Mitigation of exploding-wire-generated blast-waves by aqueous foam

2015 ◽  
Vol 27 (7) ◽  
pp. 076103 ◽  
Author(s):  
M. Liverts ◽  
O. Ram ◽  
O. Sadot ◽  
N. Apazidis ◽  
G. Ben-Dor
1998 ◽  
Author(s):  
P. Voinovich ◽  
E. Timofeev ◽  
K. Takayama ◽  
T. Saito ◽  
A. Galyukov

2020 ◽  
Vol 12 (4) ◽  
pp. 04032-1-04032-5
Author(s):  
V. V. Krivtsov ◽  
◽  
V. V. Kukla ◽  
V. V. Krivtsov ◽  
A. I. Shidlovskiy ◽  
...  

2016 ◽  
Vol 11 (1) ◽  
pp. 60-65 ◽  
Author(s):  
R.Kh. Bolotnova ◽  
E.F. Gainullina

The spherical explosion propagation process in aqueous foam with the initial water volume content α10=0.0083 corresponding to the experimental conditions is analyzed numerically. The solution method is based on the one-dimensional two-temperature spherically symmetric model for two-phase gas-liquid mixture. The numerical simulation is built by the shock capturing method and movable Lagrangian grids. The amplitude and the width of the initial pressure pulse are found from the amount of experimental explosive energy. The numerical modeling results are compared to the real experiment. It’s shown, that the foam compression in the shock wave leads to the significant decrease in velocity and in amplitude of the shock wave.


2021 ◽  
Vol 223 ◽  
pp. 110960
Author(s):  
Chi-Ming Chang ◽  
Ya-Chen Chiang ◽  
Ming-Hsiang Cheng ◽  
Shiuan-Huei Lin ◽  
Wen-Bin Jian ◽  
...  

Galaxies ◽  
2020 ◽  
Vol 8 (1) ◽  
pp. 10 ◽  
Author(s):  
Kris Davidson

Very massive stars occasionally expel material in colossal eruptions, driven by continuum radiation pressure rather than blast waves. Some of them rival supernovae in total radiative output, and the mass loss is crucial for subsequent evolution. Some are supernova impostors, including SN precursor outbursts, while others are true SN events shrouded by material that was ejected earlier. Luminous Blue Variable stars (LBV’s) are traditionally cited in relation with giant eruptions, though this connection is not well established. After four decades of research, the fundamental causes of giant eruptions and LBV events remain elusive. This review outlines the basic relevant physics, with a brief summary of essential observational facts. Reasons are described for the spectrum and emergent radiation temperature of an opaque outflow. Proposed mechanisms are noted for instabilities in the star’s photosphere, in its iron opacity peak zones, and in its central region. Various remarks and conjectures are mentioned, some of them relatively unfamiliar in the published literature.


2011 ◽  
Vol 7 (2) ◽  
pp. 71-76 ◽  
Author(s):  
R. Rodriguez ◽  
J.M. Gil ◽  
R. Florido ◽  
J.G. Rubiano ◽  
M.A. Mendoza ◽  
...  
Keyword(s):  

2012 ◽  
Vol 390 ◽  
pp. 012051
Author(s):  
Rashmita Das ◽  
Basanta Kumar Das ◽  
Rohit Shukla ◽  
Anurag Shyam
Keyword(s):  

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