Balanced Flow
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Balanced Dynamics in Rotating, Stratified Flows
Balanced Dynamics in Rotating, Stratified Flows: An IPAM Tutorial Lecture James C. McWilliams Atmospheric and Oceanic Sciences, UCLA tutorial (n) 1. schooling on a topic of common knowledge. 2. opinion offered with incomplete proof or illustration. These are notes for a lecture intended to introduce a primarily mathematical audience to the idea of balanced dynamics in geophysical fluids, specifically in relation to climate modeling. A more formal presentation of some of this material is in McWilliams (2003). 1 A Fluid Dynamical Hierarchy The vast majority of the kinetic and available potential energy in the general circulation of the ocean and atmosphere, hence in climate, is constrained by approximately “balanced” forces, i.e., geostrophy in the horizontal plane (Coriolis force vs. pressure gradient) and hydrostacy in the vertical direction (gravitational buoyancy force vs. pressure gradient), with the various external and phase-change forces, molecular viscosity and diffusion, and parcel accelerations acting as small residuals in the momentum balance. This lecture is about the theoretical framework associated with this type of diagnostic force balance. Parametric measures of dynamical influence of rotation and stratification are the Rossby and Froude numbers, V V Ro = and F r = : (1) fL NH V is a characteristic horizontal velocity magnitude, f = 2Ω is Coriolis frequency (Ω is Earth’s rotation rate), N is buoyancy frequency for the stable density stratification, and (L; H) are (hor- izontal, vertical) length scales. For flows on the planetary scale and mesoscale, Ro and F r are typically not large. Furthermore, since for these flows the atmosphere and ocean are relatively thin, the aspect ratio, H λ = ; (2) L is small. -
The Swinging Spring: Regular and Chaotic Motion
References The Swinging Spring: Regular and Chaotic Motion Leah Ganis May 30th, 2013 Leah Ganis The Swinging Spring: Regular and Chaotic Motion References Outline of Talk I Introduction to Problem I The Basics: Hamiltonian, Equations of Motion, Fixed Points, Stability I Linear Modes I The Progressing Ellipse and Other Regular Motions I Chaotic Motion I References Leah Ganis The Swinging Spring: Regular and Chaotic Motion References Introduction The swinging spring, or elastic pendulum, is a simple mechanical system in which many different types of motion can occur. The system is comprised of a heavy mass, attached to an essentially massless spring which does not deform. The system moves under the force of gravity and in accordance with Hooke's Law. z y r φ x k m Leah Ganis The Swinging Spring: Regular and Chaotic Motion References The Basics We can write down the equations of motion by finding the Lagrangian of the system and using the Euler-Lagrange equations. The Lagrangian, L is given by L = T − V where T is the kinetic energy of the system and V is the potential energy. Leah Ganis The Swinging Spring: Regular and Chaotic Motion References The Basics In Cartesian coordinates, the kinetic energy is given by the following: 1 T = m(_x2 +y _ 2 +z _2) 2 and the potential is given by the sum of gravitational potential and the spring potential: 1 V = mgz + k(r − l )2 2 0 where m is the mass, g is the gravitational constant, k the spring constant, r the stretched length of the spring (px2 + y 2 + z2), and l0 the unstretched length of the spring. -
Symmetric Instability in the Gulf Stream
Symmetric instability in the Gulf Stream a, b c d Leif N. Thomas ⇤, John R. Taylor ,Ra↵aeleFerrari, Terrence M. Joyce aDepartment of Environmental Earth System Science,Stanford University bDepartment of Applied Mathematics and Theoretical Physics, University of Cambridge cEarth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology dDepartment of Physical Oceanography, Woods Hole Institution of Oceanography Abstract Analyses of wintertime surveys of the Gulf Stream (GS) conducted as part of the CLIvar MOde water Dynamic Experiment (CLIMODE) reveal that water with negative potential vorticity (PV) is commonly found within the surface boundary layer (SBL) of the current. The lowest values of PV are found within the North