Uniform shock waves driven by thermal radiation from laser-heated cavities

1996 ◽  
Author(s):  
Th. Löwer ◽  
R. Sigel
1984 ◽  
Vol 45 (2) ◽  
pp. 159-161 ◽  
Author(s):  
M. Kemmler ◽  
G. Wartmann ◽  
D. von der Linde

2016 ◽  
Vol 23 (5) ◽  
pp. 053107 ◽  
Author(s):  
S. Sai Shiva ◽  
Ch. Leela ◽  
P. Prem Kiran ◽  
C. D. Sijoy ◽  
S. Chaturvedi

2014 ◽  
Vol 141 (2) ◽  
pp. 024302 ◽  
Author(s):  
Klavs Hansen ◽  
Yejun Li ◽  
Vladimir Kaydashev ◽  
Ewald Janssens

2012 ◽  
Vol 79 (5) ◽  
pp. 457-465
Author(s):  
D. ONIĆ

AbstractThe shock waves are important features in the analysis of transonic magnetohydrodynamical (MHD) flows where thermal radiation could also be significant. In this paper the effects of black-body radiation on non-relativistic shock waves in an ideal radiation MHD model for the optically thick case are discussed. Distilled shock conditions were derived and discussed for the case of a fixed ratio of specific heats of an ideal gas (γ) and ratio of gas to total pressure (b). The special case, when jumps in γ and/or b are allowed, was also considered.


2005 ◽  
Vol 81 (4) ◽  
pp. 827-833 ◽  
Author(s):  
L. Landström ◽  
K. Elihn ◽  
M. Boman ◽  
C.G. Granqvist ◽  
P. Heszler

2006 ◽  
Vol 2 (S238) ◽  
pp. 395-396
Author(s):  
V. Kryvdyk ◽  
A. Agapitov

AbstractThe formation of the relativistic jets and a non-thermal emission from the collapsing magnetized stars with dipole magnetic fields and the heterogeneous particles distribution are investigated. These polar jets are formed when the stellar magnetosphere compress during collapse its magnetic field increases considerable. The electric field is produced in magnetosphere, which the charged particles will be accelerated. As follow from the calculation, the jets can be formed from collapsing stars already the explosion of supernova stars without shock waves. These jets will generate the non-thermal radiation. The radiation flux depends on the distance to the star, its magnetic field and the particle spectrum in the magnetosphere. This flux can be observed near Earth by means of modern telescopes in the form of the radiation pulse with duration equal to time collapse.


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