Tailward electrons at the lobe-plasma sheet interface detected upon dipolarizations

We report on highly asymmetric spectra of electrons observed at the lobe-plasma sheet interface in the near-Earth (R 10 keV) are occasionally detected flowing earthward counter to the above electrons. The large differences in the bulk flows result in an intense field-aligned current (FAC) downward into the ionosphere. The estimated vertical thickness of the FAC layer is found to be comparable to the relevant ion inertia length, leading us to propose that the tailward electrons sustain the downward FAC originating from the near-Earth X line driven by the Hall effects in magnetotail reconnection. Such a FAC structure is indeed shown by a three-dimensional Hall-MHD simulation to be located at the high-latitude edge of the plasma sheet. We also show the currents integrated over the Hall-FAC layer to be of significant amounts in the context of magnetosphere-ionosphere coupling.

[1]  R. Elphic,et al.  FAST observations of upward accelerated electron beams and the downward field-aligned current region , 2013 .

[2]  Y. Yamade,et al.  Field‐aligned currents generated in magnetotail reconnection: 3D Hall‐MHD simulations , 2000 .

[3]  R. Ergun,et al.  Microstructure of the auroral acceleration region as observed by FAST , 1999 .

[4]  R. Elphic,et al.  The auroral current circuit and field‐aligned currents observed by FAST , 1998 .

[5]  R. Elphic,et al.  FAST satellite observations of electric field structures in the auroral zone , 1998 .

[6]  R. Elphic,et al.  FAST observations in the downward auroral current region: Energetic upgoing electron beams, parallel potential drops, and ion heating , 1998 .

[7]  Rumi Nakamura,et al.  Structure and dynamics of magnetic reconnection for substorm onsets with Geotail observations , 1998 .

[8]  M. Fujimoto,et al.  Ion dynamics and resultant velocity space distributions in the course of magnetotail reconnection , 1998 .

[9]  T. Mukai,et al.  Observations of earthward streaming electrons at the trailing boundary of a plasmoid , 1997 .

[10]  T. Nagai,et al.  Highly collimated electron beams observed during quiet times , 1997 .

[11]  M. Fujimoto,et al.  Highly collimated electron beams in the dawn-flank of the magnetotail , 1997 .

[12]  Daniel N. Baker,et al.  Neutral line model of substorms: Past results and present view , 1996 .

[13]  Dan Winske,et al.  Hybrid simulations of collisionless reconnection in current sheets , 1994 .

[14]  James F. Drake,et al.  Transition to whistler mediated magnetic reconnection , 1994 .

[15]  J. Sauvaud,et al.  Low‐energy particle layer outside of the plasma sheet boundary , 1992 .

[16]  D. Klumpar,et al.  Counter‐streaming electrons at the geomagnetic equator near 9 RE , 1988 .

[17]  T. Eastman,et al.  Particle and field characteristics of the high-latitude plasma sheet boundary layer , 1984 .

[18]  T. Terasawa Hall current effect on tearing mode instability , 1983 .

[19]  T. Eastman,et al.  The plasma sheet boundary layer , 1983 .

[20]  B. Sonnerup Magnetic field reconnection , 1979 .