Wall of the GS on the isopycnal layer occupied by Eighteen Degree Water, suggesting that processes within the GS may con- tribute to the formation of this low-PV water mass. In spite of large heat loss, the generation of negative PV was primarily attributable to cross-front advection of dense water over light by Ekman flow driven by winds with a down-front component. Beneath a critical depth, the SBL was stably strat- ified yet the PV remained negative due to the strong baroclinicity of the current, suggesting that the flow was symmetrically unstable. A large eddy simulation configured with forcing and flow parameters based on the obser- vations confirms that the observed structure of the SBL is consistent with the dynamics of symmetric instability (SI) forced by wind and surface cooling. The simulation shows that both strong turbulence and vertical gradients in density, momentum, and tracers coexist in the SBL of symmetrically unstable fronts. -
Dynamics of the Elastic Pendulum Qisong Xiao; Shenghao Xia ; Corey Zammit; Nirantha Balagopal; Zijun Li Agenda
Dynamics of the Elastic Pendulum Qisong Xiao; Shenghao Xia ; Corey Zammit; Nirantha Balagopal; Zijun Li Agenda • Introduction to the elastic pendulum problem • Derivations of the equations of motion • Real-life examples of an elastic pendulum • Trivial cases & equilibrium states • MATLAB models The Elastic Problem (Simple Harmonic Motion) 푑2푥 푑2푥 푘 • 퐹 = 푚 = −푘푥 = − 푥 푛푒푡 푑푡2 푑푡2 푚 • Solve this differential equation to find 푥 푡 = 푐1 cos 휔푡 + 푐2 sin 휔푡 = 퐴푐표푠(휔푡 − 휑) • With velocity and acceleration 푣 푡 = −퐴휔 sin 휔푡 + 휑 푎 푡 = −퐴휔2cos(휔푡 + 휑) • Total energy of the system 퐸 = 퐾 푡 + 푈 푡 1 1 1 = 푚푣푡2 + 푘푥2 = 푘퐴2 2 2 2 The Pendulum Problem (with some assumptions) • With position vector of point mass 푥 = 푙 푠푖푛휃푖 − 푐표푠휃푗 , define 푟 such that 푥 = 푙푟 and 휃 = 푐표푠휃푖 + 푠푖푛휃푗 • Find the first and second derivatives of the position vector: 푑푥 푑휃 = 푙 휃 푑푡 푑푡 2 푑2푥 푑2휃 푑휃 = 푙 휃 − 푙 푟 푑푡2 푑푡2 푑푡 • From Newton’s Law, (neglecting frictional force) 푑2푥 푚 = 퐹 + 퐹 푑푡2 푔 푡 The Pendulum Problem (with some assumptions) Defining force of gravity as 퐹푔 = −푚푔푗 = 푚푔푐표푠휃푟 − 푚푔푠푖푛휃휃 and tension of the string as 퐹푡 = −푇푟 : 2 푑휃 −푚푙 = 푚푔푐표푠휃 − 푇 푑푡 푑2휃 푚푙 = −푚푔푠푖푛휃 푑푡2 Define 휔0 = 푔/푙 to find the solution: 푑2휃 푔 = − 푠푖푛휃 = −휔2푠푖푛휃 푑푡2 푙 0 Derivation of Equations of Motion • m = pendulum mass • mspring = spring mass • l = unstreatched spring length • k = spring constant • g = acceleration due to gravity • Ft = pre-tension of spring 푚푔−퐹 • r = static spring stretch, 푟 = 푡 s 푠 푘 • rd = dynamic spring stretch • r = total spring stretch 푟푠 + 푟푑 Derivation of Equations of Motion -
Balanced Flow Natural Coordinates
Balanced Flow • The pressure and velocity distributions in atmospheric systems are related by relatively simple, approximate force balances. • We can gain a qualitative understanding by considering steady-state conditions, in which the fluid flow does not vary with time, and by assuming there are no vertical motions. • To explore these balanced flow conditions, it is useful to define a new coordinate system, known as natural coordinates. Natural Coordinates • Natural coordinates are defined by a set of mutually orthogonal unit vectors whose orientation depends on the direction of the flow. Unit vector tˆ points along the direction of the flow. ˆ k kˆ Unit vector nˆ is perpendicular to ˆ t the flow, with positive to the left. kˆ nˆ ˆ t nˆ Unit vector k ˆ points upward. ˆ ˆ t nˆ tˆ k nˆ ˆ r k kˆ Horizontal velocity: V = Vtˆ tˆ kˆ nˆ ˆ V is the horizontal speed, t nˆ ˆ which is a nonnegative tˆ tˆ k nˆ scalar defined by V ≡ ds dt , nˆ where s ( x , y , t ) is the curve followed by a fluid parcel moving in the horizontal plane. To determine acceleration following the fluid motion, r dV d = ()Vˆt dt dt r dV dV dˆt = ˆt +V dt dt dt δt δs δtˆ δψ = = = δtˆ t+δt R tˆ δψ δψ R radius of curvature (positive in = R δs positive n direction) t n R > 0 if air parcels turn toward left R < 0 if air parcels turn toward right ˆ dtˆ nˆ k kˆ = (taking limit as δs → 0) tˆ R < 0 ds R kˆ nˆ ˆ ˆ ˆ t nˆ dt dt ds nˆ ˆ ˆ = = V t nˆ tˆ k dt ds dt R R > 0 nˆ r dV dV dˆt = ˆt +V dt dt dt r 2 dV dV V vector form of acceleration following = ˆt + nˆ dt dt R fluid motion in natural coordinates r − fkˆ ×V = − fVnˆ Coriolis (always acts normal to flow) ⎛ˆ ∂Φ ∂Φ ⎞ − ∇ pΦ = −⎜t + nˆ ⎟ pressure gradient ⎝ ∂s ∂n ⎠ dV ∂Φ = − dt ∂s component equations of horizontal V 2 ∂Φ momentum equation (isobaric) in + fV = − natural coordinate system R ∂n dV ∂Φ = − Balance of forces parallel to flow. -
