The influence of the Hall term in the generalized Ohm's law on the large-scale plasma flow during conditions of ongoing magnetic reconnection at the dayside magnetopause (MP) is investigated. Of special interest is the plasma flow behavior during the transition of the MP transition layer as the Hall effect grows in proportion to the viscous-resistive effects. The governing equations are solved approximately by an ordinary perturbation expansion in orders of large Reynolds and Lundqvist numbers. It is shown that the flow pattern is strongly dependent on the magnitude of the Hall parameter; as it approaches zero, the viscous-resistive solution is obtained, while for an ordering of the same magnitude as the resistivity/viscosity, the Hall effe...
Magnetic reconnection is at the root of explosive phenomena such as solar flares, coronal mass eject...
Magnetic reconnection driven by an out-of-plane shear flow is carried out based on the three-dimensi...
Abstract This thesis examines magnetic reconnection in the solar corona. Magnetic reconnection is ...
The influence of the Hall term in the generalized Ohm's law on the large-scale plasma flow during co...
The large-scale dynamics of plasmas is well described within the framework of magnetohydrodynamics (...
Context. The role of the Hall term in magnetic reconnection at line-tied planar magnetic X-points is...
Effects of out-of-plane shear flows on fast magnetic reconnection in Hall magnetohydrodynamics appro...
A typical property of magnetopause reconnection is a significant perpendicular shear flow due to the...
The Hall effect is a key component of collisionless reconnection. A previous study showed that a qua...
Plasma processes such as magnetic reconnection, turbulent regimes or dynamo-generated magnetic field...
Magnetic reconnection at the high-latitude magnetopause is studied using 2-1/2-dimensional (2-1/2-D)...
Abstract. Magnetic reconnection at the high-latitude magnetopause is studied using 2–1/2-dimensional...
In this Master's thesis the effect of magnetic reconnection at the magnetopause is investigated whi...
Abstract. We report on experimental observations that the two-fluid Hall dynamo plays an important r...
The stationary Riemann problem including dissipation in form of resistivity and viscosity for the re...
Magnetic reconnection is at the root of explosive phenomena such as solar flares, coronal mass eject...
Magnetic reconnection driven by an out-of-plane shear flow is carried out based on the three-dimensi...
Abstract This thesis examines magnetic reconnection in the solar corona. Magnetic reconnection is ...
The influence of the Hall term in the generalized Ohm's law on the large-scale plasma flow during co...
The large-scale dynamics of plasmas is well described within the framework of magnetohydrodynamics (...
Context. The role of the Hall term in magnetic reconnection at line-tied planar magnetic X-points is...
Effects of out-of-plane shear flows on fast magnetic reconnection in Hall magnetohydrodynamics appro...
A typical property of magnetopause reconnection is a significant perpendicular shear flow due to the...
The Hall effect is a key component of collisionless reconnection. A previous study showed that a qua...
Plasma processes such as magnetic reconnection, turbulent regimes or dynamo-generated magnetic field...
Magnetic reconnection at the high-latitude magnetopause is studied using 2-1/2-dimensional (2-1/2-D)...
Abstract. Magnetic reconnection at the high-latitude magnetopause is studied using 2–1/2-dimensional...
In this Master's thesis the effect of magnetic reconnection at the magnetopause is investigated whi...
Abstract. We report on experimental observations that the two-fluid Hall dynamo plays an important r...
The stationary Riemann problem including dissipation in form of resistivity and viscosity for the re...
Magnetic reconnection is at the root of explosive phenomena such as solar flares, coronal mass eject...
Magnetic reconnection driven by an out-of-plane shear flow is carried out based on the three-dimensi...
Abstract This thesis examines magnetic reconnection in the solar corona. Magnetic reconnection is ...