Observed Inner-Core Structural Variability in Hurricane Dolly Yu-Fen Huang Hendricks E. A., B. d. Mcnoldy, and Wayne H. Schubert.

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Presentation transcript:

Observed Inner-Core Structural Variability in Hurricane Dolly Yu-Fen Huang Hendricks E. A., B. d. Mcnoldy, and Wayne H. Schubert

Introduction TC intensity change is caused by environmental, oceanic, and internal dynamical factors. (Wang and Wu 2004). An important internal process is the dynamic instability.

On aircraft reconnaissance missions, airborne radar data have shown that significant variability in the eyewall region. (Marks et al. 1992; Reasor et al. 2000; Roux and Viltard 2004)

The observations of the inner core of Dolly were taken from the National Weather Service Weather Surveillance Radar-1988 Doppler (WSR-88D) in Brownsville, Texas, prior to landfall.

The dynamic eyewall with significant azimuthal variability on short times scales (30 min to 1 h) during a 6-h rapid intensification and deepening period before it made landfall.

Synoptic history Dolly’s origin can be traced to a tropical wave exiting Africa on 11 July July 2008 formed into a tropical storm, when it was in the western Caribbean Sea.

slow down Yucatan peninsula kt

The National Hurricane Center (NHC) best-track intensity estimates are shown significant eyewall asymmetries Rapid intensify

Environmental analysis 1.SHRD: magnitude of the deep-layer hPa sheer vector averaged from r=200 to 800 km 2.RSST: Reynolds analysis sea surface temperature (Reynolds and Smith 1993) 3.D200: 200hPa divergence averaged from r=0 to 1000 km 4.RHMD: hPa relative humidity averaged from r = 200 to 800 km

When Dolly was rapidly intensifying and deepening, the environmental condition were generally becoming less favorable. The rapid intensification and deepening event may have been more strongly controlled by the vortex internal dynamics than the environmental condition for this case.

Inner-core analysis

This demonstrates that the asymmetries in the eyewall are primarily confined to lower levels during the instability. No upshear tilt of the asymmetries in the vertical, which would signify that a baroclinic instability is occurring.

Flight level: 700 hPa

NESW

NW SE

NS

Numerical Simulation Shallow-water model. Base on vorticity-divergence

Double Fourier pseudospectral discretization. 600 km * 600 km → 512 * 512 points. Dealiasing → 170 Fourier modes → resolution is 3.52 km. The numerical diffusion coefficient was set to 25 m 2 /s Time differencing was using a third-order explicit scheme with a time step of 4 s.

Initial condition A thin voricity ring was constructed in accordance with the flight-level vorticity of leg 1 from r = 0 to 30 km. eye eyewall

Barotropic instability of a vortex with Dolly’s observed radial vorticity profile can produce the high azimuthal wavenumber asymmetric variability of similar structure and on similar time scales that were observed.

Summery The most likely cause of the high-wavenumber asymmetries is a convectively modified form of dynamic instability of a thin potential vorticity ring. The asymmetric mixing of high PV air from the eyewall into the eye The internal vortex dynamics were dominant contributors to the rapid intensification and deepening.

Thanks for your listening!

Rankine vortex