TropicalM. D. Eastin TC Lifecycle and Intensity Changes Part I: Genesis Hurricane Katrina (2005) August 24-29.

Slides:



Advertisements
Similar presentations
What we now know: Difference between weather and climate.
Advertisements

Section 2: The Planetary Boundary Layer
1 Carl Schreck Lifecycle Ingredients ClimatologyData.
What Makes the Wind Blow?
Where Do the Hurricanes Come From?. Radiation Vapor/Cloud/precipitation Shallow convection Boundary layer turbulence Mesoscale convective system Thunderstorm.
Hurricanes and climate ATOC 4720 class22. Hurricanes Hurricanes intense rotational storm that develop in regions of very warm SST (typhoons in western.
Planetary Atmospheres, the Environment and Life (ExCos2Y) Topic 8: Storm Systems Chris Parkes Rm 455 Kelvin Building.
Hurricanes. Tropical Weather Tropics: the belt between the Tropic of Cancer (23.5N) and the Tropic of Capricorn (23.5S) The weather is very different.
Midlatitude Cyclones Equator-to-pole temperature gradient tilts pressure surfaces and produces westerly jets in midlatitudes Waves in the jet induce divergence.
TropicalM. D. Eastin Tropical Cyclone Climatology Where do TCs occur? When? Why? How Many?
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.
HURRICANE DEVELOPMENT What conditions are required? Water temperatures > 26.5°C Convergence of surface winds Upper air divergence Organized mass of thunderstorms.
Tephigrams ENVI1400 : Lecture 8.
Stability & Skew-T Diagrams
Earth Systems Science Chapter 5 OCEAN CIRCULATION I: SURFACE Winds, surface currents Flow within gyres: convergence, divergence, upwelling, downwelling,
Textbook chapter 2, p chapter 3, p chapter 4, p Stability and Cloud Development.
Outline Further Reading: Chapter 08 of the text book - tornadoes - tropical storms - Storm surge Natural Environments: The Atmosphere GE 101 – Spring 2007.
Typhoons and tropical cyclones
Mesoscale Convective Systems Robert Houze Department of Atmospheric Sciences University of Washington Nebraska Kansas Oklahoma Arkansas.
Lectures on Hurricanes Chanh Q. Kieu Department of Atmospheric and Oceanic Science University of Maryland AOSC400, Fall 2008.
Hurricanes. And finally… JOURNAL COLLECTION How they develop What they’re like Where to find them Andrew or Isabel Important test and other information.
Section 5: Tropical Cyclones 5.4 Theories for Genesis CISK WISHE Discussion Resources:
Hurricanes ATS 351 Lecture 12 November 30, Outline Formation Stages of development Structure of hurricanes Saffir-Simpson scale Movement Dissipation.
Atmospheric Analysis Lecture 2.
Characteristics of Isolated Convective Storms Meteorology 515/815 Spring 2006 Christopher Meherin.
Where Do the Hurricanes Come From?. Introduction A tropical cyclone is a rapidly- rotating storm system characterized by a low-pressure center, strong.
II. Synoptic Atmospheric Destabilization Processes Elevated Mixed Layer (EML) Synoptic Lifting Dynamic Destabilization Differential Advection.
Lapse Rates and Stability of the Atmosphere
TropicalM. D. Eastin Cylindrical Coordinate System.
Tropical Cyclones and Hurricanes Read Chapter 11
Tropical Meteorology I Weather Center Event #4 Tropical Meteorology What is Tropical Meteorology? – The study of cyclones that occur in the tropics.
