Pressure Fluctuations Associated with Deep Moist Convection.

Slides:



Advertisements
Similar presentations
Tornado Workshop Langen, Germany, 25 February 2005 Contents 1. Basics –Parcel Theory –Perturbation pressure field –Updraft Rotation 2. Thunderstorm Classes.
Advertisements

The Quasi-Geostrophic Omega Equation (without friction and diabatic terms) We will now develop the Trenberth (1978)* modification to the QG Omega equation.
Chapter 2: basic equations and tools 2.5 – pressure perturbations 2.6 – thermodynamic diagrams hodographs All sections are considered core material,
Hurricane Dynamics 101 Roger K. Smith University of Munich.
Cumulus Forced; pushed upward by external forces, i.e. lifting by surface convergence, topography etc. Active; growing upward from self-forcing, i.e. buoyancy,
Geostrophic Adjustment Recall winds adjust to mass for scales larger than L R and mass adjust to wind for scales smaller than L R. In mid-latitude squall.
Weismann (1992) Weisman, M. L., 1992: The role of convectively generated rear- inflow jets in the evolution of long-lived mesoconvective systems. J. Atmos.
Atmospheric Motion ENVI 1400: Lecture 3.
Vorticity.
“Dynamical Effects of Convection” Kathryn Saussy Meteorology 515: Analysis & Pred. of Severe Storms March Bluestein, Howard: Synoptic-Dynamic Meteorology.
MET 61 1 MET 61 Introduction to Meteorology MET 61 Introduction to Meteorology - Lecture 12 Midlatitude Cyclones Dr. Eugene Cordero San Jose State University.
Lifting by cold pools (RKW theory) A&OS C115/C228.
Thermally-Driven Circulations in Mountain Terrain.
AOSS 321, Winter 2009 Earth Systems Dynamics Lecture 13 2/19/2009 Christiane Jablonowski Eric Hetland
EOSC 112: THE FLUID EARTH CORIOLIS EFFECT AND GEOSTROPHY Atm3 Read: Kump et al. Chap.4, p Why do weather / climate vary around the globe? Why is.
Deep Convection A review of processes “Everything we hear is an opinion, not a fact. Everything we see is a perspective, not truth” Marcus Aurelius: AD
Hans Burchard Leibniz Institute for Baltic Sea Research Warnemünde Coastal Ocean Dynamics First course: Hydrodynamics.
Presentation Slides for Chapter 5 of Fundamentals of Atmospheric Modeling 2 nd Edition Mark Z. Jacobson Department of Civil & Environmental Engineering.
Things to look for on the weather maps Visible and IR satellite images (& radar too): Look at cloud movements and locations - do they correlate with what.
Basic dynamics  The equations of motion and continuity Scaling Hydrostatic relation Boussinesq approximation  Geostrophic balance in ocean’s interior.
TMD Lecture 2 Fundamental dynamical concepts. m Dynamics Thermodynamics Newton’s second law F x Concerned with changes in the internal energy and state.
CEE 262A H YDRODYNAMICS Lecture 18 Surface Ekman layer.
PRECIPITATION PROCESSES AT FRONTS. POSSIBLE CONDITIONS PRESENT AT FRONT 1.Air ahead of the front is stable to all forms of instability Forcing mechanism.
Cumulus Clouds. What goes on inside a cumulus cloud?
Solid body rotation (XY):
Sensitivity of Tropical Cyclone Inner-Core Size and Intensity to the Radial Distribution of Surface Entropy Flux Wang, Y., and Xu, 2010: Sensitivity of.
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS FILTERING OF EQUATIONS OF MOTION FOR ATMOSPHERE (CONT) LECTURE 7 (Reference: Peixoto & Oort, Chapter 3,7)
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS FILTERING OF EQUATIONS FOR ATMOSPHERE (CONT) LECTURE 6 (Reference: Peixoto & Oort, Chapter 3)
FLUID ROTATION Circulation and Vorticity. Arbitrary blob of fluid rotating in a horizontal plane Circulation: A measure of the rotation within a finite.
General Theme: ….Consider the evolution of convection in the absence of significant larger-scale forcing influences…or even boundary layer features….
Ekman Flow September 27, 2006.
Deep Moist Convection (DMC) Part 2 – Modes of Isolated Organization AOS 453 – Spring /3/2014.
Paul Markowski Department of Meteorology, Penn State University
ATS/ESS 452: Synoptic Meteorology
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.
CEE 262A H YDRODYNAMICS Lecture 7 Conservation Laws Part III.
Synoptic Scale Balance Equations Using scale analysis (to identify the dominant ‘forces at work’) and manipulating the equations of motion we can arrive.
1 MECH 221 FLUID MECHANICS (Fall 06/07) Tutorial 5.
Convective: Part 2 Weather Systems – Fall 2015 Outline: a. dynamics of rotating thunderstorms (supercells) b. storm splitting – right vs. left movers.
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS TIME-DEPENDENT DYNAMICS; WAVE DISTURBANCES LECTURE 21.
AOSS 401, Fall 2007 Lecture 21 October 31, 2007 Richard B. Rood (Room 2525, SRB) Derek Posselt (Room 2517D, SRB)
Conservation of Salt: Conservation of Heat: Equation of State: Conservation of Mass or Continuity: Equations that allow a quantitative look at the OCEAN.
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
Principles of Convection. BACKGROUND When vertical shear is weak, the main influence on convective updrafts & downdrafts is bouyancy. As the vertical.
AOSS 401, Fall 2006 Lecture 16 October 19, 2007 Richard B. Rood (Room 2525, SRB) Derek Posselt (Room 2517D, SRB)
ATM OCN Fall ATM OCN Fall 1999 LECTURE 17 THE THEORY OF WINDS: PART II - FUNDAMENTAL FORCES A. INTRODUCTION –How do winds originate? –What.
Cumulus Clouds. Instabilities Resulting in Vertical Overturning 1.Thermal Instability (Assuming uniform vertical pressure gradient) a) Static (Parcel.
Class #11 Monday, February 2 Class #11: Monday, February 2 Chapter 6 Forces and winds 1.
The vector measure of rotation around a point
1 This is the footer Midlatitude Weather systems Geraint Vaughan University of Manchester NCAS Director of Observations.
Atmospheric Dynamics Suzanne Gray (University of Reading) With thanks to Alan Gadian and Geraint Vaughan. Basic dynamical concepts.
Dynamics  Dynamics deals with forces, accelerations and motions produced on objects by these forces.  Newton’s Laws l First Law of Motion: Every body.
The Boussinesq and the Quasi-geostrophic approximations
Geostrophic adjustment
Supercells: Theory Richard Rotunno
Synoptic Scale Balance Equations
Vorticity Vertical component of vorticity: i.e., the rotation about the local vertical There are three types of vorticity used in geophysical fluid dynamics.
Dynamics Vorticity In the previous lecture, we used “scaling” to simplify the equations of motion and found that, to first order, horizontal winds are.
Convective: Part 2 Weather Systems – Fall 2017
ATS/ESS 452: Synoptic Meteorology
Shawnee/ Moore, Oklahoma May 20, 2013.
Dynamical Effects of Storm Generated Mesoscale Processes and Pressure perturbations Terrance Seddon.
Richard B. Rood (Room 2525, SRB)
Da-Lin Zhang, Yubao Liu, and M.K. Yau,
Monteverdi, John. Advanced Weather Analysis Lectures, Spring 2005.
Vorticity Objectives Define Vorticity
Vorticity Objectives Define Vorticity
Vorticity Objectives Define Vorticity
Presentation transcript:

