detonation mechanism
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2020 ◽  
Vol 56 (6) ◽  
pp. 716-724
Author(s):  
I. A. Spirin ◽  
D. A. Pronin ◽  
E. S. Mitin ◽  
V. G. Simakov ◽  
V. A. Bragunets ◽  
...  

2018 ◽  
Vol 243 ◽  
pp. 00027
Author(s):  
Vitaly Komarov ◽  
Gennady Sakovich ◽  
Nikolai Popok ◽  
Maxim Kazutin ◽  
Nikolai Kozyrev

The detonation performance of melt-cast plastic-bonded explosives (PBXs) based on high melting explosive octogen (HMX) was studied in the paper. It has been found that the detonation velocity strongly depends from the dispersion distribution of HMX particles: it changes from 7800 to 8700 m/s. We explain this by the possibility of detonation propagation in PBX through different mechanisms, including detonation front propagation along a percolating cluster formed by filler particles. Thus, varying the particle size distribution can bring about one detonation mechanism or another and hence control the energy release dynamics of melt-cast PBXs to attain high efficiency in practice. Experimental results confirm the assumptions.


2015 ◽  
Vol 22 (10) ◽  
pp. 949-953 ◽  
Author(s):  
Chang-gen Shi ◽  
Yu Wang ◽  
Lin-sheng Zhao ◽  
Hong-bao Hou ◽  
Yu-heng Ge

2012 ◽  
Vol 759 (1) ◽  
pp. 53 ◽  
Author(s):  
G. C. Jordan ◽  
C. Graziani ◽  
R. T. Fisher ◽  
D. M. Townsley ◽  
C. Meakin ◽  
...  

2010 ◽  
Vol 19 (05) ◽  
pp. 523-538 ◽  
Author(s):  
J. E. HORVATH

We discuss the propagation of the hypothetical "combustion" n → SQM in a dense stellar environment. We address the instabilities affecting the flame and a present new results of application to the turbulent regime. The acceleration of the flame, the possible transition to the distributed regime and a further deflagration-to-detonation mechanism are addressed. As a general result, we conclude that the burning happens in (at least) either the turbulent Rayleigh–Taylor or the distributed regime, but not in the laminar regime. In both cases the velocity of the conversion of the star is several orders of magnitude larger than u lam , making the latter irrelevant in practice for this problem. A transition to a detonation is by no means excluded; actually, it seems to be favored by the physical setting, but a definitive answer would need a full numerical simulation.


2001 ◽  
Vol 09 (03) ◽  
pp. 1215-1225 ◽  
Author(s):  
MICHAEL J. BUCKINGHAM ◽  
MILTON A. GARCÉS

A recently developed theoretical model of the airborne acoustic field from an explosive volcanic eruption of the Strombolian type is described in this article. The magma column is assumed to be a circular cylinder, which is open to the atmosphere at the top, and which opens into a large magma chamber below. The magma itself is treated as a fluid, and the surrounding bedrock is taken to be rigid. An explosive source near the base of the magma column excites the natural resonances of the conduit. These resonances result in displacement of the magma surface, which acts as a piston radiating sound into the atmosphere. The source is modeled in much the same way as an underwater explosion from a high-explosive chemical such as TNT, although in the case of the volcano the detonation mechanism is the ex-solution of magmatic gases under extremely high hydrostatic pressure. The new theory shows compelling agreement with airborne acoustic signatures that were recorded in July 1994 at a distance of 150 m from the western vent of Stromboli volcano, Italy. The theoretical and observed power spectra both display the following features: (1) four energetic peaks below 20 Hz, identified as the first four longitudinal resonances of the magma column; (2) a broad minimum around 30 Hz, interpreted as a source-depth effect, occurring because the source lay close to nulls in the fifth and sixth longitudinal resonances and thus failed to excite these modes; and (3) radial resonance peaks between 35 and 65 Hz. On the basis of the theory, an inversion of the acoustic data from Stromboli yields estimates of the depth (≈100 m) and radius (≈16 m) of the magma column as well as the depth (≈83 m), spectral shape and peak shock wave pressure (≈1 GPa) of the explosive source. Most of the parameters estimated from the acoustic inversion compare favorably with the known geometry and source characteristics of Stromboli.


1992 ◽  
Vol 28 (6) ◽  
pp. 650-654 ◽  
Author(s):  
V. I. Nifad'ev ◽  
N. M. Kalinina

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