Sect. 4.10: Coriolis & Centrifugal Forces (Motion Relative to Earth, mainly from Marion)

Slides:



Advertisements
Similar presentations
Factors Affecting Wind
Advertisements

Physics 430: Lecture 21 Rotating Non-Inertial Frames
What Makes the Wind Blow?
Air Pressure and Winds III
Fronts and Coriolis. Fronts Fronts - boundaries between air masses of different temperature. –If warm air is moving toward cold air, it is a “warm front”.
Winds and Ocean Currents. Latent Heat Transport 580 cal/g Surface wind Surface wind.
Example (Marion) Acceleration in the rotating
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 5 Force and Motion (I) Kinematics vs Dynamics.
Natural Environments: The Atmosphere
Chapter 10: Atmospheric Dynamics
What Makes the Wind Blow? ATS 351 Lecture 8 October 26, 2009.
Kinematics of Uniform Circular Motion Do you remember the equations of kinematics? There are analogous equations for rotational quantities. You will see.
AOSS 321, Winter 2009 Earth System Dynamics Lecture 6 & 7 1/27/2009 1/29/2009 Christiane Jablonowski Eric Hetland
Circular Motion and Other Applications of Newton’s Laws
PHY 6200 Theoretical Mechanics Chapter 9 Motion in a non-inertial reference frame Prof. Claude A Pruneau Notes compiled by L. Tarini.
Atmospheric Circulation
Uniform and non-uniform circular motion Centripetal acceleration Problem solving with Newton’s 2nd Law for circular motion Lecture 8: Circular motion.
The Coriolis Force and Weather By Jing Jin February 23, 2006.
AOSS 321, Winter 2009 Earth System Dynamics Lecture 8 2/3/2009 Christiane Jablonowski Eric Hetland
Chapter 8 Wind and Weather. Wind –The local motion of air relative to the rotating Earth Wind is measured using 2 characteristics –Direction (wind sock)
Warning! In this unit, we switch from thinking in 1-D to 3-D on a rotating sphere Intuition from daily life doesn’t work nearly as well for this material!
Physics 430: Lecture 20 Non-Inertial Frames
Circular Motion and Other Applications of Newton’s Laws
Atmospheric Force Balances
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.
Ch. 6 FORCE AND MOTION  II 6.1 Newton’s Law in Non-inertial Reference Frames 6.1.1Inertial force in linear acceleration reference frame From the view.
Simple and basic dynamical ideas…..  Newton’s Laws  Pressure and hydrostatic balance  The Coriolis effect  Geostrophic balance  Lagrangian-Eulerian.
Atmospheric Motions & Climate
Angular Momentum; General Rotation
Guided Notes for Weather Systems
Physics 3210 Week 9 clicker questions. Exam 2 scores Median=45 Standard deviation=22.
Chapter 6 Circular Motion and Other Applications of Newton’s Laws.
Planetary Atmospheres, the Environment and Life (ExCos2Y) Topic 6: Wind Chris Parkes Rm 455 Kelvin Building.
Chapter 6 Atmospheric Forces and Wind
Rotating Coordinate Systems For Translating Systems: We just got Newton’s 2 nd Law (in the accelerated frame): ma = F where F = F - ma 0 ma 0  A non-inertial.
Physical Oceanography SACS/AAPT Spring Meeting March 29, 2003 Coastal Carolina University.
Chapter 6: Air Pressure and Winds Atmospheric pressure Atmospheric pressure Measuring air pressure Measuring air pressure Surface and upper-air charts.
Atmospheric Circulation Patterns Unit 2 Section 6
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.
WIND Movement of air in the atmosphere.. Remember Convection Principles Solar energy strikes the _____________________, heating the air, land and water.
Conservation of Salt: Conservation of Heat: Equation of State: Conservation of Mass or Continuity: Equations that allow a quantitative look at the OCEAN.
Sect. 6-3: Gravity Near Earth’s Surface. g & The Gravitational Constant G.
Lecture 7 Forces (gravity, pressure gradient force)
2006: Assoc. Prof. R. J. Reeves Gravitation 2.1 P113 Gravitation: Lecture 2 Gravitation near the earth Principle of Equivalence Gravitational Potential.
Sect. 4.9: Rate of Change of a Vector Use the concept of an infinitesimal rotation to describe the time dependence of rigid body motion. An arbitrary.
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.
Global air circulation Mr Askew. Pressure gradient, Coriolis force and Geostrophic flow  Wind is produced by different air pressure between places. 
Air Pressure and Winds II. RECAP Ideal gas law: how the pressure, the temperature and the density of an ideal gas relay to each other. Pressure and pressure.
Dynamics  Dynamics deals with forces, accelerations and motions produced on objects by these forces.  Newton’s Laws l First Law of Motion: Every body.
9/2/2015PHY 711 Fall Lecture 41 PHY 711 Classical Mechanics and Mathematical Methods 10-10:50 AM MWF Olin 103 Plan for Lecture 4: Chapter 2 – Physics.
Warm-Up What is the device used for mearsuring air pressure called?
Inertial & Non-Inertial Frames
Inertial & Non-Inertial Frames
The Coriolis Force QMUL Interview 7th July 2016.
Global Winds.
Section 8.3 Equilibrium Define center of mass.
Chapter 6: Air Pressure and Winds
PLANETARY WIND SYSTEM.
Pressure Centers and Winds
The Transfer of Heat Outcomes:
19.2 Pressure Centers and Winds
In the Northern Hemisphere
Weather Notes Part 3.
Announcements Homeworks 1-5:
Isobars and wind barbs sea level pressure.
Physics 319 Classical Mechanics
Presentation transcript:

