Wu, C-C., and Y. Kurihara, 1996: A numerical study of the feedback
mechanisms of hurricane-environment interaction on hurricane movement from
the potential vorticity perspective. Journal of the Atmospheric
Sciences, 53(15), 2264-2282.
Abstract: The interaction between a hurricane and its environment
is studied by analyzing the generation and influence of potential vorticity
(PV) from the Geophysical Fluid Dynamics Laboratory hurricane model analysis
system. Two sets of numerical experiments are performed: one with and the
other without a bogused hurricane vortex in the initial time, for cases
of Hurricanes Bob (1991), Gilbert (1988), and Andrew (1992).
The PV budget analysis of Bob shows that the condensational heating within
the vortex redistributes the PV, causing a PV sink in the upper part of
the vortex and a PV source in the lower part. This tendency is compensated
for largely, but not entirely, by the upward transport of high-PV air from
the lower levels to the upper levels. The net effect contributes to the
increase of the negative upper-level PV anomaly during the vortex intensification
period. This result indicates that the diabatic heating effect plays a
crucial role in the evolution of the PV field in hurricanes. It also suggests
the importance of accurate representation of the heating profile in hurricane
models.
It is shown that the negative upper-level PV anomaly is spread out by the
upper-level outflow and the large-scale background flow. The impact of
the spread of the negative upper PV anomaly to the storm is quantitatively
evaluated by computing the nonlinear balanced flow associated with the
PV perturbation. Notable contribution to the steering of the storm from
the upper-level PV anomaly is found. The result supports the theory advanced
by Wu and Emanuel concerning the effect of the upper negative PV anomaly
on hurricane motion. This study also indicates the need of enhanced observation
and accurate analysis and prediction in the upper troposphere in order
to improve hurricane track forecasting.