Results 131 to 140 of about 9,963,654 (229)

Weak Turbulence in Small Prandtl Number Convection in Porous Media

open access: yes, 2010
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

On the Onsetof Thermal Instability in a Low Prandtl Number Nanofluid Layer in a Porous Medium

open access: yesJournal of Applied Fluid Mechanics, 2015
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  

Plots of concentration profile ϕ(ζ) for Prandtl number Pr.

open access: yes, 2017
Plots of concentration profile ϕ(ζ) for Prandtl number Pr.
Ahmed Alsaedi (479392)   +3 more
core   +1 more source

Profiles of θ for various values of Prandtl number Pr.

open access: yes, 2018
Profiles of θ for various values of Prandtl number Pr.
Ammar Mushtaq (633827)   +3 more
core   +1 more source

Laminar Natural Convection in a Square Cavity with a Horizontal Fin on the Heated Wall: A Numerical Study of Fin Position and Thermal Conductivity Effects

open access: yesEnergies
This study numerically examines laminar natural convection within a square cavity that has a horizontally attached adiabatic fin on its heated vertical wall.
Saleh A. Bawazeer
doaj   +1 more source

Laminar Natural Convection of Newtonian and Non – Newtonian Fluids Inside Triangular Enclosure

open access: yesAl-Khawarizmi Engineering Journal, 2007
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

open access: yesThe Astrophysical Journal Letters
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

A Phenomenological Interpretation of Laminar Natural Convection Correlations

open access: yesApplied Sciences
Natural convection heat transfer is commonly described using dimensionless correlations relating the Nusselt number to the Grashof and Prandtl numbers. For gases and non-metallic liquids, these parameters combine into the Rayleigh number, Ra=Gr·Pr, while
Massimo Corcione   +2 more
doaj   +1 more source

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