Is Nonhelical Hydromagnetic Turbulence Peaked at Small Scales?
- 24 October 2003
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 597 (2) , L141-L144
- https://doi.org/10.1086/380189
Abstract
Nonhelical hydromagnetic turbulence without an imposed magnetic field is considered in the case where the magnetic Prandtl number is unity. The magnetic field is entirely due to dynamo action. The magnetic energy spectrum peaks at a wavenumber of about 5 times the minimum wavenumber in the domain, and not at the resistive scale, as has previously been argued. Throughout the inertial range, the spectral magnetic energy exceeds the kinetic energy by a factor of about 2.5, and both spectra are approximately parallel. At first glance, the total energy spectrum seems to be close to k-3/2, but there is a strong bottleneck effect and it is suggested that the asymptotic spectrum is k-5/3. This is supported by the value of the second-order structure function exponent that is found to be ζ2 = 0.70, suggesting a k-1.70 spectrum.Keywords
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This publication has 31 references indexed in Scilit:
- Dynamic Nonlinearity in Large‐Scale Dynamos with ShearThe Astrophysical Journal, 2002
- New Regime of Magnetohydrodynamic Turbulence: Cascade below the Viscous CutoffThe Astrophysical Journal, 2002
- Simulations of Magnetohydrodynamic Turbulence in a Strongly Magnetized MediumThe Astrophysical Journal, 2002
- The Inverse Cascade and Nonlinear Alpha‐Effect in Simulations of Isotropic Helical Hydromagnetic TurbulenceThe Astrophysical Journal, 2001
- Scaling properties of three-dimensional isotropic magnetohydrodynamic turbulencePhysics of Plasmas, 2000
- The Generation of Magnetic Fields through Driven TurbulenceThe Astrophysical Journal, 2000
- Nonlocal Bottleneck Effect in Two-Dimensional TurbulencePhysical Review Letters, 1998
- Magnetic structures in a dynamo simulationJournal of Fluid Mechanics, 1996
- Nonlinear MagnetohydrodynamicsPublished by Cambridge University Press (CUP) ,1993
- Extended self-similarity in turbulent flowsPhysical Review E, 1993