Steady shock profile in solids

1973 ◽  
Vol 44 (9) ◽  
pp. 4013-4016 ◽  
Author(s):  
F. E. Prieto ◽  
C. Renero
Keyword(s):  
1969 ◽  
Vol 40 (9) ◽  
pp. 3771-3775 ◽  
Author(s):  
George E. Duvall ◽  
R. Manvi ◽  
Sherman C. Lowell

Author(s):  
Giuliano D'Ammando ◽  
Daniela Pietanza ◽  
Gianpiero Colonna ◽  
Savino Longo ◽  
Mario Capitelli

1983 ◽  
Vol 100 ◽  
pp. 145-146
Author(s):  
A. H. Nelson ◽  
T. Matsuda ◽  
T. Johns

Numerical calculations of spiral shocks in the gas discs of galaxies (1,2,3) usually assume that the disc is flat, i.e. the gas motion is purely horizontal. However there is abundant evidence that the discs of galaxies are warped and corrugated (4,5,6) and it is therefore of interest to consider the effect of the consequent vertical motion on the structure of spiral shocks. If one uses the tightly wound spiral approximation to calculate the gas flow in a vertical cut around a circular orbit (i.e the ⊝ -z plane, see Nelson & Matsuda (7) for details), then for a gas disc with Gaussian density profile in the z-direction and initially zero vertical velocity a doubly periodic spiral potential modulation produces the steady shock structure shown in Fig. 1. The shock structure is independent of z, and only a very small vertical motion appears with anti-symmetry about the mid-plane.


2017 ◽  
Vol 107 ◽  
pp. 204-228 ◽  
Author(s):  
Christophe Czarnota ◽  
Alain Molinari ◽  
Sébastien Mercier

2002 ◽  
Vol 92 (10) ◽  
pp. 5886-5891 ◽  
Author(s):  
H. Marom ◽  
D. Sherman ◽  
Z. Rosenberg ◽  
N. Murray
Keyword(s):  

2020 ◽  
Vol 135 ◽  
pp. 102816
Author(s):  
Christophe Czarnota ◽  
Alain Molinari ◽  
Sébastien Mercier

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