Downloaded 09/23/21 08:03 PM UTC 2556 MONTHLY WEATHER REVIEW VOLUME 126 Centrated at the Tropopause

Total Page:16

File Type:pdf, Size:1020Kb

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. 1. Introduction (Shapiro and Grell 1994), but the evolution of VIP is not governed by a single two-dimensional wind ®eld. For potential vorticity (PV) to be qualitatively applied Bleck (1990) proposed the three-dimensional depic- in describing the evolution of tropospheric synoptic- tion of an isosurface of isentropic vorticity (the vertical scale ¯ows, the three-dimensional PV and surface po- component of absolute vorticity computed from winds tential temperature distributions must be simply repre- along an isentropic surface). Bleck's technique has the sented and easily interpreted. Toward this goal, Hoskins advantage of combining upper- and lower-tropospheric et al. (1985, HMR hereafter) have advocated the con- information onto a single map, but with a resulting loss struction of isentropic PV analyses and surface potential of precision as to the locations and amplitudes of various temperature maps to describe and represent dynamical features. Also, unlike PV, isentropic vorticity is not con- processes within the atmosphere. By plotting Ertel PV served following adiabatic, frictionless ¯ow, so that the on an isentropic surface, one has the advantage of view- evolution of the isentropic vorticity ®eld is dif®cult to ing the dynamics of a conserved variable along the sur- infer from an instantaneous depiction. Alternatively, face of another conserved variable. Thus, with the wind three-dimensional isosurfaces of Ertel PV have been ®eld superposed on an isentropic analysis of PV, one utilized by several authors (including Uccellini 1990; may deduce the conservative (advective) time tendency Lamarque and Hess 1994; Rotunno et al. 1994) to depict of the PV. A distinct disadvantage of this technique is the structure of the tropopause during tropopause fold that several isentropic surfaces must be viewed in order events. This provides a clear depiction of the distribu- to apprehend the full three-dimensional distribution of tion of PV, but like Bleck's method, it is dif®cult to PV and PV advection. Alternatively, the mean PV with- incorporate wind information to infer the evolution. in all layers intersecting the tropopause, or VIP (ver- The focus of this paper is the analysis of both po- tically integrated potential vorticity), may be plotted tential temperature and wind along a two-dimensional projection of the dynamic tropopause (de®ned as a sur- face of constant Ertel PV). This analysis (here referred to as a tropopause map) exploits the rather simple dis- Corresponding author address: Prof. Michael C. Morgan, De- partment of Atmospheric Sciences, University of WisconsinÐMad- tribution of tropospheric PV: as will be demonstrated ison, 1225 West Dayton St., Madison, WI 53706. in the next section, isentropic gradients of PV are con- q 1998 American Meteorological Society Unauthenticated | Downloaded 09/23/21 08:03 PM UTC 2556 MONTHLY WEATHER REVIEW VOLUME 126 centrated at the tropopause. Tropopause maps are a com- tial, w), a similarly truncated form of the vorticity equa- pact way to represent this distribution. Thus, the essen- tion, a thermodynamic equation, and a mass conser- tial character of the upper-tropospheric PV may be de- vation equation. The initial conditions in a time inte- picted on a single chart, rather than several isentropic gration of a balance system need only be speci®ed by maps. a single variable (Gent and McWilliams 1983). A fa- Tropopause maps, often in conjunction with analyses miliar example is a ¯ow satisfying the quasigeostrophic of lower-tropospheric potential temperature, have been system. As long as z/f 0 .21 (where z is the relative used by many authors in studies of surface cyclogenesis vorticity and f 0 is a characteristic midlatitude value of (e.g., Hoskins and Berrisford 1988; Davis and Emanuel the Coriolis parameter), all ®elds (wind, temperature, 1991; Hakim et al. 1995; Bosart et al. 1996; Bresky and vertical motion, and height tendency) may be expressed Colucci 1996). Thorncroft et al. (1993) used the anal- in terms of the instantaneous geopotential height ®eld. yses to compactly represent the evolution of upper-tro- All ®elds could also, in principle, be speci®ed in terms pospheric PV in a modeling study of life cycles of bar- of the instantaneous temperature ®eld, or even a single oclinic waves. Upper-level systems examined using tro- component of the wind ®eld. popause maps include a tropopause fold (Nielsen et al. The PV can also be used for this purpose. In their 1991), a blocking anticyclone (Morgan et al. 1991), a review, HMR discussed the principles of conservation cutoff cyclone (Bell and Bosart 1993), and mobile and invertibility of PV. The invertibility principle states troughs (Nielsen-Gammon 1995; Lackmann et al. 1997). that the three-dimensional distribution of PV within Wu and Emanuel (1993) and Bosart