A bow shock is a boundary between a
magnetosphere and an ambient medium. For stars, this is typically the boundary between their
stellar wind and the
interstellar medium.In a planetary
magnetosphere, the bow shock is the boundary at which the
solar wind abruptly drops as a result of its approach to the
magnetopause. The best-studied example of a bow shock is that occurring where the solar wind encounters the
Earth's magnetopause, although bow shocks occur around all planets. The Earth's bow shock is about 100-1000
km thick and located about 90,000 km from the Earth.
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