174 research outputs found
On the two-dimensional state in driven magnetohydrodynamic turbulence
The dynamics of the two-dimensional (2D) state in driven tridimensional (3D)
incompressible magnetohydrodynamic turbulence is investigated through
high-resolution direct numerical simulations and in the presence of an external
magnetic field at various intensities. For such a flow the 2D state (or slow
mode) and the 3D modes correspond respectively to spectral fluctuations in the
plan and in the area . It is shown that if
initially the 2D state is set to zero it becomes non negligible in few turnover
times particularly when the external magnetic field is strong. The maintenance
of a large scale driving leads to a break for the energy spectra of 3D modes;
when the driving is stopped the previous break is removed and a decay phase
emerges with alfv\'enic fluctuations. For a strong external magnetic field the
energy at large perpendicular scales lies mainly in the 2D state and in all
situations a pinning effect is observed at small scales.Comment: 11 pages, 11 figure
Finite dissipation and intermittency in magnetohydrodynamics
We present an analysis of data stemming from numerical simulations of
decaying magnetohydrodynamic (MHD) turbulence up to grid resolution of 1536^3
points and up to Taylor Reynolds number of 1200. The initial conditions are
such that the initial velocity and magnetic fields are helical and in
equipartition, while their correlation is negligible. Analyzing the data at the
peak of dissipation, we show that the dissipation in MHD seems to asymptote to
a constant as the Reynolds number increases, thereby strengthening the
possibility of fast reconnection events in the solar environment for very large
Reynolds numbers. Furthermore, intermittency of MHD flows, as determined by the
spectrum of anomalous exponents of structure functions of the velocity and the
magnetic field, is stronger than for fluids, confirming earlier results;
however, we also find that there is a measurable difference between the
exponents of the velocity and those of the magnetic field, as observed recently
in the solar wind. Finally, we discuss the spectral scaling laws that arise in
this flow.Comment: 4 pages, 4 figure
Méthode de Prédiction de la Capacité de Conservation des Semences
The invention relates to a method for the early evaluation of the preservation capacity of recently harvested seeds and/or of the resistance capacity thereof to an abiotic stress upon germination by quantifying L-isoaspartate residues in said seeds
Spectral energy dynamics in magnetohydrodynamic turbulence
Spectral direct numerical simulations of incompressible MHD turbulence at a
resolution of up to collocation points are presented for a
statistically isotropic system as well as for a setup with an imposed strong
mean magnetic field. The spectra of residual energy,
, and total energy,
, are observed to scale self-similarly in
the inertial range as ,
(isotropic case) and ,
(anisotropic case, perpendicular to the mean
field direction). A model of dynamic equilibrium between kinetic and magnetic
energy, based on the corresponding evolution equations of the eddy-damped
quasi-normal Markovian (EDQNM) closure approximation, explains the findings.
The assumed interplay of turbulent dynamo and Alfv\'en effect yields
which is confirmed by the simulations.Comment: accepted for publication by PR
Strong Imbalanced Turbulence
We consider stationary, forced, imbalanced, or cross-helical MHD Alfvenic
turbulence where the waves traveling in one direction have higher amplitudes
than the opposite waves. This paper is dedicated to so-called strong
turbulence, which cannot be treated perturbatively. Our main result is that the
anisotropy of the weak waves is stronger than the anisotropy of a strong waves.
We propose that critical balance, which was originally conceived as a causality
argument, has to be amended by what we call a propagation argument. This
revised formulation of critical balance is able to handle the imbalanced case
and reduces to old formulation in the balanced case. We also provide
phenomenological model of energy cascading and discuss possibility of
self-similar solutions in a realistic setup of driven turbulence.Comment: this is shorter, 5 page version of what is to appear in ApJ 682, Aug.
1, 200
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