Final Technical Report ''Double discontinuities in space plasma''
Author(s) -
Y. C. Whang
Publication year - 2004
Publication title -
osti oai (u.s. department of energy office of scientific and technical information)
Language(s) - English
Resource type - Reports
DOI - 10.2172/823765
Subject(s) - classification of discontinuities , discontinuity (linguistics) , magnetohydrodynamics , physics , shock (circulatory) , magnetic field , inertial frame of reference , plasma , double layer (biology) , mechanics , classical mechanics , computational physics , layer (electronics) , materials science , mathematics , quantum mechanics , nanotechnology , mathematical analysis , medicine
This research used high-resolution magnetic field data to examine the interior structures of MHD shocks in interplanetary space and in the magnetotail; we discovered that a slow-mode shock is often followed by an adjoining rotational discontinuity layer on the postshock side. The thickness of each layer is of the order of a few ion inertial lengths. Such a compound structure is known as a double discontinuity. When the magnetic field rotates by several degrees per ion inertial length inside a thin layer, the Hall current term becomes important in the generalized Ohm's law. Steady state solutions based on the Hall-MHD theory have been obtained to show the merging of a rotational layer and a slow shock layer to form a compound structure like the observed double discontinuities
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