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Formation of Dawn‐Dusk Asymmetry in Earth's Magnetotail Thin Current Sheet: A Three‐Dimensional Particle‐In‐Cell Simulation
Author(s) -
Lu San,
Pritchett P. L.,
Angelopoulos V.,
Artemyev A. V.
Publication year - 2018
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1002/2017ja025095
Subject(s) - substorm , physics , current sheet , electric field , gyroradius , asymmetry , plasma sheet , electron , magnetic field , magnetic reconnection , flux (metallurgy) , computational physics , earth radius , magnetosphere , heliospheric current sheet , geophysics , interplanetary magnetic field , solar wind , magnetohydrodynamics , quantum mechanics , materials science , metallurgy
Using a three‐dimensional particle‐in‐cell simulation, we investigate the formation of dawn‐dusk asymmetry in Earth's magnetotail. The magnetotail current sheet is compressed by an external driving electric field down to a thickness on the order of ion kinetic scales. In the resultant thin current sheet (TCS) where the magnetic field line curvature radius is much smaller than ion gyroradius, a significant portion of the ions becomes unmagnetized and decoupled from the magnetized electrons, giving rise to a Hall electric field E z and an additional cross‐tail current j y caused by the unmagnetized ions being unable to comove with the electrons in the Hall electric field. The Hall electric field transports via E × B drift magnetic flux and magnetized plasma dawnward, causing a reduction of the current sheet thickness and the normal magnetic field B z on the duskside. This leads to an even stronger Hall effect (stronger j y and E z ) in the duskside TCS. Thus, due to the internal kinetic effects in the TCS, namely, the Hall effect and the associated dawnward E × B drift, the magnetotail dawn‐dusk asymmetry forms in a short time without any global, long‐term effects. The duskside preference of reconnection and associated dynamic phenomena (such as substorm onsets, dipolarizing flux bundles, fast flows, energetic particle injections, and flux ropes), which has been pervasively observed by spacecraft in the past 20 years, can thus be explained as a consequence of this TCS asymmetry.