Observations of Earth's bow shock for low mach numbers

Physics

Scientific paper

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Scientific paper

Four anomalous Earth's bow shock locations observed during 1969 are studied, using plasma and magnetic field data from the European satellite HEOS-1. The results show that when no magnetic storms are present, the shock position is predicted with a good approximation by magnetohydrodynamic equations, making use of the magnetosonic Mach number of the solar wind. When magnetic storms are present, symmetric and asymmetric ring currents should be taken into account. For low magnetosonic Mach numbers (1 < MMS <~ 3), the magnetosheath magnetic field is characterized by the unusual absence of low frequency turbulence. This experimental result seems to indicate that under such conditions the bow shock is a laminar shock.

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