Article ID Journal Published Year Pages File Type
1768815 Advances in Space Research 2006 6 Pages PDF
Abstract
Fast magnetosonic waves dominate in the foreshock region with correlation coefficients between the ion flux and magnetic field magnitude r(F/B) > 0.7. In the magnetosheath, the plasma flow is mainly turbulent and the character of the turbulence is strongly controlled by the angle ΘBn between the bow shock normal and the interplanetary magnetic field direction. Behind quasi-parallel bow shocks (ΘBn < 45°), variations of the ion flux and magnetic field strongly increase. As the magnetosheath is a very inhomogeneous, anisotropic medium sensitive to the external conditions, different types of MHD-modes can be observed. Behind the quasi-perpendicular bow shock, mirror-mode waves are sometimes observed in the middle of the magnetosheath and near the magnetopause.
Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Space and Planetary Science
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