Sect. 4.10: Coriolis & Centrifugal Forces (Motion Relative to Earth, mainly from Marion) Summary: For motion in an accelerating frame (r), both translating & rotating with respect to a fixed (f, inertial) frame: Velocities: vf = V + vr + ω  r Accelerations: ar = Af + ar + ω  r + ω  (ω  r) + 2(ω  vr)  Newton’s 2nd Law (inertial frame): F = maf = mAf + mar + m(ω  r) + m[ω  (ω  r)] + 2m(ω  vr)  “2nd Law” equation in the moving frame: mar  Feff  F - mAf - m(ω  r) - m[ω  (ω  r)] - 2m(ω  vr)

Motion Relative to Earth  “2nd Law” in accelerating frame: Feff  mar  F - mAf - m(ω  r) - m[ω  (ω  r)] - 2m(ω  vr)  Transformation gave: Feff  F - (non-inertial terms) Interpretations: - mAf : From translational acceleration of moving frame. - m(ω  r): From angular acceleration of moving frame. - m[ω  (ω  r)]:  “Centrifugal Force”. If ω  r: Has magnitude mω2r. Outwardly directed from center of rotation. - 2m(ω  vr):  “Coriolis Force”. From motion of particle in moving system (= 0 if vr = 0) More discussion of last two now!  ≈ 0 for motion near Earth

ω2Re = 3.38 cm/s2 = Centripetal acceleration at equator Motion of Earth relative to inertial frame: Rotation on axis causes small effects! However, this dominates over other (much smaller!) effects: ω = 7.292  10-5 s-1 ; ω2Re = 3.38 cm/s2 = Centripetal acceleration at equator 2ωvr  1.5  10-4 v = max Coriolis acceleration ( 15 cm/s2 = 0.015g for v = 105 cm/s) Even Smaller effects! Revolution about Sun Motion of Solar System in Galaxy Motion of Galaxy in Universe Also, ω = (dω/dt) ≈ 0

Coordinate systems (figure): z direction = local vertical Fixed: (x,y,z) At Earth center Moving: (x,y,z) On Earth surface

Mass m at r in moving system. Physical forces in inertial system: F  S + mg0 S  Sum of non-gravitational forces mg0  Gravitational force on m g0  Gravitational field vector, vertical (towards Earth center; along R in fig). From Newton’s Gravitation Law: g0 = -[(GME)eR]/(R2) G  Gravitational constant, R  Earth radius ME  Earth mass, eR  Unit vector in R direction Assumes isotropic, spherical Earth Neglects gravitational variations due to oblateness; non-uniformity; ...

ez  unit vector along z Effective force on m, measured in moving system is thus: Feff  S + mg0 - mAf - m(ω  r) - m[ω  (ω  r)] - 2m(ω  vr) Earth’s angular velocity ω is in z direction in inertial system (North): ω  ωez ez  unit vector along z Earth rotation period T = 1 day ω = (2π)/T = 7.3  10-5 rad/s (Note: ω  365 ωes) ω  constant  ω  0  Neglect m(ω  r) Consider mAf term in Feff & use again formalism of last time (rotation instead of translation): Af = (ω  Vf ) = [ω  (ω  R)]

