Coexistence of Weak and Strong Wave Turbulence in Incompressible Hall Magnetohydrodynamics

被引:21
|
作者
Meyrand, Romain [1 ,2 ]
Kiyani, Khurom H. [2 ,3 ]
Gurcan, Ozgur D. [2 ]
Galtier, Sebastien [2 ,4 ]
机构
[1] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[2] Univ UPMC, Univ Paris Sud, PSL Res Univ,CNRS,Ecole Polytech, Univ Paris Saclay,Sorbonne Univ,Observ Paris,LPP, F-91128 Palaiseau, France
[3] Univ Warwick, Ctr Fus Space & Astrophys, Coventry CV4 7AL, W Midlands, England
[4] Univ Paris Sud, Dept Phys, F-91400 Orsay, France
来源
PHYSICAL REVIEW X | 2018年 / 8卷 / 03期
关键词
SOLAR-WIND; BICOHERENCE ANALYSIS; COLLISIONAL PLASMAS; ENERGY-TRANSFER; ALFVEN-WAVE; SPECTRUM; SIMULATIONS; ANISOTROPY; CASCADES; DENSITY;
D O I
10.1103/PhysRevX.8.031066
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We report a numerical investigation of three-dimensional, incompressible, Hall magnetohydrodynamic turbulence with a relatively strong mean magnetic field. Using helicity decomposition and cross-bicoherence analysis, we observe that the resonant three-wave coupling is substantial among ion-cyclotron and whistler waves. A detailed study of the degree of nonlinearity of these two populations shows that the ion-cyclotron component experiences a transition from weak to strong wave turbulence going from large to small scales, while the whistler fluctuations display a weak wave turbulence character for all scales. This nontrivial coexistence of the two regimes with two populations of waves gives rise to anomalous anisotropy and scaling properties. The weak and strong wave turbulence components can be distinguished rather efficiently using spatiotemporal Fourier transforms. The analysis shows that while resonant triad interactions survive the highly nonlinear bath of ion-cyclotron fluctuations at large scales for which the degree of nonlinearity is low for both populations of waves, whistler waves tend to be killed by the nonlinear cross-coupling at smaller scales where the ion-cyclotron component is in the strong wave turbulent regime. Such a situation may have far-reaching implications for the physics of magnetized turbulence in many astrophysical and space plasmas and probably beyond, where different waves coexist and compete to transfer energy nonlinearly, across scales.
引用
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页数:19
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