and Lackmann some domain and boundary conditions on that domain (1995) used the analyses to represent the out¯ow from uniquely determine the velocity and temperature distri- tropical cyclones and the interaction of tropical cyclones bution consistent with a particular balance constraint. with midlatitude systems. The conservation principle states that for inviscid ¯ows Despite the growing use of such analyses, no com- in which the gradient of diabatic heating does not project prehensive discussion of the motivation for these anal- onto the local absolute vorticity vector, PV is conserved yses, nor a guide to constructing or interpreting them, following the ¯uid motion. Together, conservation and has been presented. The intent of this paper is to present invertibility imply that the dynamics of quasi-balanced various techniques for representing the dynamically im- ¯ows may be expressed simply and entirely in terms of portant characteristics of the tropospheric PV distribu- the distribution of PV and the boundary conditions nec- tion in a compact form and to offer an interpretation for essary in the inversion1 of the PV. The use of conser- these representations. The paper is divided into six sec- vation and invertibility to infer the dynamics of quasi- tions, any of which may be skipped without serious loss balanced ¯ows is called ``PV thinking.'' of continuity. In section 2, the theoretical and obser- A simple example of conservation and invertibility vational motivation for tropopause maps is presented. is nondivergent barotropic ¯ow. For such a ¯ow, the Section 3 describes and contrasts the various techniques absolute vorticity and lateral boundary conditions con- one might use to represent the PV near the tropopause tain all of the dynamical information concerning the and the potential temperature and PV distribution in the ¯uid motion. The streamfunction ®eld, which can be lower troposphere. The next two sections are brief case determined from the relative vorticity ®eld through the studies of cyclogenesis that illustrate how tropopause inversion of a two-dimensional elliptic operator, com- maps may be used to diagnose and interpret synoptic- pletely speci®es the velocity ®eld. The balance condi- scale (i.e., quasi-balanced) weather systems. A summary tion that this ¯ow satis®es is nonlinear balance. and further suggestions for how these analyses might In the quasigeostrophic (QG) system, the quasigeo- be utilized is presented in section 6. strophic potential vorticity (hereafter QGPV,also known as the pseudo-PV) is conserved following the geo- strophic ¯ow (Charney and Stern 1962). Quasigeos- 2. Observational and dynamical motivation trophic PV, qp, is de®ned as a. Balanced ¯ow, PV, and PV inversion 1 ] 1 ] q 2 f [¹2w91 f w9 , (2.1) A characteristic of low Rossby number ¯ow in rotating p 0 f0 ]pS12]p ¯uids is the tendency of the ¯ow toward balance. A general type of balance, which subsumes geostrophic balance and where f is the
Recommended publications
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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......
    [Show full text]
  • Accurate Boussinesq Oceanic Modeling with a Practical, В
    Ocean Modelling 38 (2011) 41–70 Contents lists available at ScienceDirect Ocean Modelling journal homepage: www.elsevier.com/locate/ocemod Accurate Boussinesq oceanic modeling with a practical, ‘‘Stiffened’’ Equation of State ⇑ Alexander F. Shchepetkin , James C. McWilliams Institute of Geophysics and Planetary Physics, University of California, 405 Hilgard Avenue, Los Angeles, CA 90095-1567, United States article info abstract Article history: The Equation of State of seawater (EOS) relates in situ density to temperature, salinity and pressure. Most Received 9 August 2008 of the effort in the EOS-related literature is to ensure an accurate fit of density measurements under the Received in revised form 25 December 2010 conditions of different temperature, salinity, and pressure. In situ density is not of interest by itself in oce- Accepted 31 January 2011 anic models, but rather plays the role of an intermediate variable linking temperature and salinity fields Available online 13 February 2011 with the pressure-gradient force in the momentum equations, as well as providing various stability func- tions needed for parameterization of mixing processes. This shifts the role of EOS away from representa- Keywords: tion of in situ density toward accurate translation of temperature and salinity gradients into adiabatic Seawater Equation of State derivatives of density. Seawater compressibility Barotropic–baroclinic mode splitting In this study we propose and assess the accuracy of a simplified, computationally-efficient algorithm Boussinesq and
    [Show full text]
  • Balanced Flow: Large-Scale Balances Geostrophic Motion Now Go Back to the Equations of Motion in a Rotating Framework