1 The Thermodynamic Diagram Adapted by K. Droegemeier for METR 1004 from Lectures Developed by Dr. Frank Gallagher III OU School of Meteorology.
Chapter 11 Notes Hurricanes. Tropical Storms Boris and Christiana Together-2008 Profile of a Hurrican Most hurricanes form between the latitudes of 5.
Cumulus Clouds. What goes on inside a cumulus cloud?
Frontogenesis – Kinematics & Dynamics
Tropical Cyclone Motion
ThermodynamicsM. D. Eastin We just the covered the large-scale hydrostatic environment… We now need to understand whether a small-scale moist air parcel.
Modeling the Atmospheric Boundary Layer (2). Review of last lecture Reynolds averaging: Separation of mean and turbulent components u = U + u’, = 0 Intensity.
(C, B, A, C, D, D, B, A) x x x x x.
Hurricanes.
Lecture #2 Weather. Convection and Atmospheric Pressure Much of solar energy absorbed by the Earth is used to evaporate water. – Energy stored in water.
Tropical Cyclone Structure
TC Lifecycle and Intensity Changes Part III: Dissipation / Transition
Tropical Severe Local Storms Nicole Hartford. How do thunderstorms form?  Thunderstorms result from moist warm air that rises due to being less dense.
Genesis of Hurricane Julia (2010) from an African Easterly Wave Stefan Cecelski 1 and Dr. Da-Lin Zhang Department of Atmospheric and Oceanic Science, University.
Overview of Tropical Cyclones AOS 453 April 2004 J. P. Kossin CIMSS/UW-Madison.
Chapter 5 - PBL MT 454 Material Based on Chapter 5 The Planetary Boundary Layer.
The Tropics: Convective Processes
Idealized Tropical Cyclone Structure. Tropical Cyclone Extension of the Warm Core middle –level vortex to the surface. Inducement of Ekman pumping Non-linear.
Principles of Convection. BACKGROUND When vertical shear is weak, the main influence on convective updrafts & downdrafts is bouyancy. As the vertical.
1 SourcesSources n AWS/TR-95/001 n AWS TR240 n NAVEDTRA 40970/40971 n JTWC Forecasters Handbook n NEPRF TR n Tropical Weather Course (Keesler) n.
The Tropical Transition of Cyclones: Science Issues and Critical Observations or TC Genesis: A Global Problem Chris Davis (NCAR) Collaborators: Lance Bosart.
Chapter 9 Winds: Small scale and local systems. Scales of motion Smallest - microscale (few meters or less) Middle - Mesoscale (few to about 100 km) Large.
Cumulus Clouds. Instabilities Resulting in Vertical Overturning 1.Thermal Instability (Assuming uniform vertical pressure gradient) a) Static (Parcel.
Weather’s Triple Killer Thunderstorms, Tornadoes & Hurricanes.
Mesoscale Convective Systems. Definition Mesoscale convective systems (MCSs) refer to all organized convective systems larger than supercells Some classic.
TropicalM. D. Eastin TC Lifecycle and Intensity Changes Part I: Genesis Hurricane Katrina (2005) August
TC Structure Theta_e Structure Grid 3: Vertical motion surfaces 15:30 UTC 26 August, m/s – red -1 m/s -blue +0.5 m/s – red -0.5 m/s -blue.
Yumin Moon & David S. Nolan (2014)
Dynamics of Thunderstorms Part 1: Downdraft Organization Lecture 12a
The Genesis of Hurricane Guillermo: TEXMEX Analyses and a Modeling Study BISTER AND EMANUEL.
Downdraft Storms Lecture 12a
Cyclogenesis in Polar Airstreams
Stability and Cloud Development
The Course of Synoptic Meteorology
Hurricanes.
The Course of Synoptic Meteorology
Presentation transcript:

