
doi: 10.1007/bf00636465
Equations governing the coupling of the scalar and vector potentials for a resistive electron-positron plasma in a strong magnetic field are derived. It is shown that in the presence of magnetic shear, a tearing instability may occur. The latter can lead to magnetic field line reconnection and the formation of magnetic islands which could affect the dynamics of the pulsar magnetosphere.
magnetic field line reconnection, tearing instability, Ionized gas flow in electromagnetic fields; plasmic flow, strong magnetic field, resistive electron-positron plasma, formation of magnetic islands, magnetic shear, Galactic and stellar dynamics, Stability and instability of magnetohydrodynamic and electrohydrodynamic flows, vector potentials, pulsar magnetosphere
magnetic field line reconnection, tearing instability, Ionized gas flow in electromagnetic fields; plasmic flow, strong magnetic field, resistive electron-positron plasma, formation of magnetic islands, magnetic shear, Galactic and stellar dynamics, Stability and instability of magnetohydrodynamic and electrohydrodynamic flows, vector potentials, pulsar magnetosphere
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 5 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
