Data di Pubblicazione:
2011
Abstract:
The three-dimensional structure and evolution of
an isolated and stationary microburst are simulated using
a time-dependent, high resolution Large-Eddy-Simulation
(LES) model. The microburst is initiated by specifying a
simplified cooling source at the top of the domain around
2 km a.g.l. that leads to a strong downdraft. Surface winds
of the order of 30ms-1 were obtained over a region of
500m radius around the central point of the impinging downdraft,
with the simulated microburst lasting for a few minutes.
These characteristic length and time scales are consistent
with results obtained from numerical simulations of microbursts
using cloud-resolving models. The simulated flow
replicated some of the principal features of microbursts observed
by Doppler radars: in particular, the horizontal spread
of strong surface winds and a ring vortex at the leading
edge of the cold outflow. In addition to the primary surface
outflow, the simulation also generated a secondary surge of
strong winds that appears to represent a pulsation in the microburst
evolution.
These results highlight the capability of LES to reproduce
complex phenomena like microbursts, indicating the potential
usage of LES models to represent atmospheric phenomena
of time and space scales between the convective scale
and the microscale. These include short-lived convectivelygenerated
damaging winds.
Tipologia CRIS:
01.01 Articolo in rivista
Keywords:
Large-Eddy Simulation
Elenco autori:
Rizza, Umberto
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