Effective force on m is:  Feff  S+mg0 - (mω)  [ω  (r + R)] - 2m(ω  vr) Rewrite as: Feff  S + mg - 2m(ω  vr) Where, mg  Effective Weight g  Effective gravitational field (= measured gravitational acceleration, g on Earth surface!) g  g0 - ω  [ω  (r + R)] Considering motion of mass m, at point r near Earth surface. R = |R| = Earth radius.  |r| << |R|  ω  [ω  (r + R)]  ω  (ω  R)  Effective g near Earth surface: g  g0 - ω  (ω  R)

g = g0 - ω  [ω  (r + R)] Centrifugal force: If m is at point r far from Earth surface, must consider both R & r terms. Effective g for any r: g = g0 - ω  [ω  (r + R)] Second term = Centrifugal force per unit mass (Centrifugal acceleration). Centrifugal force: Causes Earth oblateness (g0 neglects). Goldstein discussion, p 176 Earth  Solid sphere. Earth  Viscous fluid with solid crust. Rotation  “fluid” deforms,  Requator - Rpole  21.4 km gpole - gequator  0.052 m/s2 Surface of calm ocean water is  g instead of g0. Deviation of g from local vertical direction!

Summary: Effective force: Feff = S + mg - 2m(ω  vr) (1) Where, g = g0 - ω  [ω  (r + R)] (2) Often, g  g0 - ω  (ω  R) (3) These are all we need for motion near the Earth!

Direction of g Consider: g = g0 - (ω)  [ω  (r + R)] (2) Effective g = Eqtn (2). Consider experiments. Magnitude of g: Determined by measuring the period of a pendulum (small θ). DIRECTION of g: Determined by the direction of a “plumb bob” in equilibrium. Magnitude of 2nd term in (2): ω2R  0.034 m/s2  (ω2R)/(g0)  0.35% Direction of 2nd term in (2): Outward from the axis of the rotating Earth. Direction of g = Direction of plumb bob = Direction of the vector sum in (2). Slightly different from the “true” vertical  line to the Earth’s center. (Figure next page!)

Direction of plumb bob = Direction of g = g0 - (ω)  [ω  (r + R)] (2) Figure: (r in figure = r in previous figures!) Deviation of g from g0 direction is exaggerated! r = R + z where z = altitude

Coriolis Effects Effective force on m near Earth: Feff = S + mg - 2m(ω  vr) - 2m(ω  vr) = Coriolis force. Obviously, = 0 unless m moves in the rotating frame (moving with respect to Earth’s surface) with velocity vr. Figure again:

- 2m(ω  vr) = Coriolis force. Northern Hemisphere: Earth’s angular velocity ω is in z direction in inertial system (North) ω  ωez ez  unit vector along z (Figures):  In general, ω has components along x, y, z axes of the rotating system. All can have effects, depending on the direction of vr. Most dominant is ω component which is locally vertical in rotating system, that is ωz  Component along local vertical.

- 2m(ω  vr) = Coriolis force, Northern hemisphere. Consider ωz only for now. Particle moving in locally horizontal plane (at Earth surface): vr has no vertical component.  Coriolis force has horizontal component only, magnitude = 2mωzvr & direction to right of particle motion (figure).  Particle is deflected to right of the original direction:

Magnitude of (locally) horizontal component of Coriolis force  ωz = (locally) vertical component of ω  (Local) vertical component of ω depends on latitude! Easily shown: ωz = ω sin(λ), λ = latitude angle (figure).  ωz = 0, λ =0 (equator); ωz = ω, λ = 90 (N. pole)  Horizontal component of Coriolis force, magnitude = 2m ωzvr depends on latitude! 2mωzvr = 2mωvrsin(λ) All of this the in N. hemisphere! S. Hemisphere: Vertical component ωz is directed inward along the local vertical.  Coriolis force & direction of deflections are opposite of N. hemisphere (left of the direction of velocity vr )

Coriolis Deflections: Noticeable effects on: Flowing water (whirlpools) Air masses  Weather. Air flows from high pressure (HP) to low pressure (LP) regions. Coriolis force deflects it. Produces cyclonic motion. N. Hemisphere: Right deflection: Air rotates with HP on right, LP on left. HP prevents (weak) Coriolis force from deflecting air further to right.  Counterclockwise air flow! S. Hemisphere: Left deflection. (Falkland Islands story) Bathtub drains!

More Coriolis Effects on the Weather: Temperate regions: Airflow is not along pressure isobars due to the Coriolis force (+ the centrifugal force due to rotating air mass). Equatorial regions: Sun heating the Earth causes hot surface air to rise (vr has a vertical component).  In Coriolis force need to account ALSO for (local) horizontal components of ω Northern hemisphere: Results in cooler air moving South towards equator, giving vr a horizontal component . Then, horizontal component of Coriolis force deflects South moving air to right (West) Trade winds in N. hemisphere are Southwesterly. Southern hemisphere: The opposite! No trade winds at equator because Coriolis force = 0 there All is idealization, of course, but qualitatively correct!