magnetospheric convection
Quick Summary
Magnetospheric convection is the circulation of plasma within Earth's magnetosphere, driven by the transfer of momentum from the solar wind. This process involves plasma flowing parallel to the solar wind on the edges of the magnetosphere and returning towards Earth in its interior. This system acts as a secondary magnetohydrodynamic generator, producing significant electrical potential. This convection is crucial for phenomena like the auroral oval, where energetic particles precipitate into the atmosphere, creating the aurora. Magnetic reconnection is a primary driver of magnetospheric convection, more efficiently than viscous interactions.123
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geomagnetic fieldThe magnetotail current…two closed loops is called magnetospheric convection. This mechanism, together with the more important one due to reconnection, produces the tail current system.
Read More…two closed loops is called magnetospheric convection. This mechanism, together with the more important one due to reconnection, produces the tail current system.
Read More- geomagnetic fieldGeneration of a magnetospheric electric field
Magnetic reconnection drives magnetospheric convection much more efficiently than does viscous interaction. Consequently, all phenomena associated with convection are much enhanced over quiet times. Convecting particles approach closer to Earth before they are deflected by drift in the main field. Field-aligned currents and the ionospheric electrojets driven by…
Read MoreMagnetic reconnection drives magnetospheric convection much more efficiently than does viscous interaction. Consequently, all phenomena associated with convection are much enhanced over quiet times. Convecting particles approach closer to Earth before they are deflected by drift in the main field. Field-aligned currents and the ionospheric electrojets driven by…
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