Lecture Guidelines for GEOF110 Chapter 5 ( 2 hours) Chapter 6 (2 Hours) Ilker Fer Guiding for blackboard presentation. Following Pond & Pickard, Introductory.

Slides:



Advertisements
Similar presentations
ECMWF Governing Equations 1 Slide 1 Governing Equations I by Clive Temperton (room 124) and Nils Wedi (room 128)
Advertisements

Torque, Equilibrium, and Stability
Chapter 14 Fluid Mechanics.
In this presentation you will:
Rotating Earth. Spinning Sphere  A point fixed to the Earth is a non-inertial system.  The surface is nearly spherical. Radius R E = 6.37 x 10 6 m 
Atmospheric Motion ENVI 1400: Lecture 3.
Chapter 8 Coordinate Systems.
AOSS 321, Winter 2009 Earth System Dynamics Lecture 6 & 7 1/27/2009 1/29/2009 Christiane Jablonowski Eric Hetland
PHY 6200 Theoretical Mechanics Chapter 9 Motion in a non-inertial reference frame Prof. Claude A Pruneau Notes compiled by L. Tarini.
1 MECH 221 FLUID MECHANICS (Fall 06/07) Chapter 2: FLUID STATICS Instructor: Professor C. T. HSU.
The Equations of Motion
Hydrostatic Pressure distribution in a static fluid and its effects on solid surfaces and on floating and submerged bodies. Fluid Statics M. Bahrami ENSC.
Hans Burchard Leibniz Institute for Baltic Sea Research Warnemünde Coastal Ocean Dynamics First course: Hydrodynamics.
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.
Spring Topic Outline for Physics 1 Spring 2011.
Force on Floating bodies:
Simple and basic dynamical ideas…..  Newton’s Laws  Pressure and hydrostatic balance  The Coriolis effect  Geostrophic balance  Lagrangian-Eulerian.
Dynamics. Chapter 1 Introduction to Dynamics What is Dynamics? Dynamics is the study of systems in which the motion of the object is changing (accelerating)
Basic dynamics  The equations of motion and continuity Scaling Hydrostatic relation Boussinesq approximation  Geostrophic balance in ocean’s interior.
Chapter 9: Rotational Dynamics
CE 1501 CE 150 Fluid Mechanics G.A. Kallio Dept. of Mechanical Engineering, Mechatronic Engineering & Manufacturing Technology California State University,
Lecture Guidelines for GEOF110 Chapter 2 + Thermodynamics (2 hours) Chapters 3+ 4 (2 hours) Ilker Fer Guiding for blackboard presentation. Following Pond.
Phy 201: General Physics I Chapter 5: Uniform Circular Motion Lecture Notes.
Equations that allow a quantitative look at the OCEAN
Momentum Equations in a Fluid (PD) Pressure difference (Co) Coriolis Force (Fr) Friction Total Force acting on a body = mass times its acceleration (W)
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS FILTERING OF EQUATIONS OF MOTION FOR ATMOSPHERE (CONT) LECTURE 7 (Reference: Peixoto & Oort, Chapter 3,7)
Section 5.4 Gravity Waves. Gravity Waves Gravity acts as the restoring force on parcels displaced from hydrostatic equilibrium. Pure gravity exists when.
6.2 Gravitational field and gravitational field strength
1© Manhattan Press (H.K.) Ltd. 1.7 Stability 2 © Manhattan Press (H.K.) Ltd. Stability 1.7 Stability (SB p. 75) What makes objects more stable than others?
Physical Oceanography SACS/AAPT Spring Meeting March 29, 2003 Coastal Carolina University.
