Shock wave effects in solar cosmic ray events

Solar Physics ◽  
1972 ◽  
Vol 27 (2) ◽  
pp. 466-477 ◽  
Author(s):  
I. D. Palmer
Keyword(s):  
Author(s):  
Kenneth S. Vecchio

Shock-induced reactions (or shock synthesis) have been studied since the 1960’s but are still poorly understood, partly due to the fact that the reaction kinetics are very fast making experimental analysis of the reaction difficult. Shock synthesis is closely related to combustion synthesis, and occurs in the same systems that undergo exothermic gasless combustion reactions. The thermite reaction (Fe2O3 + 2Al -> 2Fe + Al2O3) is prototypical of this class of reactions. The effects of shock-wave passage through porous (powder) materials are complex, because intense and non-uniform plastic deformation is coupled with the shock-wave effects. Thus, the particle interiors experience primarily the effects of shock waves, while the surfaces undergo intense plastic deformation which can often result in interfacial melting. Shock synthesis of compounds from powders is triggered by the extraordinarily high energy deposition rate at the surfaces of the powders, forcing them in close contact, activating them by introducing defects, and heating them close to or even above their melting temperatures.


2006 ◽  
Vol 134 ◽  
pp. 1065-1070
Author(s):  
E. Lach ◽  
M. Scharf
Keyword(s):  

Author(s):  
Charles Becht ◽  
Frederick J. Moody

The rupture of a pipe containing gas or steam at high pressure will cause a shock wave. In order to assess the potential damage that such a shock wave may cause to the surrounding structures, systems and components, it is necessary to determine the amplitude and propagation properties of the shock. A CFD model has been developed for the purpose of predicting shock propagation transients resulting from a sudden pipe rupture in terms of the fluid properties, pipe geometry, and surroundings. A simplified shock propagation model also is included, which offers verification of the CFD model results.


1991 ◽  
Vol 3 (7) ◽  
pp. 1792-1806 ◽  
Author(s):  
Douglas Rotman

2013 ◽  
Vol 26 (1) ◽  
pp. 29-42 ◽  
Author(s):  
Jerzy Małachowski ◽  
Marian Klasztorny ◽  
Łukasz Mazurkiewicz ◽  
Damian Kołodziejczyk ◽  
Tadeusz Niezgoda

Abstract Issues related to critical infrastructure safety is highly demanding in aspect of newly projected systems. In this paper a problem of modeling and simulation of the supporting structure behavior of critical facility (without or with proposed protective cover) loaded with a shock wave is presented. Authors assume that two different phenomena will be responsible for minimization of shock wave effects: flow around cylindrical panel and energy absorption by panel structure. In this paper research focuses on the description and analysis of the process of explosion near the supporting elements and the blast interaction with the structure.


Sadhana ◽  
1998 ◽  
Vol 23 (5-6) ◽  
pp. 579-596 ◽  
Author(s):  
B Sturtevant
Keyword(s):  

Author(s):  
Dimitra Lingri ◽  
Helen Mavromichalaki ◽  
Anatoly V. Belov ◽  
Eugenia A. Eroshenko

Many previous studies have shown that before the beginning of a Forbush Decrease (FD) of the cosmic ray intensity, a precursor signal can be observed. All these surveys were focused on FDs that are associated with a sudden storm com- mencement (SSC). In this work we demonstrate that precursors could also be observed in events without a SSC that is determined by an abrupt increase of the interplanetary magnetic field. The type of precursory signals and their diversity among the events are the main purpose of this study. We try to figure out similarities and differences on the signals and the associated events from both categories in the last fifty years, from 1969 to 2019, using the same selection criteria of the under investigation FDs. Simultaneously the orientation of the upcoming solar disturbances in comparison to the way they configure the increase of the interplanetary magnetic field and create these signals are discussed.


2019 ◽  
Vol 129 (3) ◽  
pp. 375-385 ◽  
Author(s):  
S. N. Taneev ◽  
S. A. Starodubtsev ◽  
V. G. Grigor’ev ◽  
E. G. Berezhko

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