Three-dimensional simulations of turbulent spectra in the local interstellar medium

Three-dimensional time dependent numerical simulations of compressible magnetohydrodynamic fluids describing super-Alfvénic, supersonic and strongly magnetized space and laboratory plasmas show a nonlinear relaxation towards a state of near incompressibility. The latter is characterized essentially...

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Main Authors: D. Shaikh, G. P. Zank
Format: Article
Language:English
Published: Copernicus Publications 2007-07-01
Series:Nonlinear Processes in Geophysics
Online Access:http://www.nonlin-processes-geophys.net/14/351/2007/npg-14-351-2007.pdf
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author D. Shaikh
G. P. Zank
author_facet D. Shaikh
G. P. Zank
author_sort D. Shaikh
collection DOAJ
description Three-dimensional time dependent numerical simulations of compressible magnetohydrodynamic fluids describing super-Alfvénic, supersonic and strongly magnetized space and laboratory plasmas show a nonlinear relaxation towards a state of near incompressibility. The latter is characterized essentially by a subsonic turbulent Mach number. This transition is mediated dynamically by disparate spectral energy dissipation rates in compressible magnetosonic and shear Alfvénic modes. Nonlinear cascades lead to super-Alfvénic turbulent motions decaying to a sub-Alfvénic regime that couples weakly with (magneto)acoustic cascades. Consequently, the supersonic plasma motion is transformed into highly subsonic motion and density fluctuations experience a passive convection. This model provides a self-consistent explaination of the ubiquitous nature of incompressible magnetoplasma fluctuations in the solar wind and the interstellar medium.
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spelling doaj.art-96cd3a4e07d44b45b0af3670c53c124e2022-12-21T23:22:34ZengCopernicus PublicationsNonlinear Processes in Geophysics1023-58091607-79462007-07-01144351359Three-dimensional simulations of turbulent spectra in the local interstellar mediumD. ShaikhG. P. ZankThree-dimensional time dependent numerical simulations of compressible magnetohydrodynamic fluids describing super-Alfvénic, supersonic and strongly magnetized space and laboratory plasmas show a nonlinear relaxation towards a state of near incompressibility. The latter is characterized essentially by a subsonic turbulent Mach number. This transition is mediated dynamically by disparate spectral energy dissipation rates in compressible magnetosonic and shear Alfvénic modes. Nonlinear cascades lead to super-Alfvénic turbulent motions decaying to a sub-Alfvénic regime that couples weakly with (magneto)acoustic cascades. Consequently, the supersonic plasma motion is transformed into highly subsonic motion and density fluctuations experience a passive convection. This model provides a self-consistent explaination of the ubiquitous nature of incompressible magnetoplasma fluctuations in the solar wind and the interstellar medium.http://www.nonlin-processes-geophys.net/14/351/2007/npg-14-351-2007.pdf
spellingShingle D. Shaikh
G. P. Zank
Three-dimensional simulations of turbulent spectra in the local interstellar medium
Nonlinear Processes in Geophysics
title Three-dimensional simulations of turbulent spectra in the local interstellar medium
title_full Three-dimensional simulations of turbulent spectra in the local interstellar medium
title_fullStr Three-dimensional simulations of turbulent spectra in the local interstellar medium
title_full_unstemmed Three-dimensional simulations of turbulent spectra in the local interstellar medium
title_short Three-dimensional simulations of turbulent spectra in the local interstellar medium
title_sort three dimensional simulations of turbulent spectra in the local interstellar medium
url http://www.nonlin-processes-geophys.net/14/351/2007/npg-14-351-2007.pdf
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