GEF 1100 – Klimasystemet Chapter 7: Balanced Flow
GEF1100–Autumn 2014 30.09.2014 GEF 1100 – Klimasystemet Chapter 7: Balanced flow Prof. Dr. Kirstin Krüger (MetOs, UiO) 1 Ch. 7 – Balanced flow 1. Motivation Ch. 7 2. Geostrophic motion 2.1 Geostrophic wind – 2.2 Synoptic charts 2.3 Balanced flows 3. Taylor-Proudman theorem 4. Thermal wind equation* 5. Subgeostrophic flow: The Ekman layer 5.1 The Ekman layer* 5.2 Surface (friction) wind 5.3 Ageostrophic flow 6. Summary Lecture Outline Lecture 7. Take home message *With add ons. 2 1. Motivation Motivation x Oslo wind forecast for today 12–18: 2 m/s light breeze, east-northeast x www.yr.no 3 2. Geostrophic motion Scale analysis – geostrophic balance Consider magnitudes of first 2 terms in momentum eq. for a fluid on a rotating 퐷퐮 1 sphere (Eq. 6-43 + f 풛 × 풖 + 훻푝 + 훻훷 = ℱ) for horizontal components 퐷푡 휌 in a free atmosphere (ℱ=0,훻훷=0): 퐷퐮 휕푢 • +f 풛 × 풖 = +풖 ∙ 훻풖 + f 풛 × 풖 퐷푡 휕푡 Large-scale flow magnitudes in atmosphere: 푈 푈2 fU 푢 and 푣 ∼ 풰, 풰∼10 m/s, length scale: L ∼106 m, 5 2 -4 -2 푇 time scale: 풯 ∼10 s, U/ 풯≈ 풰 /L ∼10 ms , 퐿 f ∼ 10-4 s-1 10−4 10−4 10−3 45° • Rossby number: - Ratio of acceleration terms (U2/L) to Coriolis term (f U), - R0=U/f L - R0≃0.1 for large-scale flows in atmosphere -3 (R0≃10 in ocean, Chapter 9) 4 2. Geostrophic motion Scale analysis – geostrophic balance • Coriolis term is left (≙ smallness of R0) together with the pressure gradient term (~10-3): 1 f 풛 × 풖 + 훻푝 = 0 Eq. -
Climatology of the Great Plains Low Level Jet Using a Balanced Flow Model with Linear Friction By
Climatology of the Great Plains Low Level Jet Using a Balanced Flow Model with Linear Friction by Stephanie Marder Vaughn Submitted to the Department of Civil and Environmental Engineering in Partial Fulfillment of the Requirements of the Degree of Master of Science in Civil and Environmental Engineering at the Massachusetts Institute of Technology June 1996 @ Massachusetts Institute of Technology 1996. All Rights Reserved. Signature of Author....................... .. .......... ................. Department of Civil and Environmenal Engineering March 29, 1996 Certified by................................... ........................................... ............ .. Dara Entekhabi Associate Professor Thesis Supervisor •i Chairman, Departmental Connmittee on Graduate Studih. iMASSACHUSETTS INS'ITiJ TE OF TECHNOLOGY JUN 0 5 1996 LIBRARIES . ·1 Climatology of the Great Plains Low Level Jet Using a Balanced Flow Model with Linear Friction by Stephanie Marder Vaughn Submitted to the Department of Civil and Environmental Engineering on March 29, 1996 in Partial Fulfillment of the Requirements of the Degree of Master of Science in Civil and Environmental Engineering Abstract The nighttime low-level-jet (LLJ) originating from the Gulf of Mexico carries moisture into the Great Plains area of the United States. The LLJ is considered to be a major contributor to the low-level transport of water vapor into this region. In order to study the effects of this jet on the climatology of the Great Plains, a balanced-flow model of low- level winds incorporating a linear friction assumption is applied. Two summertime data sets are used in the analysis. The first covers an area from the Gulf of Mexico up to the Canadian border. This 10 x 10 resolution data is used, first, to determine the viability of the linear friction assumption and, second, to examine the extent of the LLJ effects. -
Chapter 7 Balanced Flow
