Slow mode shocks propagating in open and closed magnetic fields.

Physics

Scientific paper

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Magnetohydrodynamics: Magnetic Fields

Scientific paper

A 2-D MHD model is used to investigate the propagation of slow mode shocks in the open and closed magnetic fields of the meridional plane near the Sun. The solutions demonstrate that a forward slow shock could retain its slow shock characteristics into interplanetary space in the magnetically open region; however, it can evolve into an intermediate shock through the helmet-type current sheet to the open magnetic field.

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