Terminology, Equations and Data section before beginning your responses. Answer all
More informationFour ways of inferring the MMC. 1. direct measurement of [v] 2. vorticity balance. 3. total energy balance
Four ways of inferring the MMC 1. direct measurement of [v] 2. vorticity balance 3. total energy balance 4. eliminating time derivatives in governing equations Four ways of inferring the MMC 1. direct
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 informationLecture 4. Coordinate Systems & Projections
Lecture 4 Coordinate Systems & Projections Outline Geodesy Geoids Ellipsoids Geographic Coordinate Systems Magnetic North vs. True North Datums Projections Applying Coordinate Systems and Projections Why
More informationGeneral Relativity I
General Relativity I presented by John T. Whelan The University of Texas at Brownsville whelan@phys.utb.edu LIGO Livingston SURF Lecture 2002 July 5 General Relativity Lectures I. Today (JTW): Special
More informationAspherical Gravitational Field II
Aspherical Gravitational Field II p. 1/19 Aspherical Gravitational Field II Modeling the Space Environment Manuel Ruiz Delgado European Masters in Aeronautics and Space E.T.S.I. Aeronáuticos Universidad
More informationThe Hamiltonian Particle-Mesh Method for the Spherical Shallow Water Equations
The Hamiltonian Particle-Mesh Method for the Spherical Shallow Water Equations Jason Fran CWI P.O. Box 94079, 1090 GB Amsterdam, The Netherlands Sebastian Reich Department of Mathematics, Imperial College
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 informationWaves in Planetary Atmospheres R. L. Walterscheid
Waves in Planetary Atmospheres R. L. Walterscheid 2008 The Aerospace Corporation The Wave Zoo Lighthill, Comm. Pure Appl. Math., 20, 1967 Wave-Deformed Antarctic Vortex Courtesy of VORCORE Project, Vial
More informationTorben Königk Rossby Centre/ SMHI
Fundamentals of Climate Modelling Torben Königk Rossby Centre/ SMHI Outline Introduction Why do we need models? Basic processes Radiation Atmospheric/Oceanic circulation Model basics Resolution Parameterizations
More informationGRACE Gravity Model GGM02
GRACE Gravity Model GGM02 The GGM02S gravity model was estimated with 363 days (spanning April 2002 through December 2003) of GRACE K-band range-rate, attitude, and accelerometer data. No Kaula constraint,
More informationIntegrals in cylindrical, spherical coordinates (Sect. 15.7)
Integrals in clindrical, spherical coordinates (Sect. 15.7 Integration in spherical coordinates. Review: Clindrical coordinates. Spherical coordinates in space. Triple integral in spherical coordinates.
More informationNR402 GIS Applications in Natural Resources Lesson 4 Map Projections
NR402 GIS Applications in Natural Resources Lesson 4 Map Projections From http://www.or.blm.gov/gis/ 1 Geographic coordinates Coordinates are expressed as Latitude and Longitude in Degrees, Minutes, Seconds
More informationBlack Holes. Jan Gutowski. King s College London
Black Holes Jan Gutowski King s College London A Very Brief History John Michell and Pierre Simon de Laplace calculated (1784, 1796) that light emitted radially from a sphere of radius R and mass M would
More information