Results 31 to 40 of about 208,604 (196)
Since Sir Osborne Reynolds presented the Reynolds-averaged Navier–Stokes (RANS) equations in 1895, the construction of complete closure for RANS equations has been regarded as extremely challenging.
Sungmin Ryu
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A stability condition for turbulence model: From EMMS model to EMMS-based turbulence model
The closure problem of turbulence is still a challenging issue in turbulence modeling. In this work, a stability condition is used to close turbulence.
Li, Jinghai +3 more
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Average Turbulence Dynamics from a One-Parameter Kinetic Theory
We show theoretically that the mean turbulent dynamics can be described by a kinetic theory representation with a single free relaxation time that depends on space and time.
Hudong Chen +3 more
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Spherical model for turbulence [PDF]
A new set of models for homogeneous, isotropic turbulence is considered in which the Navier-Stokes equations for incompressible fluid flow are generalized to a set of N coupled equations in N velocity fields. It is argued that in order to be useful these models must embody a new group of symmetries, and a general formalism is laid out for their ...
, Mou, , Weichman
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Wind turbulence inputs for horizontal axis wind turbines [PDF]
Wind turbine response characteristics in the presence of atmospheric turbulence was predicted using two major modeling steps. First, the important atmospheric sources for the force excitations felt by the wind turbine system were identified and ...
Holley, W. E. +2 more
core +1 more source
Collisional transport across the magnetic field in drift-fluid models [PDF]
Drift ordered fluid models are widely applied in studies of low-frequency turbulence in the edge and scrape-off layer regions of magnetically confined plasmas.
A. H. Nielsen +5 more
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This paper describes a numerical simulation in the Amazon water system, aiming to develop a quasi-three-dimensional numerical tool for refined modeling of turbulent flow and passive transport of mass in natural waters.
Li-ren Yu
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Modelling supernova-driven turbulence [PDF]
High Mach number shocks are ubiquitous in interstellar turbulence. The Pencil Code is particularly well suited to the study of magnetohydrodynamics in weakly compressible turbulence and the numerical investigation of dynamos because of its high-order advection and time evolution algorithms.
Gent, F. A. +5 more
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CONFORMAL MODELS OF MAGNETOHYDRODYNAMIC TURBULENCE [PDF]
Following the previous work of Ferretti and Yang on the role of magnetic fields in the theory of conformal turbulence, we show that nonunitary minimal model solutions to two-dimensional magnetohydrodynamics (MHD) obtained by dimensional reduction from three dimensions exist under different (and more restrictive) conditions.
Coceal, Omduth, Thomas, Steven
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TURBULENCE MODELING FOR COMPUTATIONAL FLUID DYNAMICS, PART I: CONCEPTUAL OUTLOOK
The motivations like economics, and in house availability of powerful computers advocates the use of numerical methods as a complementary tool for experiments.
Murat Uygun +2 more
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