On Large-Scale Vortical Structures in (Incompressible) Fluids with Thermal Expansion

1997 ◽  
Vol 07 (01) ◽  
pp. 113-123 ◽  
Author(s):  
Y. A. Berezin ◽  
K. Hutter

This paper extends the analysis of Ref. 1 to non-Boussinesq fluids whose thermal equation of state depends negligibly on pressure but non-negligibly on temperature. It is demonstrated that these fluids are more stable than the Boussinesq fluids under the same conditions. We study the effect of the helicity on the stability of the Bénard problem and demonstrate that there is no separatrix that divides the instability regimes into two classes. Here, the phenomenon of inverse energy cascade is present at all values of helicities.

2005 ◽  
Vol 66 (5) ◽  
pp. 706-710 ◽  
Author(s):  
G.A. Voronin ◽  
C. Pantea ◽  
T.W. Zerda ◽  
L. Wang ◽  
Y. Zhao

2007 ◽  
Vol 164 (3-4) ◽  
pp. 142-160 ◽  
Author(s):  
Konstantin D. Litasov ◽  
Eiji Ohtani ◽  
Sujoy Ghosh ◽  
Yu Nishihara ◽  
Akio Suzuki ◽  
...  

2019 ◽  
Vol 46 (20) ◽  
pp. 11018-11024 ◽  
Author(s):  
Xiaojun Hu ◽  
Yingwei Fei ◽  
Jing Yang ◽  
Yang Cai ◽  
Shijia Ye ◽  
...  

1993 ◽  
Vol 157 ◽  
pp. 255-261
Author(s):  
N. Kleeorin ◽  
I. Rogachevskii

The nonlinear (in terms of the large-scale magnetic field) effect of the modification of the magnetic force by an advanced small-scale magnetohydrodynamic (MHD) turbulence is considered. The phenomenon is due to the generation of magnetic fluctuations at the expense of hydrodynamic pulsations. It results in a decrease of the elasticity of the large-scale magnetic field.The renormalization group (RNG) method was employed for the investigation of the MHD turbulence at the large magnetic Reynolds number. It was found that the level of the magnetic fluctuations can exceed that obtained from the equipartition assumption due to the inverse energy cascade in advanced MHD turbulence.This effect can excite an instability of the large-scale magnetic field due to the energy transfer from the small-scale turbulent pulsations. This instability is an example of the inverse energy cascade in advanced MHD turbulence. It may act as a mechanism for the large-scale magnetic ropes formation in the solar convective zone and spiral galaxies.


2008 ◽  
Vol 15 (3) ◽  
pp. 359-368 ◽  
Author(s):  
A. B. Kaplun ◽  
B. I. Kidyarov ◽  
A. B. Meshalkin ◽  
A. V. Shishkin

2003 ◽  
Vol 88 (1) ◽  
pp. 80-86 ◽  
Author(s):  
Yu Nishihara ◽  
Eiichi Takahashi ◽  
Kyoko Matsukage ◽  
Takumi Kikegawa

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