Numerical study of the transition from regular to mach reflection in steady supersonic flows

Author(s):  
M. S. Ivanov ◽  
S. F. Gimelshein ◽  
A. N. Kudryavtsev ◽  
G. N. Markelov
1998 ◽  
Author(s):  
J.-H. Kim ◽  
Y. Yoon ◽  
J.-Y. Choi ◽  
I.-S. Jeung

Author(s):  
Valentin Bityurin ◽  
Alexei Bocharov ◽  
E. Filimonova ◽  
A. Klimov

Shock Waves ◽  
2005 ◽  
Vol 14 (4) ◽  
pp. 307-311 ◽  
Author(s):  
T. I. Tseng ◽  
R. J. Yang

1994 ◽  
Vol 263 ◽  
pp. 293-318 ◽  
Author(s):  
Hideshi Hanazaki

A numerical study of the three-dimensional internal waves excited by topography in the flow of a stratified fluid is described. In the resonant flow of a nearly two-layer fluid, it is found that the time-development of the nonlinearly excited waves agrees qualitatively with the solution of the forced KP equation or the forced extended KP equation. In this case, the upstream-advancing solitary waves become asymptotically straight crested because of abnormal reflection at the sidewall similar to Mach reflection. The same phenomenon also occurs in the subcritical flow of a nearly two-layer fluid. However, in the subcritical flow of a linearly stratified Boussinesq fluid, the two-dimensionalization of the upstream waves can be interpreted as the separation of the lateral modes due to the differences in the group velocity of the linear wave, although this does not mean in general that the generation of upstream waves is describable by the linearized equation.


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.


1995 ◽  
pp. 191-196
Author(s):  
A. Sasoh ◽  
K. Takayama ◽  
T. Saito

2021 ◽  
Vol 104 (5) ◽  
Author(s):  
Rohtash Goyal ◽  
A. Sameen ◽  
T. Jayachandran ◽  
G. Rajesh

1999 ◽  
Vol 386 ◽  
pp. 213-232 ◽  
Author(s):  
G. BEN-DOR ◽  
T. ELPERIN ◽  
H. LI ◽  
E. VASILIEV

The effect of the downstream pressure (defined here as the wake pressure behind the tail of the reflecting wedge) on shock wave reflection in steady flows is investigated both numerically and analytically. The dependence of the shock wave configurations on the downstream pressure is studied. In addition to the incident-shock-wave-angle-induced hysteresis, which was discovered a few years ago, a new downstream- pressure-induced hysteresis has been found to exist. The numerical study reveals that when the downstream pressure is sufficiently high, an inverse-Mach reflection wave configuration, which has so far been observed only in unsteady flows, can be also established in steady flows. Very good agreement between the analytical predictions and the numerical results is found.


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