TropicalM. D. Eastin TC Lifecycle and Intensity Changes Part I: Genesis Hurricane Katrina (2005) August 24-29

TropicalM. D. Eastin Outline Tropical Cyclone Genesis Large-Scale Factors Easterly Waves and MCVs CISK Mechanism WISHE Mechanism VHT Mechanism

TropicalM. D. Eastin TC Genesis Genesis: The transformation of a “disorganized” cold-core convective system into a self-sustaining synoptic-scale warm-core vortex with a cyclonic circulation at the surface Necessary (but not sufficient) Conditions: Pre-existing convection Significant planetary vorticity Favorable wind shear pattern Moist Mid-troposphere Warm ocean with deep mixed layer Conditionally unstable atmosphere

TropicalM. D. Eastin Pre-existing Convection: Source of latent heating Persistent heating in one area will lower the local surface pressure and begin to converge air toward the low pressure (recall the hypsometric equation) TC Genesis

TropicalM. D. Eastin Significant Planetary Vorticity: Convection near the equator results in little if any rotation in the low-level inflow Convection off the equator will contain rotation in the low level inflow due to appreciable Coriolis forcing Systems need to be ~5º off the equator in order to have a chance for development TC Genesis

TropicalM. D. Eastin Favorable Wind Shear Pattern: Wind shear is often defined as the vector difference between winds at two altitudes (850 and 200 mb) Low magnitudes of shear (< 20 knots) are desired TC Genesis High westerly shearLow easterly shear Bad – convection torn apart Good – latent heat can concentrate in one area

TropicalM. D. Eastin Moist Mid-Troposphere: Dry air will lead to evaporation and cooling Cooling produces a surface high pressure, low-level divergence, sinking air, and a suppression of convection TC Genesis Red Areas = Dry Gray/Blue Areas = Moist GOES Water Vapor Image Strong downdrafts = Outflow Boundaries

TropicalM. D. Eastin Warm Ocean: Allows for sensible and latent heat fluxes from the ocean in order to sustain deep convection SSTs > 26.5ºC is the rule TC Genesis Deep Convection L Standard Flux Equations The inflowing air gains heat and moisture only if the ocean is warmer and moister than the air

TropicalM. D. Eastin Deep Oceanic Mixed Layer: Mixed layer: Nearly isothermal ocean layer from the surface to a depth where temperatures cool rapidly (the thermocline) Strong winds churn up cool water from the thermocline or below Deeper mixed layers prevent the cooling of surface waters Cold surface waters limit (or reverse) sensible and latent heat fluxes, reducing convection TC Genesis Mixed Layer

TropicalM. D. Eastin Conditionally Unstable Atmosphere: Lapse rate between the dry adiabatic and moist adiabatic lapse rates Parcels become unstable only when lifted to their Level of Free Convection (LFC) Further ascent produces latent heat release and locally warm air (lowers surface pressure) Frictional convergence produces lift TC Genesis Sounding on a Skew-T

TropicalM. D. Eastin Easterly Waves Origin: Develop over sub-Saharan Africa from instabilities along the African Easterly Jet Basics: Wavelengths of ~3000 km Move westward at 6-8 m/s easterly waves cross the Atlantic each year between July and October 7-9 develop into tropical cyclones Why do we care about easterly waves? Often emerge over warm waters with convection Like mid-latitude synoptic waves, have preferred regions of lift (east of the trough): helps generate persistent convection in the same location Often contain mid-level (but not surface) vortices Systems “pre-conditioned” for successful genesis

TropicalM. D. Eastin Mesoscale Convective Vortices (MCVs) Origin: Develop within persistent mesoscale convection from heating aloft (convection) and cooling below (cold downdrafts) Basics: Confined to mid-levels with little or no signature at the surface Often present in easterly waves Dynamically stable (last several days) Multiple convective cycles Can emerge from the continental U.S. and developed into tropical cyclones (e.g. Hurricane Danny 1997) Why do we care about MCVs? Often emerge over warm waters with convection Systems “pre-conditioned” for successful genesis Cold Typical MCV Cross-Section Warm Positive Vorticity Negative Vorticity

TropicalM. D. Eastin TC Genesis One of the greatest enigmas of tropical meteorology: How do we transform a cold-core synoptic-scale disturbance with a mid-level vortex to a warm-core system with a surface vortex? “This question has been asked at every tropical cyclone conference since the dawn of time.” (Dr. Bill Gray, 2003)

TropicalM. D. Eastin Convective Instability of the Second Kind (CISK): First proposed by Jule Charney in 1964 Assumes the atmosphere is conditionally unstable Requires the presence of a finite amplitude synoptic scale disturbance (easterly wave) Assumes latent heat release results from synoptic-scale frictional convergence Remaining question: How does the surface vortex form? Genesis via the CISK Mechanism Jule Charney

TropicalM. D. Eastin Genesis via the CISK Mechanism 1 Friction with surface causes inflow into the disturbance to be “deflected” inward toward the surface center. Mass continuity dictates upward motion must result. This process is called “Ekman Pumping” Upward motion causes saturation and thus latent heat release. If conditionally unstable, upward motion will continue and enhance secondary circulation. Vortex will stretch, which will develop and intensify low-level cyclonic vorticity (through conservation of angular momentum) 2 Latent Heat Release L Charney and Eliassen (1964) showed that CISK developed a TC with a diameter of 100 km in 2.5 days (similar to observations)

