scholarly journals Defense Model of Intercepting a High-Velocity Long Rod by Multiple Linear Shaped Charges

2021 ◽  
Vol 1855 (1) ◽  
pp. 012039
Author(s):  
Yishu Li ◽  
Hequan Cao ◽  
Likun Yang ◽  
Chao Qin
Keyword(s):  
Long Rod ◽  
2014 ◽  
Vol 5 (1) ◽  
pp. 47-63 ◽  
Author(s):  
Ali Alavi Nia ◽  
Mojtaba Zolfaghari ◽  
Hossein Khodarahmi ◽  
Mahmoud Nili ◽  
Amir Hossein Gorbankhani
Keyword(s):  

2000 ◽  
Vol 10 (PR9) ◽  
pp. Pr9-589-Pr9-594 ◽  
Author(s):  
F. Malaise ◽  
F. Collombet ◽  
J. Y. Tranchet

2015 ◽  
Vol 2015 ◽  
pp. 1-15 ◽  
Author(s):  
Yunhou Sun ◽  
Cuncheng Shi ◽  
Zheng Liu ◽  
Desheng Wen

With the hypervelocity kinetic weapon and hypersonic cruise missiles research projects being carried out, the damage mechanism for high-velocity/hypervelocity projectile impact on semi-infinite targets has become the research keystone in impact dynamics. Theoretical research progress in high-velocity/hypervelocity impact on semi-infinite targets was reviewed in this paper. The evaluation methods for critical velocity of high-velocity and hypervelocity impact were summarized. The crater shape, crater scaling laws and empirical formulae, and simplified analysis models of crater parameters for spherical projectiles impact on semi-infinite targets were reviewed, so were the long rod penetration state differentiation, penetration depth calculation models for the semifluid, and deformed long rod projectiles. Finally, some research proposals were given for further study.


1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


1967 ◽  
Vol 31 ◽  
pp. 117-119
Author(s):  
F. D. Kahn ◽  
L. Woltjer

The efficiency of the transfer of energy from supernovae into interstellar cloud motions is investigated. A lower limit of about 0·002 is obtained, but values near 0·01 are more likely. Taking all uncertainties in the theory and observations into account, the energy per supernova, in the form of relativistic particles or high-velocity matter, needed to maintain the random motions in the interstellar gas is estimated as 1051·4±1ergs.


1914 ◽  
Vol 111 (5) ◽  
pp. 82-82
Author(s):  
Frank C. Perkins
Keyword(s):  

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