Damage Mechanisms in Polymers and Composites Under High-Velocity Liquid Impact

2009 ◽  
pp. 320-320-23 ◽  
Author(s):  
DA Gorham ◽  
MJ Matthewson ◽  
JE Field
2008 ◽  
Vol 59 (5) ◽  
pp. 499-502 ◽  
Author(s):  
Srinivasa R. Bakshi ◽  
Virendra Singh ◽  
D. Graham McCartney ◽  
Sudipta Seal ◽  
Arvind Agarwal

The type of stress pulse produced when a liquid mass strikes a solid at high velocity is first examined. Compressible behaviour, giving rise to a sharp peak of pressure, is found to occur in the initial stages of the impact. The duration of this peak depends on the dimensions and impact velocity of the liquid mass, and also on the compressible wave velocity for the liquid. A comparison is made with pulses produced by solid/solid impact and by the detonation of small quantities of explosive. Both the high-speed liquid impact and the explosive loading give intense pulses of duration only a few microseconds. A solid/solid impact has, by comparison, a much longer impact time of the order of hundreds of microseconds. The fracture of glasses and hard polymers using these three types of loading is described. The development of fracture is followed by high-speed photography. Differences in the modes of fracture are attributed to variations in the shape and duration of the applied stress pulses. Short circumferential fractures produced around the loaded area in liquid impact and explosive loading are shown to be initiated by the Rayleigh surface wave at points where flaws existed. More complex fracture patterns on the front surfaces of plates are due to the reinforcement of the surface wave with components of stress waves reflected from the back surface. A combination of impact loading and etching makes it possible to investigate the distribution and depths of flaws, their role in the fracture process, and the effect which etching has upon them. The observation on the deformation produced in solids by liquid impact has practical significance in the problem of supersonic aircraft flying through rain and in the erosion of turbine blades moving at high velocity through wet steam.


Wear ◽  
1977 ◽  
Vol 41 (2) ◽  
pp. 213-222 ◽  
Author(s):  
D.A. Gorham ◽  
J.E. Field

1980 ◽  
Vol 15 (6) ◽  
pp. 1518-1520 ◽  
Author(s):  
M. J. Matthewson ◽  
D. A. Gorham

2017 ◽  
Vol 109 ◽  
pp. 46-62 ◽  
Author(s):  
I. Mohagheghian ◽  
Y. Wang ◽  
J. Zhou ◽  
L. Yu ◽  
X. Guo ◽  
...  

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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