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A model of nonlinear evolution and saturation of the turbulent MHD dynamo
A. A. Schekochihin
,
S. C. Cowley
,
G. W. Hammett
, J. L. Maron
, J. C. McWilliams
PPPL Computational Science
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Article
›
peer-review
77
Scopus citations
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Keyphrases
Nonlinear Evolution
100%
Nonlinear Saturation
100%
MHD Dynamo
100%
Magnetic Energy
66%
Low Density
33%
Galaxies
33%
Magnetic Energy Spectrum
33%
Magnetic Field
33%
MHD Turbulence
33%
Astrophysical Plasmas
33%
Kinetic Energy
33%
Eddies
33%
Weak Magnetic Field
33%
Kinematics
33%
Fully Developed
33%
Magnetic Perturbations
33%
Large-scale Magnetic Fields
33%
Velocity Scaling
33%
Magnetic Prandtl number
33%
Fokker-Planck Model
33%
Turbulent Media
33%
Physics
Magnetohydrodynamic Generator
100%
Magnetic Field
66%
Energy Spectra
33%
Kinetic Energy
33%
Astrophysical Plasma
33%
Prandtl Number
33%
Turbulent Medium
33%