    Balanced Flow: Large-Scale Balances Geostrophic Motion Now go back to the equations of motion in a rotating framework Geostrophic Balance A very powerful constraint on large-scale flows But what happens near the equator? Geostrophic flow is horizontally nondivergent! At a boundary But the atmosphere is not incompressible So we head back to pressure coordinates! Geostrophic Wind in pressure coordinates Highs and Lows in Synoptic Charts Gradient wind balance Balanced flow in the radial-inflow experiment Angular Momentum Magnified at small r Cyclostrophic and Geostrophic limits of Gradient Wind Balance The Taylor-Proudman Theorem Vertical Component of is of If is the gradient along The Taylor-Proudman Theorem Taylor-Proudman Theorem Taylor Columns The Thermal Wind Equation Geostrophic flow should increase with height True in the real world But the atosphere is ot really arotropi……so Consider water - So thermal wind is just geostrophy and hydrostatic balance! Analogous to - Thermal Winds in the Lab In Spherical Coordinates The Thermal Wind Equation and the Taylor- Proudman Theorem How does the fluid adjust on large scales when gravitational pull downward is counterbalanced by the rigidity of the Taylor columns? This is a general statement of the thermal wind Reduces to Because is parallel to But…………………. for a Barolii Fluid - If is Baroclinicity If and Then (7 – 20) is the same as This is why temperature surfaces can maintain the slopes despite gravity – Earth’s rotatio a alae gravity Cylinder Collapse under Gravity and Rotation Theory following
    [Show full text]
  • Meeting Review
    meeting review Eighth Cyclone Workshop Scientific Summary, Val Morin, Quebec, Canada, 12-16 October 1992 Rainer Bleck,* Howard Bluestein,+ Lance Bosart,@ W. Edward Bracken,@ Toby Carlson,++ Jeffrey Chapman,@ Michael Dickinson,@ John R. Gyakum,++ Gregory Hakim,@ Eric Hoffman,@ Haig lskenderian,@ Daniel Keyser,@ Gary Lackmann,@ Wendell Nuss,@@ Paul Roebber,@ Frederick Sanders,*** David Schultz,@ Kevin Tyle,@ and Peter Zwack+++ Abstract in the Washington, D.C., area in October 1978. Donald Johnson chaired a preliminary planning meeting (at- The Eighth Cyclone Workshop was held at the Far Hills Inn and tending were Lance Bosart, John Cahir, John Conference Center in Val Morin, Quebec, Canada, 12-16 October Hovermale, Carl Kreitzberg, Chester Newton, Norman 1992. The workshop was arranged around several scientific themes Phillips, Frederick Sanders, Phillip Smith, Ronald Tay- of current research interest. The most widely debated theme was the applicability of "potential vorticity thinking" to theoretical, observa- lor, Dayton Vincent, and Johnson) in which it was tional, and numerical studies of the life cycle of cyclones and the generally agreed that a focused research effort on the interaction of these cyclones with their environment on all spatial extratropical cyclone should be initiated and carried and temporal scales. A combination of invited and contributed talks, out, and the findings debated at periodic scientific with preference given to younger scientists, made up the workshop. workshops. Johnson agreed to serve as the chair of the informal Extratropical Cyclone Project Steering Com- 1. Workshop background mittee (other steering committee members included David Baumhefner, Bosart, Hovermale, Smith, Taylor, Working scientists and students interested in cy- and Vincent), which would arrange and organize the clone-related research problems have used the venue workshops.
    [Show full text]
  • An Introduction to Dynamic Meteorology.Pdf
    January 24, 2004 12:0 Elsevier/AID aid An Introduction to Dynamic Meteorology FOURTH EDITION January 24, 2004 12:0 Elsevier/AID aid This is Volume 88 in the INTERNATIONAL GEOPHYSICS SERIES A series of monographs and textbooks Edited by RENATADMOWSKA, JAMES R. HOLTON and H.THOMAS ROSSBY A complete list of books in this series appears at the end of this volume. January 24, 2004 12:0 Elsevier/AID aid AN INTRODUCTION TO DYNAMIC METEOROLOGY Fourth Edition JAMES R. HOLTON Department of Atmospheric Sciences University of Washington Seattle,Washington Amsterdam Boston Heidelberg London New York Oxford Paris San Diego San Francisco Singapore Sydney Tokyo January 24, 2004 12:0 Elsevier/AID aid Senior Editor, Earth Sciences Frank Cynar Editorial Coordinator Jennifer Helé Senior Marketing Manager Linda Beattie Cover Design Eric DeCicco Composition Integra Software Services Printer/Binder The Maple-Vail Manufacturing Group Cover printer Phoenix Color Corp Elsevier Academic Press 200 Wheeler Road, Burlington, MA 01803, USA 525 B Street, Suite 1900, San Diego, California 92101-4495, USA 84 Theobald’s Road, London WC1X 8RR, UK This book is printed on acid-free paper. Copyright c 2004, Elsevier Inc. All rights reserved. No part of this publication may be reproduced or transmitted in any form or by any means, electronic or mechanical, including photocopy, recording, or any information storage and retrieval system, without permission in writing from the publisher. Permissions may be sought directly from Elsevier’s Science & Technology Rights Department in
    [Show full text]