Comments on “Flows with Radiant Energy Absorption and Thermonuclear Reactions behind the Shock Wave”

1972 ◽  
Vol 15 (10) ◽  
pp. 1866
Author(s):  
Jan Rosciszewski
Keyword(s):  
Shock Wave ◽  
Energy Absorption ◽  
Radiant Energy ◽  
Thermonuclear Reactions

scholarly journals NUMERICAL ASSESSMENT OF THE SELECTED SUPPORTING ELEMENT CARRYING CAPACITY OF CRITICAL INFRASTRUCTURE FACILITY / SZACOWANIE NUMERYCZNE NOŚNOŚCI WYBRANEGO ELEMENTU KONSTRUKCYJNEGO OBIEKTU INFRASTRUKTURY KRYTYCZNEJ

2013 ◽  
Vol 26 (1) ◽  
pp. 29-42 ◽  
Author(s):  
Jerzy Małachowski ◽  
Marian Klasztorny ◽  
Łukasz Mazurkiewicz ◽  
Damian Kołodziejczyk ◽  
Tadeusz Niezgoda
Keyword(s):  
Shock Wave ◽  
Modeling And Simulation ◽  
Energy Absorption ◽  
Carrying Capacity ◽  
Critical Infrastructure ◽  
Cylindrical Panel ◽  
Numerical Assessment ◽  
Wave Effects ◽  
Protective Cover ◽  
Supporting Element

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.

Theory of radiant-energy absorption by randomly dispersed discrete particles

1957 ◽  
Vol 9 (2) ◽  
pp. 148-156 ◽  
Author(s):  
John W. Otvos ◽  
Henry Stone ◽  
W.R. Harp
Keyword(s):  
Energy Absorption ◽  
Radiant Energy

NUCLEOSYNTHESIS IN SUPERNOVA SHOCK WAVES

1967 ◽  
Vol 45 (7) ◽  
pp. 2315-2332 ◽  
Author(s):  
J. W. Truran ◽  
W. D. Arnett ◽  
A. G. W. Cameron
Keyword(s):  
Shock Wave ◽  
Shock Waves ◽  
Neutron Flux ◽  
Neutron Capture ◽  
Alpha Particles ◽  
Extreme Conditions ◽  
Stellar Envelope ◽  
Capture Process ◽  
Thermonuclear Reactions ◽  
Supernova Explosions

It is generally assumed that element synthesis will take place readily under the extreme conditions believed to exist in supernova explosions. We have examined the types of thermonuclear reactions that can occur in a supernova shock wave which propagates through the stellar envelope, in which a temperature ~5 × 109 °K may occur for ~10−2 seconds. The calculations are performed using a network of nuclei connected to their neighbors by absorption or emission of neutrons, protons, alpha particles and photons (Truran et al. 1966). The results show that iron-peak elements can be produced by a supernova shock wave, but the iron-peak composition observed in nature is not produced unless some transformation of protons to neutrons has taken place in the material before the passage of the shock wave. Furthermore, a neutron flux sufficient to drive the rapid neutron-capture process is not attained under these conditions in the stellar envelope.

Shock Wave Energy Absorption in Metal–Organic Framework

2019 ◽  
Vol 141 (6) ◽  
pp. 2220-2223 ◽  
Author(s):  
Xuan Zhou ◽  
Yu-Run Miao ◽  
William L. Shaw ◽  
Kenneth S. Suslick ◽  
Dana D. Dlott
Keyword(s):  
Shock Wave ◽  
Energy Absorption ◽  
Wave Energy ◽  
Metal Organic Framework ◽  
Shock Wave Energy ◽  
Metal Organic ◽  
Organic Framework

RADIANT TRANSFER IN GAS FILLED ENCLOSURES BY RADIANT ENERGY ABSORPTION DISTRIBUTION METHOD

1986 ◽  
Author(s):  
Hiroshi Taniguchi ◽  
Wen-Jei Yang ◽  
Kazuhiko Kudo ◽  
Hiroshi Hayasaka ◽  
Masahito Oguma ◽  
...  
Keyword(s):  
Energy Absorption ◽  
Radiant Energy ◽  
Distribution Method ◽  
Radiant Transfer
Sign in / Sign up

Export Citation Format

Share Document