dorsal/arxiv
View SchemaWave turbulence in incompressible Hall MHD
| Authors | S. Galtier |
|---|---|
| Categories | |
| ArXiv ID | physics/0608227 |
| URL | https://arxiv.org/abs/physics/0608227 |
| DOI | 10.1017/S0022377806004521 |
Abstract
We investigate the steepening of the magnetic fluctuation power law spectra observed in the inner solar wind for frequencies higher than 0.5 Hz. This high frequency part of the spectrum may be attributed to dispersive nonlinear processes. In that context, the long-time behavior of weakly interacting waves is examined in the framework of 3D incompressible Hall MHD turbulence. The Hall term added to the standard MHD equations makes the Alfv\'en waves dispersive and circularly polarized. We introduce the generalized Els\"asser variables and, using a complex helicity decomposition, we derive for three-wave interaction processes the general wave kinetic equations; they describe the nonlinear dynamics of Alfv\'en, whistler and ion cyclotron wave turbulence in the presence of a strong uniform magnetic field $B_0 \ep$. Hall MHD turbulence is characterized by anisotropies of different strength. We show that electron and standard MHD turbulence can be seen as two frequency limits of the present theory but the standard MHD limit is singular; additionally, we analyze in detail the ion MHD turbulence limit. Exact power law solutions of the master wave kinetic equations are given in the small and large scale limits for which we have, respectively, the total energy spectra $E(\kpn,\kpa) \sim \kpn^{-5/2} |\kpa|^{-1/2}$ and $E(\kpn,\kpa) \sim \kpn^{-2}$. An anisotropic phenomenology is developed to describe continuously the different scaling laws of the energy spectrum; one predicts $E(\kpn,\kpa) \sim \kpn^{-2} |\kpa|^{-1/2} (1+\kpn^2d_i^2)^{-1/4}$. Nonlocal interactions between Alfv\'en, whistler and ion cyclotron waves are investigated; a non trivial dynamics exists only when a discrepancy from the equipartition between the large scale kinetic and magnetic energies happens.
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"abstract": "We investigate the steepening of the magnetic fluctuation power law spectra\nobserved in the inner solar wind for frequencies higher than 0.5 Hz. This high\nfrequency part of the spectrum may be attributed to dispersive nonlinear\nprocesses. In that context, the long-time behavior of weakly interacting waves\nis examined in the framework of 3D incompressible Hall MHD turbulence. The Hall\nterm added to the standard MHD equations makes the Alfv\\\u0027en waves dispersive\nand circularly polarized. We introduce the generalized Els\\\"asser variables\nand, using a complex helicity decomposition, we derive for three-wave\ninteraction processes the general wave kinetic equations; they describe the\nnonlinear dynamics of Alfv\\\u0027en, whistler and ion cyclotron wave turbulence in\nthe presence of a strong uniform magnetic field $B_0 \\ep$. Hall MHD turbulence\nis characterized by anisotropies of different strength. We show that electron\nand standard MHD turbulence can be seen as two frequency limits of the present\ntheory but the standard MHD limit is singular; additionally, we analyze in\ndetail the ion MHD turbulence limit. Exact power law solutions of the master\nwave kinetic equations are given in the small and large scale limits for which\nwe have, respectively, the total energy spectra $E(\\kpn,\\kpa) \\sim \\kpn^{-5/2}\n|\\kpa|^{-1/2}$ and $E(\\kpn,\\kpa) \\sim \\kpn^{-2}$. An anisotropic phenomenology\nis developed to describe continuously the different scaling laws of the energy\nspectrum; one predicts $E(\\kpn,\\kpa) \\sim \\kpn^{-2} |\\kpa|^{-1/2}\n(1+\\kpn^2d_i^2)^{-1/4}$. Nonlocal interactions between Alfv\\\u0027en, whistler and\nion cyclotron waves are investigated; a non trivial dynamics exists only when a\ndiscrepancy from the equipartition between the large scale kinetic and magnetic\nenergies happens.",
"arxiv_id": "physics/0608227",
"authors": [
"S. Galtier"
],
"categories": [
"physics.space-ph",
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],
"doi": "10.1017/S0022377806004521",
"title": "Wave turbulence in incompressible Hall MHD",
"url": "https://arxiv.org/abs/physics/0608227"
},
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