Pressure Fluctuations Associated with Deep Moist Convection

Introduction pressure perturbations may arise from density anomalies or from wind speed gradients, and perturbation pressure gradients may, in turn, influence the wind in important ways –reduction of vertical velocity (generally the case) –enhancement of vertical velocity in some special cases (may intensify storms or rotation within storms) –forced lifting of air to the LFC (critical to storm maintenance and propagation) nonhydrostatic vs hydrostatic pressure dynamic vs buoyancy pressure

Review of the origins of pressure perturbations Describe the pressure and density as the sum of a horizontally homogeneous base state pressure and density, respectively, and a deviation from this base state, i.e., The base state is in hydrostatic balance, i.e., The inviscid vertical momentum equation then can be written as

Hydrostatic and nonhydrostatic pressure perturbations We can represent the perturbation pressure as the sum of a hydrostatic pressure perturbation (p’ h ) and a nonhydrostatic pressure perturbation (p’ nh ), i.e., arises from density perturbations by way of the relation Thus we can rewrite the vertical momentum equation as

Where is the velocity vector, is a constant specific volume, and f is the Coriolis parameter (the Coriolis force has been approximated as ). Dynamic and buoyancy pressure perturbations Another common approach undertaken to decompose the perturbation pressure is to form a diagnostic pressure equation by taking the divergence of the three-dimensional momentum equation,

Dynamic and buoyancy pressure perturbations Thus, we have Using, we obtain And after evaluating and, we obtain

Dynamic and buoyancy pressure perturbations very small on all scales dominates on the synoptic scale when p’ is reasonably “well- behaved,”... relatively unimportant on convective scales

Dynamic and buoyancy pressure perturbations Define vorticity (  ) and deformation (D) vectors… Then the pressure equation can be written as

Dynamic and buoyancy pressure perturbations Again, when p’ is reasonably “well-behaved,” such that, then Rotation (of any sense) is associated with low pressure Convergence and divergence (fluid extension terms) are associated with high pressure Deformation is associated with high pressure Low (high) pressure is found below (above) the level of maximum buoyancy

Dynamic and buoyancy pressure perturbations “dynamic pressure” “buoyancy pressure” + part of remainder of

Dynamic and buoyancy pressure perturbations high pressure upshear, low pressure downshear of an updraft

Courtesy of Matt Parker

Results: 2D, no upper-level shear Courtesy of Mike Coniglio

Results: 2D, 10 m s -1 upper- level shear Courtesy of Mike Coniglio