von Karman Correlation Similarity of the Turbulent Interplanetary Magnetic Field

2021 ◽  
Vol 919 (2) ◽  
pp. L27
Author(s):  
Sohom Roy ◽  
R. Chhiber ◽  
S. Dasso ◽  
M. E. Ruiz ◽  
W. H. Matthaeus
2016 ◽  
Vol 47 (5) ◽  
pp. 471-488
Author(s):  
Lyes Bordja ◽  
Emilia Crespo del Arco ◽  
Eric Serre ◽  
Rachid Bessaih

2012 ◽  
Vol 693 ◽  
pp. 243-260 ◽  
Author(s):  
Gautier Verhille ◽  
Ruslan Khalilov ◽  
Nicolas Plihon ◽  
Peter Frick ◽  
Jean-François Pinton

AbstractThe influence of an externally applied magnetic field on flow turbulence is investigated in liquid-gallium von-Kármán (VK) swirling flows. Time-resolved measurements of global variables (such as the flow power consumption) and local recordings of the induced magnetic field are made. From these measurements, an effective Reynolds number is introduced as ${\mathit{Rm}}_{\mathit{eff}} = \mathit{Rm}(1\ensuremath{-} \ensuremath{\alpha} \sqrt{N} )$, so as to take into account the influence of the interaction parameter $N$. This effective magnetic Reynolds number leads to unified scalings for both global variables and the locally induced magnetic field. In addition, when the flow rotation axis is perpendicular to the direction of the applied magnetic field, significant flow and induced magnetic field fluctuations are observed at low interaction parameter values, but corresponding to an Alfvèn speed ${v}_{A} $ of the order of the fluid velocity fluctuations ${u}_{\mathit{rms}} $. This strong increase in the flow fluctuations is attributed to chaotic changes between hydrodynamic and magnetohydrodynamic velocity profiles.


2012 ◽  
Vol 2 (10) ◽  
pp. 1-3 ◽  
Author(s):  
Praveen Kumar Gupta ◽  
◽  
Puspraj Singh Puspraj Singh ◽  
Puspraj Singh Puspraj Singh ◽  
P. K. Chamadia P. K. Chamadia

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