Fully developed turbulence in accretion discs of binary stars: turbulent viscosity coefficient and power spectrum.

Author(s):  
A. M. Fridman ◽  
D. V. Bisikalo ◽  
A. A. Boyarchuk ◽  
L. Pustil’nik ◽  
Y. M. Torgashin
Fractals ◽  
1993 ◽  
Vol 01 (04) ◽  
pp. 1080-1085 ◽  
Author(s):  
Y.-H. TAGUCHI

The flow patterns in the vibrated bed of powder are investigated numerically in two dimensions. They turn out to exhibit turbulent flow like that observed in fully developed turbulence. The power spectrum of their flow lines has k−5/3 power, where k is the wave number. Since the numerical investigation of powder requires very few computational resources, it provides us with a new tool to study turbulence easily.


1996 ◽  
Vol 6 (4) ◽  
pp. 573-583 ◽  
Author(s):  
F. Belin ◽  
J. Maurer ◽  
P. Tabeling ◽  
H. Willaime

1995 ◽  
Vol 5 (7) ◽  
pp. 895-899 ◽  
Author(s):  
B. Castaing ◽  
B. Dubrulle

2020 ◽  
Vol 5 (4) ◽  
Author(s):  
Jason R. Picardo ◽  
Akshay Bhatnagar ◽  
Samriddhi Sankar Ray

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