A magnetopause flows along the boundary between a
magnetic field, (see:
magnetosphere) and surrounding
plasma. It behaves roughly like a droplet of liquid exposed to supersonic flow. The magnetopause will ripple, flap, and sometimes droplets will break off. In terms of
planetary science, the magnetopause is the location where the outward
magnetic pressure of the Earth's magnetic field is counterbalanced by the
solar wind, a plasma. Most of the solar particles are deflected to either side of the magnetopause, much like
water is deflected before the
bow of a
ship. However, some particles become trapped within the Earth's magnetic field and form
radiation belts.
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