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The spectra of magnetohydrodynamic turbulence in collisionless plasma

M. A. Livshits, В. Н. Цытович

Open publisher page 29 citations

Abstract

The authors consider steady-stat e frequency spectra for Alfvén and magnetohydrodynamic waves created when the waves interact non-linearly. The principal form of non-linear interaction is scattering by plasma particles. A study is made of the stability conditions for the power-type spectra W ωΩ = (1/ω ν )W Ω . It is demonstrated that power-type spectra with ν ≥ 1 are stable; at ν = 1;2 the power-type nature of the spectrum is not disturbed during establishment of the steady state, as distinct from other values of ν.

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What this paper is about

The authors consider steady-stat e frequency spectra for Alfvén and magnetohydrodynamic waves created when the waves interact non-linearly. The principal form of non-linear interaction is scattering by plasma particles. A study is made of the stability conditions for the power-type spectra W ωΩ = (1/ω ν )W Ω . It is demonstrated that power-type spectra with ν ≥ 1 are stable; at ν = 1;2 the power-type nature of the spectrum is not disturbed during establishment of the steady state, as distinct from other values of ν.

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Available abstract

The authors consider steady-stat e frequency spectra for Alfvén and magnetohydrodynamic waves created when the waves interact non-linearly. The principal form of non-linear interaction is scattering by plasma particles. A study is made of the stability conditions for the power-type spectra W ωΩ = (1/ω ν )W Ω . It is demonstrated that power-type spectra with ν ≥ 1 are stable; at ν = 1;2 the power-type nature of the spectrum is not disturbed during establishment of the steady state, as distinct from other values of ν.

Key concepts: Magnetohydrodynamic drive, Physics, Spectral line, Plasma, Magnetohydrodynamic turbulence, Turbulence, Magnetohydrodynamics, Computational physics

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