An elliptical eye that rotated cyclonically with a period of approximately
144 minutes in Typhoon Herb 1996 was documented. The elliptical region had
a semimajor axis of 30 km and a semiminor axis of 20 km. Two complete perio
ds of approximately 144 min were observed in the Doppler radar data. The ro
tation of the elliptical eye in the context of barotropic dynamics at three
levels were explored: linear waves on a Rankin vortex, a nonlinear Kirchho
ff vortex, and with a nonlinear spectral model. The linear wave theory invo
lves the existence of both the high (potential) vorticity gradient near the
eye edge and the cyclonic mean tangential Bow in the typhoon. The propagat
ion of (potential) vorticity waves in the cyclonic mean flow makes the elli
ptical eye rotate cyclonically. The rotation period is longer than the peri
od of a parcel trajectory moving in the cyclonic mean flow around the circu
mference, because the vorticity wave propagates upwind. The nonlinear theor
y stems from the rotation of Kirchhoff's vortex. Estimates of the eye rotat
ion period from both linear and nonlinear theories agree with observations
of the eye rotation period when the observed maximum wind from Herb is used
. Nonlinear numerical computations suggest the importance of the interactio
n of neutral vorticity waves, which determine the shape and the rotation pe
riod of the eye. The calculations also support the rotation of the eye in a
pproximately 144 min in the presence of axisymmetrization, vorticity redist
ribution, wave breaking, and vortex merging processes.