Ion cyclotron and heavy ion effects on reconnection in a global magnetotail

Details Ion cyclotron and heavy ion effects on reconnection in a global magnetotail Ion cyclotron and heavy ion effects on reconnection in a global magnetotail

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004jgra..10909206w&link_type=abstract

Journal of Geophysical Research, Volume 109, Issue A9, CiteID A09206

Physics

28

Magnetospheric Physics: Magnetotail, Magnetospheric Physics: Numerical Modeling, Magnetospheric Physics: Storms And Substorms, Magnetospheric Physics: Magnetosphere/Ionosphere Interactions, Ionosphere: Ionosphere/Magnetosphere Interactions (2736)

Scientific paper

Finite ion cyclotron effects play a significant role in determining the dynamics of the neutral sheet. The demagnetization of the ions facilitates reconnection and produces an electric field perpendicular to the direction of the tail currents. This in-plane electric field drives field-aligned currents and an out-of-plane (or core) magnetic field in conjunction with the generation of flux ropes. In addition to these electromagnetic effects, it is shown that ion cyclotron effects lead to the preferential convection of plasma from the dawnside to the duskside. This convection is consistent with results from single-particle tracking but differs from ideal MHD treatment where the flow occurs symmetrically around the Earth. A physical manifestation of these asymmetric particle trajectories is the wrapping of the field-aligned current between the region 1 currents and the region 2 and/or region 0 currents. In addition, localized density enhancements and depletions are seen in the tail where the local heavy ion density can be substantially elevated over ionospheric conditions. Because of the local density variations, reconnection across the tail is inhomogeneous. Reconnection is initiated postmidnight and then sweeps across to the dawn and dusk flanks within a few minutes. Because of this spatial variation, the ejection plasmoid is actually U-shaped and the subsequent flux rope formation is highly skewed.

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