1 Equations of Motion Buoyancy Ekman and Inertial Motion September 17.
Physics 111: Mechanics Lecture 4
Sect. 4.10: Coriolis & Centrifugal Forces (Motion Relative to Earth, mainly from Marion)
Basic dynamics ●The equations of motion and continuity Scaling
Atmospheric Motion SOEE1400: Lecture 7. Plan of lecture 1.Forces on the air 2.Pressure gradient force 3.Coriolis force 4.Geostrophic wind 5.Effects of.
ATM OCN 100 Summer ATM OCN 100 – Summer 2002 LECTURE 18 (con’t.) THE THEORY OF WINDS: PART II - FUNDAMENTAL FORCES A. INTRODUCTION B. EXPLANATION.
OCN 5401 Chapter 5 Equations of Motion Instructor: Dr. George A. Maul / X 7453.
200 Physics Concepts from Delores Gende Website
Ship Computer Aided Design Displacement and Weight.
Conservation of Salt: Conservation of Heat: Equation of State: Conservation of Mass or Continuity: Equations that allow a quantitative look at the OCEAN.
Circular Motion and Other Applications of Newton’s Laws
Definitions in-situ density anomaly: σs,t,p = ρ – 1000 kg/m3
Basic dynamics ●The equations of motion and continuity Scaling Hydrostatic relation Boussinesq approximation ●Geostrophic balance in ocean’s interior.
Basic dynamics The equation of motion Scale Analysis
Guidelines for GEOF110: Lecture 1. Relevant Mathematical Review (2 hours) Ilker Fer Guiding for blackboard presentation. Following Pond & Pickard, Introductory.
Scales of Motion, Reynolds averaging September 22.
Potential temperature In situ temperature is not a conservative property in the ocean. Changes in pressure do work on a fluid parcel and changes its internal.
 p and  surfaces are parallel =>  =  (p) Given a barotropic and hydrostatic conditions, is geostrophic current. For a barotropic flow, we have and.
Lecture Guidelines for GEOF110 Chapter 7 Until Re-averaging + movie = 2 h scaling/ hydrostatic equation = 2 h Ilker Fer Guiding for blackboard presentation.
1 Equations of Motion September 15 Part Continuum Hypothesis  Assume that macroscopic behavior of fluid is same as if it were perfectly continuous.
ATM OCN Fall ATM OCN Fall 1999 LECTURE 17 THE THEORY OF WINDS: PART II - FUNDAMENTAL FORCES A. INTRODUCTION –How do winds originate? –What.
Dynamics  Dynamics deals with forces, accelerations and motions produced on objects by these forces.  Newton’s Laws l First Law of Motion: Every body.
Sverdrup, Stommel, and Munk Theories of the Gulf Stream
Inertial & Non-Inertial Frames
Introduction to Fluid Mechanics
Ch 8 : Rotational Motion .
College Physics, 7th Edition
For a barotropic flow, we have is geostrophic current.
Dynamical Balance in the Earth’s Atmosphere
ATOC 4720 class31 1. Coordinate systems 2. Forces.
ATOC 4720 class32 1. Forces 2. The horizontal equation of motion.
Hydrostatics Dp Dz Air Parcel g.
Chapter 7 Equations of Motion
Chapter 7 Equations of Motion
Fluid statics Hydrostatics or Fluid Statics is the study of fluids at rest. It's practical applications are numerous. Some of which are Fluid Manometers,
Chapter 7 Equations of Motion
Chapter 14 Fluid Mechanics.
Announcements Homeworks 1-5:
AOSS 401, Fall 2013 Lecture 3 Coriolis Force September 10, 2013
Presentation transcript:

Lecture Guidelines for GEOF110 Chapter 5 ( 2 hours) Chapter 6 (2 Hours) Ilker Fer Guiding for blackboard presentation. Following Pond & Pickard, Introductory Dynamical Oceanography

GEOF110 Guidelines / 3 2 Static Stability Atmosphere Ocean   Sketch: Incompressible fluid. Parcel 0 is in hydrostatic equilibrium. Atmosphere: Ocean: “Parcel” or “particle” : we mean a (infinitesimal) fluid sample of uniform T and composition in a continuous environment

GEOF110 Guidelines / 3 3 Level 1 z Level 2 z+  z PARCEL (P) ENVIRONMENT (W) Parcel at level 1 is displaced to level 2 with environment in situ properties given on the figure. At level 2, the restoring force on the parcel with volume  V is: F= buoyant upthrust – weight Archimedes: Buoyant upthrust = weight of displaced volume (=g  2  V)

GEOF110 Guidelines / 3 4

5 E > 0 : STABLEparcel displaced vertically will tend to return to its position. Due to its inertia, overshoot equilibrium position  oscillate (with frequency N) E = 0 : NEUTRALvertically displaced parcel will remain there E < 0 : UNSTABLEoverturning

GEOF110 Guidelines / 3 6 In the upper 1 km of ocean E range between x /m, largest values at the pycnocline, in the upper a few 100 m. In deep ocean, deep trenches, E is close to 1x /m. i.e., in situ T increases about (0.1 – 0.2) K / km This is OK using eq. of state and an accurate relation for C. Use of in-situ density would look very stably stratified in neutral stability: compensates for compressibility These are comparable

GEOF110 Guidelines / 3 7 This is not very convenient, nor practical (e.g.  /  S taken while holding in situ values of T and P).

GEOF110 Guidelines / 3 8 NOTE: In a stable environment, an inviscid fluid parcel displaced a small distance  vertically will go through simple harmonic oscillations described by

GEOF110 Guidelines / 3 9 Double Diffusion Double-diffusion occurs when the density variations are caused by two different components with different rates of diffusion. In seawater heat and salt have different molecular rates of diffusion: K H / K S  100 z TS TS Salt Finger Double-Diffusive Convection Recall- diffusion and mixing is from high concentration of stuff to low concentration, i.e. downgradient. Double-Diffusion gives UPGRADIENT density flux.

GEOF110 Guidelines / 3 10 Equation of Motion (Ch. 6) Acceleration due to resultant force acting per unit mass Forces: Pressure Coriolis Gravity (gravitational acceleration, g f ) Other (e.g., tidal, friction) Will derive the terms, and then give the complete equation

GEOF110 Guidelines / 3 11 Pressure force on a surface element δA with outward normal vector n: i.e., directed towards the surface element. Derivation of the Pressure Term (Pressure Gradient Force) The net force δF p in the x-direction: Using δm =  δV = 1/  δV  Using all 3-D:

GEOF110 Guidelines / 3 12 Source: J.H.E.Weber

GEOF110 Guidelines / 3 13 Source: J.H.E.Weber

GEOF110 Guidelines / 3 14

GEOF110 Guidelines / 3 15 Eq. of motion relative to fixed axes: Eq. of motion relative to rotating Earth: For our use: Absolute frames is fixed  subscript f Relative frames is Earth  subscript e No translation of Earth  a o = 0 velocity relative to Earth  v  = 2  radians per sidereal day = 7.292x10 -5 radians/s Conversion from fixed to Earth frames: r = Distance to the centre of Earth

GEOF110 Guidelines / 3 16 Gravitation and Gravity m1m1 m2m2 r, directed along the line connecting masses. G : Gravitational constant Gravitation is the attractive force between two masses:  Equator  In our case, mass of Earth, m E. Gravitational force on body m, per unit mass: Centripetal acceleration : to move a body at distance r from the center of Earth to circulate about Earth’s axis with . Acceleration due to gravity: Note, g does not point to Earth’s center of mass due to centripetal acc.  Equatorial bulge.  Earth’s surface not spherical g=f(latitude) Max at poles Min. near eq. Variation about 0.5%  Assume g = 9.8 m/s 2

GEOF110 Guidelines / 3 17 Equation of motion Pressure Gravity Coriolis Other forces/m For convenience, move the coordinate to Earth’s surface. In Cartesian:

GEOF110 Guidelines / 3 18 Coordinate Systems Cartesian Coordinate System: The standard convention in geophysical fluid mechanics is x is to the east, y is to the north, and z is up. f-Plane is a Cartesian coordinate system in which the Coriolis parameter is assumed constant. It is useful for describing flow in regions small compared with the radius of the Earth (up to 100 km). β-plane is a Cartesian coordinate system in which the Coriolis force is assumed to vary linearly with latitude. It is useful for describing flow over areas as large as ocean basins. Spherical coordinates are used to describe flows that extend over large distances and in numerical calculations of basin and global scale flows.