scholarly journals Steady State Modeling of Highly Rotating and Viscous Flow using VOF Method for Rotary Glass Fiberization Process

Author(s):  
Rohit Sharma ◽  
Vinay K. Gupta ◽  
Alok Khaware ◽  
Prem Andrade
Keyword(s):  
2012 ◽  
Vol 536 ◽  
pp. S109-S112
Author(s):  
E. Soinila ◽  
S. Bossuyt ◽  
H. Hänninen

2010 ◽  
Vol 2010 ◽  
pp. 1-12 ◽  
Author(s):  
Promise Mebine ◽  
Rhoda H. Gumus

This paper investigates steady-state solutions to MHD thermally radiating and reacting thermosolutal viscous flow through a channel with porous medium. The reaction is assumed to be strongly exothermic under generalized Arrhenius kinetics, neglecting the consumption of the material. Approximate solutions are constructed for the governing nonlinear boundary value problem using WKBJ approximations. The results, which are discussed with the aid of the dimensionless parameters entering the problem, are seen to depend sensitively on the parameters.


1967 ◽  
Vol 34 (4) ◽  
pp. 819-822 ◽  
Author(s):  
M. Friedman ◽  
J. Gillis

A study is made of the steady-state axisymmetric flow of a homogeneous viscous liquid in a straight circular pipe with absorbing walls. The complete equations are solved numerically and the streamlines and other features of the flow are computed. Comparison is made with earlier results obtained by various approximate methods.


1965 ◽  
Vol 21 (4) ◽  
pp. 623-633 ◽  
Author(s):  
Carl E. Pearson

The nature of the steady-state viscous flow between two large rotating disks has often been discussed, usually qualitatively, in the literature. Using a version of the numerical method described in the preceding paper (Pearson 1965), digital computer solutions for the time-dependent case are obtained (steady-state solutions are then obtainable as limiting cases for large times). Solutions are given for impulsively started disks, and for counter-rotating disks. Of interest is the fact that, at high Reynolds numbers, the solution for the latter problem is unsymmetrical; moreover, the main body of the fluid rotates at a higher angular velocity than that of either disk.


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