HIGHLIGHTS
SUMMARY
Instrumented spacecraft in the near-Earth`s magnetosphere detect significant dynamic variations in the magnetic_fields and plasma properties in response to variations in the solar wind (Araki, 1994; Araki et_al, 1997; Archer et_al, 2013; Blum et_al, 2021). An equilibrium state is found when the solar wind ram pressure balances the magnetic_field pressure at the stagnation point of the solar wind flow as argued by Chapman and Bartels and Alfvén. For describing the Earth`s magnetic_field the authors here ignore the small tilt of the magnetic axis with respect to the rotation axis. The . . .
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