Chapter 7 Balanced flow In Chapter 6 we derived the equations that govern the evolution of the at- mosphere and ocean, setting our discussion on a sound theoretical footing. However, these equations describe myriad phenomena, many of which are not central to our discussion of the large-scale circulation of the atmosphere and ocean. In this chapter, therefore, we focus on a subset of possible motions known as ‘balanced flows’ which are relevant to the general circulation. We have already seen that large-scale flow in the atmosphere and ocean is hydrostatically balanced in the vertical in the sense that gravitational and pressure gradient forces balance one another, rather than inducing accelera- tions. It turns out that the atmosphere and ocean are also close to balance in the horizontal, in the sense that Coriolis forces are balanced by horizon- tal pressure gradients in what is known as ‘geostrophic motion’ – from the Greek: ‘geo’ for ‘earth’, ‘strophe’ for ‘turning’. In this Chapter we describe how the rather peculiar and counter-intuitive properties of the geostrophic motion of a homogeneous fluid are encapsulated in the ‘Taylor-Proudman theorem’ which expresses in mathematical form the ‘stiffness’ imparted to a fluid by rotation. This stiffness property will be repeatedly applied in later chapters to come to some understanding of the large-scale circulation of the atmosphere and ocean. We go on to discuss how the Taylor-Proudman theo- rem is modified in a fluid in which the density is not homogeneous but varies from place to place, deriving the ‘thermal wind equation’. Finally we dis- cuss so-called ‘ageostrophic flow’ motion, which is not in geostrophic balance but is modified by friction in regions where the atmosphere and ocean rubs against solid boundaries or at the atmosphere-ocean interface. -
Downloaded 09/23/21 08:03 PM UTC 2556 MONTHLY WEATHER REVIEW VOLUME 126 Centrated at the Tropopause
OCTOBER 1998 MORGAN AND NIELSEN-GAMMON 2555 Using Tropopause Maps to Diagnose Midlatitude Weather Systems MICHAEL C. MORGAN Department of Atmospheric and Oceanic Sciences, University of WisconsinÐMadison, Madison, Wisconsin JOHN W. N IELSEN-GAMMON Department of Meteorology, Texas A&M University, College Station, Texas (Manuscript received 23 June 1997, in ®nal form 28 November 1997) ABSTRACT The use of potential vorticity (PV) allows the ef®cient description of the dynamics of nearly balanced at- mospheric ¯ow phenomena, but the distribution of PV must be simply represented for ease in interpretation. Representations of PV on isentropic or isobaric surfaces can be cumbersome, as analyses of several surfaces spanning the troposphere must be constructed to fully apprehend the complete PV distribution. Following a brief review of the relationship between PV and nearly balanced ¯ows, it is demonstrated that the tropospheric PV has a simple distribution, and as a consequence, an analysis of potential temperature along the dynamic tropopause (here de®ned as a surface of constant PV) allows for a simple representation of the upper-tropospheric and lower-stratospheric PV. The construction and interpretation of these tropopause maps, which may be termed ``isertelic'' analyses of potential temperature, are described. In addition, techniques to construct dynamical representations of the lower-tropospheric PV and near-surface potential temperature, which complement these isertelic analyses, are also suggested. Case studies are presented to illustrate the utility of these techniques in diagnosing phenomena such as cyclogenesis, tropopause folds, the formation of an upper trough, and the effects of latent heat release on the upper and lower troposphere. -
Announcements
Announcements • HW5 is due at the end of today’s class period • Exam 2 is due next Wednesday (4 Nov) • Let me know if you have any conflicts or problems with this due date related to election day on 3 Nov • The exam will be posted on the class Canvas web page after Friday’s review session on 30 Oct • The exam will be a closed book exam but you will be allowed to use one double-sided cheat sheet • You should plan to complete the exam in one sitting in about 2 hours • The completed exam needs to be e-mailed to me by no later than 1:45PM on Wednesday 4 Nov • During Friday’s review session I will be happy to answer any questions about material that may be on exam 2 Balanced Flow • We will consider balanced flows in which the wind is parallel to height (pressure) contours and the horizontal momentum equation reduces to: �! �Φ + �� = − � �� • We will look at all possible force balances represented by this equation and consider when each of these balances is most appropriate. Balanced Flow: Inertial Flow • Assume negligible pressure gradient �! + �� = 0 � • What is the path followed by an air parcel for this force balance? � � = − � Antarctic Inertial Flow Balanced Flow: Cyclostrophic Flow " ! " $ • Rossby number: �� = # = #$ #% • What conditions result in a large Rossby number? • What does a large Rossby number imply about the force balance acting on the flow? �! �Φ = − � �� Balanced Flow: Cyclostrophic Flow • Can cyclostrophic flow occur around both low and high pressure centers? �Φ &.