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One-dimensional hybrid simulations of current sheets in the quiet magnetotail

Journal Article · · Geophysical Research Letters
DOI:https://doi.org/10.1029/94GL01693· OSTI ID:159779
Hybrid simulations (kinetic ions, massless fluid electrons) have been performed of the magnetotail current sheet for parameters characteristic of the quiet magnetotail (v{sub D}, b{sub n}<<1). Here b{sub n} = B{sub n}/B{sub 0}, v{sub D} = (cEy/Bn)/v{sub i}, B{sub n} is the north/south (z) magnetic field, B{sub 0} the asymptotic value of the tailward (x) field and v{sub i} the ion thermal speed, where the magnetospheric coordinate system is used. It is shown that the current sheet is more stable than in previously examined cases with high v{sub D} and/or large b{sub n}. A clear single reversal in B{sub x} persists over the entire simulation and a B{sub y} component is created, with a slow rate of growth (hundreds of {Omega}{sub i}{sup {minus}1}, where {Omega}{sub i} = eB{sub 0}/m{sub i}c). This is many minutes in real time. It is suggested that the waves are due to an electromagnetic instability of the cross-field ion current. 14 refs., 3 figs.
OSTI ID:
159779
Journal Information:
Geophysical Research Letters, Journal Name: Geophysical Research Letters Journal Issue: 20 Vol. 21; ISSN GPRLAJ; ISSN 0094-8276
Country of Publication:
United States
Language:
English

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