Development of Advanced Thermoplastic Composite Projectiles for High-Velocity Shots With the PEGASUS Railgun

2011 ◽  
Vol 39 (12) ◽  
pp. 3391-3395 ◽  
Author(s):  
C. Avril ◽  
D. Perreux ◽  
F. Thiebaud ◽  
B. Reck ◽  
S. Hundertmark
Author(s):  
R Keck ◽  
W Machunze ◽  
W Dudenhausen ◽  
P Middendorf

Regarding aircrafts, the application of composites within impact endangered areas is unusual. Therefore, an advanced thermoplastic composite slat had been developed with the aim of minimizing weight and manufacturing costs in scheduled series production. The investigation of many manufacturing techniques had been performed as well as integration of new materials. Several generic and full-scale thermoplastic demonstrators were manufactured, using endless fibre-reinforced carbon-fibre-reinforced polyetheretherketone tapes. The critical point, concerning the casting of thick and highly tapered, single curved thermoplastic shells, was identified and new manufacturing methods had been developed. Additionally, the thermoplastic welding process was improved, resulting in a low-cost assembly technique as an alternative to state-of-the-art joining methods. In addition to conventional linear static analysis, dynamic high-velocity impact simulations were carried out. A numerical approach for high-velocity bird strike impact had been developed. The results were used to dimension the residual strength of a damaged slat. Furthermore, a good compliance between the dynamic analysis and the performed tests has been reached. It has been shown that a significant weight reduction is possible by numerical optimization, even if composites are used for impact-sensitive areas.


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):  

1994 ◽  
Vol 4 (4) ◽  
pp. 451-471 ◽  
Author(s):  
Nobuyuki Yatsuyanagi ◽  
Hiroshi Sakamoto ◽  
Kazuo Sato

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