Magnetic neutral sheets in weakly ionized interstellar gas are rapidly annihilated by ohmic diffusion. In this paper we extend the model to a sheared magnetic configuration, and show that the magnetic pressure associated with even a small nonzero field drastically reduces the reconnection rate of the reversing component
Electron-inertia effects on the magnetic field reconnection induced by perturbing the boundaries of ...
The problem of dynamic, three-dimensional magnetic reconnection is considered. Analytic “fan current...
Magnetic reconnection is at the root of explosive phenomena such as solar flares, coronal mass eject...
Magnetic reconnection plays an essential role in the generation and evolution of astrophysical magne...
The linear theory of magnetic reconnection demonstrates that the rate of energy release at an X-type...
We discuss the role of ambipolar diffusion for simple reconnection in a partially ionized gas, follo...
We consider the linear and nonlinear evolution of disturbed magnetic X-type neutral points. The prob...
We investigate favourable circumstances for fast magnetic reconnection in astrophysical plasmas base...
A linear theory is developed for the dissipation of the free magnetic energy in small disturbances i...
We investigate favourable circumstances for fast magnetic reconnection in astrophysical plasmas base...
We discuss the role of ambipolar diffusion for simple reconnection in a partially ionized gas, follo...
Fast magnetic reconnection refers to annihilation or topological rearrangement of magnetic fields on...
The problem of incompressible, nonlinear magnetic reconnection in three-dimensional "open" geometrie...
We investigate the dynamical relaxation of a disturbed X-type magnetic neutral point in a periodic g...
Electron-inertia effects on the magnetic field reconnection induced by perturbing the boundaries of ...
The problem of dynamic, three-dimensional magnetic reconnection is considered. Analytic “fan current...
Magnetic reconnection is at the root of explosive phenomena such as solar flares, coronal mass eject...
Magnetic reconnection plays an essential role in the generation and evolution of astrophysical magne...
The linear theory of magnetic reconnection demonstrates that the rate of energy release at an X-type...
We discuss the role of ambipolar diffusion for simple reconnection in a partially ionized gas, follo...
We consider the linear and nonlinear evolution of disturbed magnetic X-type neutral points. The prob...
We investigate favourable circumstances for fast magnetic reconnection in astrophysical plasmas base...
A linear theory is developed for the dissipation of the free magnetic energy in small disturbances i...
We investigate favourable circumstances for fast magnetic reconnection in astrophysical plasmas base...
We discuss the role of ambipolar diffusion for simple reconnection in a partially ionized gas, follo...
Fast magnetic reconnection refers to annihilation or topological rearrangement of magnetic fields on...
The problem of incompressible, nonlinear magnetic reconnection in three-dimensional "open" geometrie...
We investigate the dynamical relaxation of a disturbed X-type magnetic neutral point in a periodic g...
Electron-inertia effects on the magnetic field reconnection induced by perturbing the boundaries of ...
The problem of dynamic, three-dimensional magnetic reconnection is considered. Analytic “fan current...
Magnetic reconnection is at the root of explosive phenomena such as solar flares, coronal mass eject...
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