TropicalM. D. Eastin Wind Induced Surface Heat Exchange (WISHE): First proposed by Kerry Emanuel in 1986 Assumes the tropical atmosphere is not conditionally unstable, but rather near neutral to moist convection (i.e. the thermodynamic profile is moist adiabatic) Assumes the primary instability is the thermodynamic difference between ocean and the boundary layer air (i.e. sensible and latent heat fluxes are crucial) Genesis requires the presence of a finite amplitude disturbance (i.e. an easterly wave or MCV) Remaining question: How does the surface vortex form? Genesis via the WISHE Mechanism Kerry Emanuel

TropicalM. D. Eastin Genesis via the WISHE Mechanism a. Prior convective cycle creates a MCV. Continued stratiform rain leads to cooling and a mesoscale downdraft, which transports the mid-level vorticity and low-θ e air to the surface b. New surface cyclone envokes sensible and latent heat fluxes. Frictional driven inflow begins to warm and moisten, and develop new convection. c. Downdrafts disappear, convection regularly occurs in near neutral air, warm core gradually develops, further vortex intensification near the surface

TropicalM. D. Eastin Vortical Hot Towers (VHT): First proposed by Mike Montgomery in 2004 Assumes the atmosphere is conditionally unstable Assumes the preferred route to genesis is from multiple “merger events” between convective-scale cumulonimbus towers that possess intense cyclonic vorticity Genesis requires the presence of a finite amplitude disturbance (easterly wave or MCV) for a background vorticity source Remaining question: How does the surface vortex form? Genesis via the VHT Mechanism Mike Montgomery

TropicalM. D. Eastin Genesis via the VHT Mechanism a. Hot towers (buoyant updrafts) develop and feed off the conditional instability. Minimal low-level vorticity. b. Upward acceleration leads to vorticity stretching and low-level convergence (via angular momentum conservation) of background vorticity Considerable low-level vorticity

TropicalM. D. Eastin Genesis via the VHT Mechanism Observational Evidence: Tropical Storm Gustav (2002) Vertically sheared from the northeast Exposed low-level circulation Convection confined to the southwest Episodic convective bursts (hot towers) developed multiple low-level vortices that rotated around to the northeast Shear Vector Low-level vortices

TropicalM. D. Eastin Genesis via the VHT Mechanism z = 0.67 km Low-level vorticity maxima associated with two distinct hot towers are present Roughly 0.5 hrs later the maxima have merged into a single stronger low-level vorticity maximum The low-level vortex develops through multiple merger events.

TropicalM. D. Eastin TC Lifecycle and Intensity Changes Part I: Genesis Summary Necessary Large-Scale Conditions Pre-existing convection Significant planetary vorticity Favorable wind shear pattern Moist Mid-troposphere Warm ocean with deep mixed layer Conditionally unstable atmosphere Easterly Waves (origin, structure, importance) Mesoscale Convective Vortices (origin, structure, importance) Genesis Mechanisms CISK (assumptions, physical processes) WISHE (assumptions, physical processes) VHTs (assumptions, physical processes)

TropicalM. D. Eastin References Charney, J. G., and A. Eliassen, 1964: On the growth of the hurricane depression. J. Atmos. Sci., 21, Emanuel, K. A., 1986: An air-sea interaction theory for tropical cyclones. Part I: Steady-state maintenance., J. Atmos. Sci., 43, Gray, W. M., 1968: Global view of the origin of tropical disturbances and storms. Mon. Wea. Rev., 96, Hendricks, E. A., M. T, Montgomery, and C. A. Davis, 2004: On the role of “vortical” hot towers in formation of tropical cyclone Diana (1984), J. Atmos. Sci., 61, Montgomery, M. T., M. E. Nicholls, T. A. Cram, and A. B. Saunders, 2006: A vortical hot tower route to tropical cyclogenesis. J. Atmos. Sci., 63,