The Transition of Interplanetary Shocks through the Magnetosheath
作者： A Szabo , CW Smith , RM Skoug
DOI: 10.1063/1.1618709
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摘要: WIND, ACE, IMP 8 and Geotail data shows that the magnetosheath signature of IP shocks is primarily a fast‐mode shock or pressure pulse with wide ramp. No model predicted secondary discontinuities could be identified above background fluctuation level. Even though interplanetary surface geometry significantly corrugated, this study suggests there no significant deceleration front in magnetosheath.
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