Origins of the k-2 spectrum in decaying Taylor-Green magnetohydrodynamic turbulent flows

被引:10
|
作者
Dallas, V. [1 ]
Alexakis, A. [1 ]
机构
[1] Univ Paris Diderot, Univ Paris 06, Lab Phys Stat, Ecole Normale Super,CNRS, F-75005 Paris, France
关键词
MHD SIMULATIONS; SOLAR-WIND; SCALES;
D O I
10.1103/PhysRevE.88.053014
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
We investigate the origins of k(-2) spectrum in a decaying Taylor-Green magnetohydrodynamic flow with zero large scale magnetic flux that was reported by Lee et al. [Phys. Rev. E 81, 016318 ( 2010)]. So far, a possible candidate for this scaling exponent has been the weak turbulence phenomenology. From our numerical simulations, we observe that current sheets in the magnetic Taylor-Green flow are formed in regions of magnetic discontinuities. Based on this observation and by studying the influence of the current sheets on the energy spectrum, using a filtering technique, we argue that the discontinuities are responsible for the -2 power law scaling of the energy spectra of this flow.
引用
收藏
页数:7
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