The dynamic behavior of disturbances in the vicinity of a pair of magnetically connected three-dimensional null points is examined. The aim is to investigate how nonlinear disturbances lead to strong localized currents that initiate magnetic reconnection at the separator. The problem is formulated in an incompressible cylindrical geometry by superposing arbitrary disturbance fields onto a “background” two-null field. Two different regimes are found for the dynamic evolution, depending on the relative strengths of the background magnetic and velocity fields. In one regime, disturbance pulses split into ingoing and outgoing components, which propagate along the background field lines. In the other “flux pileup” regime, a strong driving flow l...
In this review paper we discuss several aspects of magnetic reconnection theory, focusing on the fie...
Magnetic reconnection at a three-dimensional null point is the natural extension of the familiar two...
Context. The magnetic field in many astrophysical plasmas, for example in the solar corona, is known...
The dynamic behavior of disturbances in the vicinity of a pair of magnetically connected three-dimen...
The behaviour of magnetic perturbations of an initially potential three-dimensional equilibrium magn...
It is known that exact analytic solutions can be constructed for incompressible magnetic reconnectio...
The skeleton of an isolated null point in three dimensions consists of a 'spine curve' and a 'fan su...
Magnetic reconnection around three dimensional (3D) magnetic null points is the natural progression ...
The problem of incompressible, nonlinear magnetic reconnection in three-dimensional "open" geometrie...
Magnetic separators, which lie on the boundary between four topologically-distinct flux domains, are...
We are thankful to the Higher Education Commission (HEC, Pakistan) for their financial support to on...
Three-dimensional magnetic null points are ubiquitous in the solar corona and in any generic mixed-p...
Three dimensional magnetic null points are now accepted as important topological features at which m...
In two dimensions magnetic energy release takes place at locations where the magnetic field strength...
Here we detail the dynamic evolution of localized reconnection regions about 3D magnetic null points...
In this review paper we discuss several aspects of magnetic reconnection theory, focusing on the fie...
Magnetic reconnection at a three-dimensional null point is the natural extension of the familiar two...
Context. The magnetic field in many astrophysical plasmas, for example in the solar corona, is known...
The dynamic behavior of disturbances in the vicinity of a pair of magnetically connected three-dimen...
The behaviour of magnetic perturbations of an initially potential three-dimensional equilibrium magn...
It is known that exact analytic solutions can be constructed for incompressible magnetic reconnectio...
The skeleton of an isolated null point in three dimensions consists of a 'spine curve' and a 'fan su...
Magnetic reconnection around three dimensional (3D) magnetic null points is the natural progression ...
The problem of incompressible, nonlinear magnetic reconnection in three-dimensional "open" geometrie...
Magnetic separators, which lie on the boundary between four topologically-distinct flux domains, are...
We are thankful to the Higher Education Commission (HEC, Pakistan) for their financial support to on...
Three-dimensional magnetic null points are ubiquitous in the solar corona and in any generic mixed-p...
Three dimensional magnetic null points are now accepted as important topological features at which m...
In two dimensions magnetic energy release takes place at locations where the magnetic field strength...
Here we detail the dynamic evolution of localized reconnection regions about 3D magnetic null points...
In this review paper we discuss several aspects of magnetic reconnection theory, focusing on the fie...
Magnetic reconnection at a three-dimensional null point is the natural extension of the familiar two...
Context. The magnetic field in many astrophysical plasmas, for example in the solar corona, is known...