( � = −� �� Balanced Flow: Cyclostropic Flow Example: A tornado is observed to have a radius of 600 m and a wind speed of 130 m s-1 - What is the Rossby number for this flow? - Estimate the pressure at the center of this tornado, assuming that the pressure at the outer edge of the tornado is 1000 mb. -
The Coriolis Effect, Geostrophy, Winds and the General Circulation of The
VII. the Coriolis effect, winds, storms and the general circulation of the atmosphere clicker question absorbed solar emitted IR (OLR) The local imbalances of received and emitted radiation (above) mean that: a) the poles will cool forever, b) the tropics will heat up forever, c) both a & b, d) there must be a poleward transport of heat, e) there must be an equatorward transport of heat clicker question heating at the surface leads to: a) expansion of air, b) buoyancy, c) convection, d) gradients of pressure, e) all of the above review (from last week) northern limb Hadley cell 500 mb high low 500 mb 950 mb low high 1050 mb tropics extra (30 °N) tropics the horizontal movements of air can be satisfied by buoyancy driven vertical movements, comprising a circulation cell, such as the Hadley cell review (from last week) • differential heating leads to gradients of pressure • air moves from areas of high pressure to areas of low pressure • but does air always move in a straight line? surface pressure mbar surface pressure “belts” high low high low high low another high down under pressure-force-only winds is this the observed pattern? the Coriolis effect • Newton says pushed objects will move in a straight line, but....... • the coriolis force describes the apparent tendency of a fluid (air or water) moving across the surface of the Earth to be deflected from its straight line path • this is not a real force, but apparent only from the w/in of the rotating Earth system (an observer in space would not note deflection) • let’s see a simple experiment platter is stationary Newton was right! a simple experiment platter now rotates! what happened ??????? how would it look from above? the Coriolis effect • Newton says pushed objects will move in a straight line, but...... -
A New Pendulum Motion with a Suspended Point Near Infinity
www.nature.com/scientificreports OPEN A new pendulum motion with a suspended point near infnity A. I. Ismail In this paper, a pendulum model is represented by a mechanical system that consists of a simple pendulum suspended on a spring, which is permitted oscillations in a plane. The point of suspension moves in a circular path of the radius (a) which is sufciently large. There are two degrees of freedom for describing the motion named; the angular displacement of the pendulum and the extension of the spring. The equations of motion in terms of the generalized coordinates ϕ and ξ are obtained using Lagrange’s equation. The approximated solutions of these equations are achieved up to the third order of approximation in terms of a large parameter ε will be defned instead of a small one in previous studies. The infuences of parameters of the system on the motion are obtained using a computerized program. The computerized studies obtained show the accuracy of the used methods through graphical representations. Te pendulum motions are studied in many works 1–7. Te motion of the pendulum on an ellipse is studied in 8. Te supported point of this pendulum moves on an ellipse path while the end moves with arbitrary angular dis- placements. Te equation of motion is obtained and solved for one degree of freedom ϕ . In9, the relative periodic solutions of a rigid body suspended on an elastic string in a vertical plane are considered. Te equations of motion are obtained and solved in terms of the small parameter ε .