EFFECT OF RADIATION ON THE FLOW STRUCTURE AND HEAT TRANSFER IN A TWO - DIMENSIONAL GRAY MEDIUM

Isocontours of temperature in the pipe for simulations with different operating pressures and having all a CO 2 inlet velocity of 1 m/s: the thin solid lines represent fields

(1997) studied numerically the fluid flow and heat transfer induced by natural convection in a finite horizontal channel containing an indefinite number of uniformly spaced

This investigation deals with the effects of slip, magnetic field and non-Newtonian flow parameters on flow and heat transfer of an incompressible, electrically conduct- ing

In this note, one will mainly focus on the combined effects of velocity slip and porosity on the von Kármán swirling flow and heat transfer of a viscous fluid for a rough

We recall that the boundary conditions imposed at z ∗ = 0 correspond to the laminar regime with a linear Taylor-Couette profile for V θ ∗ and a parabolic Poiseuille profile for V z

The temperature pro- The heat transfer from thermal plasmas to file in the entrance of the canal is assumed to be reactor walls is of major importance for the design parabolic,

When the radiative flux within a turbulent gaseous medium is of the same order of magnitude or higher than the averaged turbulent convective flux, or the wall conductive flux,

Patterson MC, Eugen M, Wijburg FA, Audrey M, Barbara S, Harir D, Vanier MT, Mercé P: Disease and patient characteristics in NP-C patients: findings from an international