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Typhoon Dynamics. Roger K. Smith University of Munich. Aim To review some of the fundamental processes involved in the dynamics and thermodynamics of typhoon structure and evolution. Outline of talk. Structure of a mature hurricane Basic dynamics Primary circulation The eye
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Typhoon Dynamics Roger K. Smith University of Munich Aim To review some of the fundamental processes involved in the dynamics and thermodynamics of typhoon structure and evolution.
Outline of talk • Structure of a mature hurricane • Basic dynamics • Primary circulation • The eye • Effects of friction & the secondary circulation • Hurricane intensification • Buoyancy in a hurricane • Maintenance of the warm core • Summary/omissions
Schematic cross-section of a mature tropical cyclone Warm core in approximate thermal- wind balance Eyewall clouds: are they buoyant?
Structure of a mature hurricane isotachs isotherms Warm core Houze Fig. 10.11 From Wallace and Hobbs, (1977)
Primary (tangential) circulation z v(r,z,t) ~ 500 m Friction layer r
Approximate force balance above the friction layer Rotation axis Lowest pressure on the axis Primary (tangential) circulation Radial pressure gradient force Vertical pressure gradient force r Centrifugal force and Coriolis force v Gravitational force Gradient wind balance Hydrostatic balance
Thermal wind equation Gradient wind balance Hydrostatic balance Write Eliminate p using Thermal wind equation
Physical interpretation Thermal wind equation Balance in toroidal circulation tendency z light heavy z z light heavy r r r
Mathematical solution Characteristics z z(r) r Governs the variation of ρ along characteristics
Characteristics are isobaric surfaces z p = constant po ,ro z(r) r Along a characteristic
Inferences p = constant z po ,ro z(r) r Barotropic vortex Baroclinic vortex Equation of state
Summary • A barotropic vortex is cold cored if temperature contrasts are measured at constant height. • A baroclinic vortex is warm cored if temperature contrasts are measured at constant height and if-∂v/∂zis large enough. A sample calculation =>
Eye dynamics z Gradient wind balance warm cool v(r,z) r
Summary • The decline in the tangential wind speed with height at all radii there is a reduced upward force acting on air parcels compared with that at large radii (perturbation pressure gradient is downwards). • The air density is less also and there is approximate balance. • Exactly thermal wind balance there is no net upward force to drive vertical motion – presumably the case in a mature hurricane. • The subsidence near the axis of a hurricane occurs mainly during the intensification stage. • As the tangential circulation intensifies, the density of an air parcel in the eye must be slightly larger than it would be in the exactly balanced state the air slowly subsides. • When the tangential circulation weakens, the density is slightly less than in the exactly balanced state the air slowly rises.
Hurricane intensification • Basic principle - Conservation of absolute angular momentum: M = rv + r2f/2 r v v = M/r - rf/2 If r decreases, v increases! Spin up requires radial convergence
Frictionally-induced secondary circulation Secondary circulation Pressure gradient force r v v Centrifugal force and Coriolis force are reduced by friction
Dynamics of vortex spin down Vertikal cross-section v Friction layer Level of nondivergence
Vertical velocity at the top of the friction layer Another reason to expect the existence of an eye!
Buoyancy in a hurricane buoyancy warm Tv Tv Friction layer Level of nondivergence Buoyancyhorizontal gradient of (virtual) Temperature
Maintenance of the warm core in a tropical cyclone qe1 qe2 eye v qeb1 qeb2 Moisture flux |Vs|(q*(Ts,p) – qb)
Summary • Structure of a mature hurricane • Basic dynamics • Primary circulation • The eye • Effects of friction & the secondary circulation • Hurricane intensification • Buoyancy in a hurricane • Maintenance of the warm core (WISHE mechanism) • Omissions: hurricane motion, asymmetric processes, eye-wall replacement cycles