Weak Turbulence in Small Prandtl Number Convection in Porous Media
The dynamics of weak turbulence in small Prandtl number convection in porous media is substantially distinct than the corresponding dynamics for moderate and large Prandtl numbers.
Peter Vadasz
core +1 more source
Double-Diffusive Convection at Low Prandtl Number
This work reviews present knowledge of double-diffusive convection at low Prandtl number obtained using direct numerical simulations, in both the fingering regime and the oscillatory regime. Particular emphasis is given to modeling the induced turbulent
Pascale Garaud
core +1 more source
On the Onsetof Thermal Instability in a Low Prandtl Number Nanofluid Layer in a Porous Medium
Thermal instability in a low Prandtl number nanofluid in a porous medium is investigated by using Galerkin weighted residuals method for free-free boundaries. For porous medium, Brinkman-Darcy modelis applied.
Ramesh Chand, G. C. Rana
doaj
Numerical Simulation of Turbulent Channel Flow at Low Prandtl Number [PDF]
Liquid metals are primary coolants in Generation IV nuclear reactors. For low Prandtl\ud fluids, such as liquid metals, classical Reynolds analogy of using turbulent Prandtl number\ud close to unity doesnt predict heat transfer characteristics ...
K, Vasudeva Rao
core
Thermal field reconstruction and compressive sensing using proper orthogonal decomposition
Model order reduction allows critical information about sensor placement and experiment design to be distilled from raw fluid mechanics simulation data.
John Matulis, Hitesh Bindra
doaj +1 more source
Statistics of Heat Transfer in Two-Dimensional Turbulent Rayleigh-Bénard Convection at Various Prandtl Number. [PDF]
Yang H, Wei Y, Zhu Z, Dou H, Qian Y.
europepmc +1 more source
Laminar Natural Convection of Newtonian and Non Newtonian Fluids Inside Triangular Enclosure
In the present work, steady two dimensional laminar natural convection heat transfer of Newtonian and non-Newtonian fluids inside isosceles triangular enclosure has been analyzed numerically for a wide range of the modified Rayleigh numbers of (103 ...
Ala?a Abbas Muhadi
doaj +2 more sources
Asymptotic Behaviour of Galactic Small-scale Dynamos at Modest Magnetic Prandtl Number
Magnetic fields are critical at many scales to galactic dynamics and structure, including multiphase pressure balance, dust processing, and star formation. Dynamo action determines their dynamical structure and strength.
Frederick A. Gent +4 more
doaj +1 more source
Riga - Plate flow of γ Al2O3-water/ethylene glycol with effective Prandtl number impacts. [PDF]
Ganesh NV +3 more
europepmc +1 more source
Enhanced enstrophy generation for turbulent convection in low-Prandtl-number fluids. [PDF]
Schumacher J, Götzfried P, Scheel JD.
europepmc +1 more source

