Aims. This paper discusses the systematic drift of magnetic field lines under the influence of asymmetric turbulence where the asymmetry is caused by Alfvén wave helicity. Methods. The basic method of investigation is numerically tracing random magnetic field lines to discuss the average displacement of field lines owing to the asymmetric turbulence. Results. The main result is that as long as one has any non-zero degree of asymmetric turbulence, there is a systematic drift of field lines on average; an effect not seen when the turbulence is taken to be symmetric. This result implies that diffusion of field lines takes place relative to the mean drift and so alters the consequences for discussions of field line diffusion
"The transport dynamo mechanism, which describes the magnetic field generation by diffusion flow is ...
We perform direct numerical simulations of decaying magnetohydrodynamic turbulence subject to initia...
A gauge invariant and hence physically meaningful definition of magnetic helicity density for random...
A general quasilinear transport parameter for particle drift in arbitrary turbulence geometry is pre...
[1] We examine charged particle transport perpendicular to the large scale magnetic field. We find t...
The turbulent diffusion tensor describing the evolution of the mean concentration of a passive scala...
The random walk of magnetic field lines is examined numerically and analytically in the context of re...
Observations of magnetic reconnection at Earth's magnetopause often display asymmetric structures th...
Thesis (Ph.D. (Physics))--North-West University, Potchefstroom Campus, 2006.In the present study we ...
We use direct numerical simulations of forced MHD turbulence with a forcing function that produces t...
Abstract. It is well known that the structure of magnetic field lines in solar wind can be influence...
It is well known that the structure of magnetic field lines in solar wind can be influenced by the ...
The action of turbulence on a passive convected scalar field (e.g. temperature) or vector field (e.g...
It is shown that the turbulent dynamo $\alpha$-effect converts magnetic helicity from the turbulent ...
We investigate analytically the amplification of a weak magnetic field in a turbulent flow lacking r...
"The transport dynamo mechanism, which describes the magnetic field generation by diffusion flow is ...
We perform direct numerical simulations of decaying magnetohydrodynamic turbulence subject to initia...
A gauge invariant and hence physically meaningful definition of magnetic helicity density for random...
A general quasilinear transport parameter for particle drift in arbitrary turbulence geometry is pre...
[1] We examine charged particle transport perpendicular to the large scale magnetic field. We find t...
The turbulent diffusion tensor describing the evolution of the mean concentration of a passive scala...
The random walk of magnetic field lines is examined numerically and analytically in the context of re...
Observations of magnetic reconnection at Earth's magnetopause often display asymmetric structures th...
Thesis (Ph.D. (Physics))--North-West University, Potchefstroom Campus, 2006.In the present study we ...
We use direct numerical simulations of forced MHD turbulence with a forcing function that produces t...
Abstract. It is well known that the structure of magnetic field lines in solar wind can be influence...
It is well known that the structure of magnetic field lines in solar wind can be influenced by the ...
The action of turbulence on a passive convected scalar field (e.g. temperature) or vector field (e.g...
It is shown that the turbulent dynamo $\alpha$-effect converts magnetic helicity from the turbulent ...
We investigate analytically the amplification of a weak magnetic field in a turbulent flow lacking r...
"The transport dynamo mechanism, which describes the magnetic field generation by diffusion flow is ...
We perform direct numerical simulations of decaying magnetohydrodynamic turbulence subject to initia...
A gauge invariant and hence physically meaningful definition of magnetic helicity density for random...