Numerical Study of Plasma Assisted Mixing and Combustion in Non-Premixed Supersonic Flows

Author(s):  
Valentin Bityurin ◽  
Alexei Bocharov ◽  
E. Filimonova ◽  
A. Klimov
1998 ◽  
Author(s):  
J.-H. Kim ◽  
Y. Yoon ◽  
J.-Y. Choi ◽  
I.-S. Jeung

2010 ◽  
Vol 6 (S274) ◽  
pp. 373-375
Author(s):  
Fabio Del Sordo ◽  
Axel Brandenburg

AbstractA spherical hydrodynamical expansion flow can be described as the gradient of a potential. In that case no vorticity should be produced, but several additional mechanisms can drive its production. Here we analyze the effects of baroclinicity, rotation and shear in the case of a viscous fluid. Those flows resemble what happens in the interstellar medium. In fact in this astrophysical environment supernovae explosion are the dominant flows and, in a first approximation, they can be seen as spherical. One of the main difference is that in our numerical study we examine only weakly supersonic flows, while supernovae explosions are strongly supersonic.


2014 ◽  
Vol 21 (7) ◽  
pp. 072510 ◽  
Author(s):  
Rajiv Goswami ◽  
Jean-François Artaud ◽  
Frédéric Imbeaux ◽  
Predhiman Kaw

1989 ◽  
Vol 29 (11) ◽  
pp. 911-918 ◽  
Author(s):  
Natsuo Hatta ◽  
Hitoshi Fujimoto ◽  
Ryuji Ishii ◽  
Yoshikuni Umeda ◽  
Jun-ichi Kokado

1994 ◽  
Vol 144 ◽  
pp. 185-187
Author(s):  
S. Orlando ◽  
G. Peres ◽  
S. Serio

AbstractWe have developed a detailed siphon flow model for coronal loops. We find scaling laws relating the characteristic parameters of the loop, explore systematically the space of solutions and show that supersonic flows are impossible for realistic values of heat flux at the base of the upflowing leg.


1998 ◽  
Vol 77 (2) ◽  
pp. 473-484 ◽  
Author(s):  
M. Sampoli, P. Benassi, R. Dell'Anna,

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