Studying Hydrodynamic Instability Using Shock-Tube Experiments

被引：0
作者：
O. Sadot
K. Levy
A. Yosef-Hai
D. Cartoon
Y. Elbaz
Y. Srebro
G. Ben-Dor
D. Shvarts
机构：
[1] BEER-SHEVA,Physics Department, Nuclear Research Center Negev
[2] Ben-Gurion University of the Negev,undefined
[3] BEER-SHEVA,undefined
来源：
Astrophysics and Space Science | 2005年 / 298卷
关键词：
Richtmyer-Meshkov instability; turbulent mixing; shock-tube experiments;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
The hydrodynamic instability, which develops on the contact surface between two fluids, has great importance in astrophysical phenomena such as the inhomogeneous density distribution following a supernova event. In this event acceleration waves pass across a material interface and initiate and enhance unstable conditions in which small perturbations grow dramatically.
引用
收藏
页码：305 / 312
页数：7
相关论文
共 64 条
  • [1] Aleshin A.N.(1990)undefined Sov. Phys. Dokl. 35 159-undefined
  • [2] Lazareva E.V.(1995)undefined Phys. Rev. Lett. 74 534-undefined
  • [3] Zaitsev S.G(1996)undefined Phys. Plasmas 3 614-undefined
  • [4] Rozanov V.B.(2000)undefined Shock Waves J. 4 241-undefined
  • [5] Gamali E.G.(1994)undefined Phys. Fluids 6 4019-undefined
  • [6] Lebo I.G.(1999)undefined J. Fluid Mech. 389 55-undefined
  • [7] Alon U.(1995)undefined Phys. Plasmas 2 3933-undefined
  • [8] Hecht J.(2004)undefined L&PB 21 335-undefined
  • [9] Ofer D.(1969)undefined Fluid Dyn. 4 101-undefined
  • [10] Shvarts D.(1972)undefined Phys. Fluids 15 753-undefined
1234567