The magnetospheric electric convection field refers to the electric field generated in the magnetosphere, which is the region of space around Earth dominated by its magnetic field. This electric field arises primarily from processes related to the interaction of the solar wind (a stream of charged particles, mainly electrons and protons, emitted by the Sun) with Earth's magnetic field. When the solar wind encounters Earth's magnetosphere, it can cause the magnetic field lines to be distorted and draped around the Earth.
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