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Stellar Fluid Dynamics and Numerical Simulations: From the Sun to Neutron Stars
M. Rieutord and B. Dubrulle (eds)
EAS Publications Series, 21 (2006) 197-218
DOI: 10.1051/eas:2006114
Subgrid-Scale modeling
L. ValdettaroDipartimento di Matematica, Politecnico di Milano, Italy
Abstract
The purpose of this lecture is to give an overview of
the subgrid scale models used for Large Eddy Simulations (LES).
The first models where essentially eddy-viscosity models,
where the turbulent viscosity coefficient was found
by simple dimensional considerations (the mixing length theory) or
taking into account Kolmogorov theory (the
Smagorinsky model).
Since then there have been many improvements, and now some of the
physical ingredients of turbulence, such as the local
backscatter and the anisotropy of small scale structures, can
be successfully taken into account.
Far from being a black box
tool to obtain answers to
turbulent flow problems, the Large Eddy Simulation technique
is still a work in progress with many odds and ends.
We give in this lecture an overview of the historical
development of turbulence models and we
point out the lights and shadows of them with
attention to the open problems that still remain to be solved.
© EAS, EDP Sciences 2006
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