Abstract

A simulation method to track the time evolution of coherent vorticity and current density, called coherent vorticity and current density simulation (CVCS), is developed for three-dimensional (3D) incompressible magnetohydrodynamic (MHD) turbulence. The vorticity and current density fields are, respectively, decomposed at each time step into two orthogonal components, the coherent and incoherent fields, using an orthogonal wavelet representation. Each of the coherent fields is reconstructed from the wavelet coefficients whose modulus is larger than a threshold, while their incoherent counterparts are obtained from the remaining coefficients. The two threshold values depend on the instantaneous kinetic and magnetic enstrophies. The induced coherent velocity and magnetic fields are computed from the coherent vorticity and current density using the Biot–Savart kernel. In order to compute the flow evolution, one should retain not only the coherent wavelet coefficients but also their neighbors in wavelet space, and the set of those additional coefficients is called the safety zone. CVCS is performed for 3D forced incompressible homogeneous MHD turbulence without mean magnetic field for a magnetic Prandtl number equal to unity and with 2563 grid points. The quality of CVCS is assessed by comparing the results with a direct numerical simulation. It is found that CVCS with the safety zone well preserves the statistical predictability of the turbulent flow with a reduced number of degrees of freedom. CVCS is also compared with a Fourier truncated simulation using a spectral cutoff filter where the number of retained Fourier modes is similar to the number of the wavelet coefficients retained by CVCS. It is shown that the wavelet representation is more suitable than the Fourier representation, especially concerning the probability density functions of vorticity and current density.

Highlights

  • Magnetohydrodynamic (MHD) turbulence is ubiquitous in astrophysical flows (Goldstein et al 1995, Brandenburg and Subramanian 2005), as hydrodynamic (HD) turbulence is in our daily life

  • We have developed the coherent vorticity and current density simulation (CVCS) method to track the time evolution of coherent vorticity and current density for 3D incompressible MHD turbulence, generalizing the CVS method for 3D incompressible HD turbulence previously introduced by Farge and Schneider (2001)

  • CVCS is based on the orthogonal wavelet decomposition of the vorticity and current density fields at each time step

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Summary

Introduction

Magnetohydrodynamic (MHD) turbulence is ubiquitous in astrophysical flows (Goldstein et al 1995, Brandenburg and Subramanian 2005), as hydrodynamic (HD) turbulence is in our daily life. To reduce the degrees of freedom of turbulent flows and computational load in numerical simulations, a wavelet-based approach, called coherent vorticity simulation (CVS), was introduced for incompressible HD turbulence (Farge et al 1999, Farge and Schneider 2001, Farge et al 2003). It was shown that only few degrees of freedom of both vorticity and current density, the coherent ones, well preserve the statistics of the total 3D MHD turbulence Using this extraction method at each time step and neglecting or modeling the incoherent contributions, the time evolution of the coherent vorticity and current density can be simulated if a safety zone is introduced as in the case of HD turbulence.

Coherent vorticity and current density simulation method
Orthogonal wavelet decomposition of 3D vector field
Coherent vorticity and current density extraction method
Wavelet filtered MHD equations
Numerical method
1.49 Â 10À2
Assessment of CVCS
Findings
Conclusions
Full Text
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