2009
DOI: 10.1103/physreve.79.066404
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Numerical study of the magnetic electron drift vortex mode turbulence in a nonuniform magnetoplasma

Abstract: A simulation study of the magnetic electron drift vortex (MEDV) mode turbulence in a magnetoplasma in the presence of inhomogeneities in the plasma temperature and density, as well as in the external magnetic field, is presented. The study shows that the influence of the magnetic field inhomogeneity is to suppress streamer-like structures observed in previous simulation studies without background magnetic fields. The MEDV mode turbulence exhibits non-universal (non-Kolmogorov type) spectra for different sets o… Show more

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Cited by 1 publication
(7 citation statements)
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“…We have adapted the nonlinear fluid code that was developed to study the evolution of MEDV modes in [23] in the presence of equilibrium electron density and temperature gradients, to also include a background gradient in the magnetic field [24]. Consequently, the energy stored in these gradients excite linear as well as nonlinear instabilities in a different manner, than that described in [23], because the nonlinear mode coupling interactions are significantly modified by the presence of both plasma and magnetic field gradients.…”
Section: Nonlinear Simulationsmentioning
confidence: 99%
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“…We have adapted the nonlinear fluid code that was developed to study the evolution of MEDV modes in [23] in the presence of equilibrium electron density and temperature gradients, to also include a background gradient in the magnetic field [24]. Consequently, the energy stored in these gradients excite linear as well as nonlinear instabilities in a different manner, than that described in [23], because the nonlinear mode coupling interactions are significantly modified by the presence of both plasma and magnetic field gradients.…”
Section: Nonlinear Simulationsmentioning
confidence: 99%
“…Evolution of anisotropic mode structures as described by kx and ky mode averaged over the entire turbulent spectrum in inhomogeneous MEDV turbulence. Initially, kx = ky. Progressive development of anisotropy kx > ky is ascribed to the presence of background gradients in magnetic and temperature fields for which the anisotropy angle 0 = tan Ref [24]). …”
Section: Anisotropic Inhomogeneous Modesmentioning
confidence: 99%
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