Numerical investigation of primary air-blast atomization and modal analysis of flow instabilities

Author(s):  
Jeremy O. McCaslin ◽  
Olivier Desjardins
2021 ◽  
Vol 774 (1) ◽  
pp. 012115
Author(s):  
K Yamamoto ◽  
M Roubaty ◽  
M Morisod ◽  
M Coulaud ◽  
S Houde

2003 ◽  
Vol 208 ◽  
pp. 385-386
Author(s):  
D. Chakrabarty ◽  
J. Murray ◽  
G.A. Wynn ◽  
A.R. King

In this article we report the results of our numerical investigation of warped accretion discs in binary stellar systems. We perform complete 3-D hydrodynamic simulations of binary discs. The disc is rendered unstable to the warp mode under the action of the magnetic field of the companion star in the binary. The disc thus warped is noted to undergo retrograde precession with a precession period just slightly less than the binary period. This small difference in periods can explain the phenomenon of negative superhumps observed in a number of binaries. Besides the modal analysis based on Fourier transforms, warps were also studied by a simple and robust technique that we developed; this is based on an analysis of the azimuthal distributions of particles that lie above and below the mid-plane of the disc.


2019 ◽  
Vol 130 ◽  
pp. 46-65 ◽  
Author(s):  
K. Christou ◽  
W.C. Radünz ◽  
B. Lashore ◽  
F.B.S. de Oliveira ◽  
J.L.M.A. Gomes

2019 ◽  
Vol 31 (7) ◽  
pp. 074105 ◽  
Author(s):  
Yuya Ohmichi ◽  
Kenji Kobayashi ◽  
Masahiro Kanazaki

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