HR: 08:52h
AN: A11G-04 [Abstracts]
TI: Inner Core Structures and Intensity Change Simulated With the Advanced Hurricane WRF Model
AU: * Corbosiero, K L
EM: kristen@atmos.ucla.edu
AF: UCLA, Department of Atmospheric and Oceanic Sciences
University of California, Los Angeles
7149 Math Sciences Building, Los Angeles, CA 90095, United States
AU: Wang, W
EM: weiwang@ucar.edu
AF: NCAR, Mesoscale and Microscale Meteorology Division
P.O. BOX 3000, Boulder, CO 80307, United States
AU: Done, J
EM: done@ucar.edu
AF: NCAR, Mesoscale and Microscale Meteorology Division
P.O. BOX 3000, Boulder, CO 80307, United States
AU: Chen, Y
EM: yochen@ucar.edu
AF: NCAR, Mesoscale and Microscale Meteorology Division
P.O. BOX 3000, Boulder, CO 80307, United States
AU: Dudhia, J
EM: dudhia@ucar.edu
AF: NCAR, Mesoscale and Microscale Meteorology Division
P.O. BOX 3000, Boulder, CO 80307, United States
AU: Davis, C
EM: cdavis@ucar.edu
AF: NCAR, Mesoscale and Microscale Meteorology Division
P.O. BOX 3000, Boulder, CO 80307, United States
AB:
The Advanced Hurricane WRF (AHW) has been used for real-time prediction and retrospective research
simulations of Atlantic basin tropical cyclones since 2003. Verification of the intensity and track errors of the AHW
forecasts has shown that 12 km and 4 km simulations perform as well as, and occasionally superior to, the
National Hurricane Center official forecasts and other operational forecast systems. Verification of the inner core
structure of the simulated storms, examined with a finest mesh of 1.33 km, has proven less successful. Realistic
eye, eyewall and inner spiral rainband structures are simulated, but the eye is generally too small and the
eyewall convection too wide. Outside of the eyewall, the azimuthal location of convective bands and asymmetries
in the wind field agree well with reconnaissance observations and concentric eyewall cycles are simulated on
realistic time and spatial scales. Closer to the core, the eyewall potential vorticity maximum provided steep
gradients on which copious vortex Rossby waves and mesovortices were noted to propagate in accord with
theory. The amplitude of these asymmetries and their dominant wavenumbers however, are inconsistent with
observations. Possible explanations for the high Rossby wave activity, the effects of these asymmetries on storm
intensity and sensitivity experiments undertaken to reduce the spurious wave activity will be the focus of this
presentation.
DE: 3314 Convective processes
DE: 3329 Mesoscale meteorology
DE: 3374 Tropical meteorology
SC: Atmospheric Sciences [A]
MN: 2007 Fall Meeting