Oa. Troshichev et al., RELATIONSHIP OF THE IONOSPHERIC CONVECTION REVERSAL TO THE HARD AURORAL PRECIPITATION BOUNDARY, J GEO R-S P, 101(A7), 1996, pp. 15423-15432
Plasma drift and particle measurements from the DMSP spacecraft for th
e three Geospace Environmental Modeling (GEM) campaign periods (Januar
y 27-29, March 28-29, and July 20-21, 1992) have been used to study th
e relationship between the plasma convection reversal and the poleward
boundary of the diffuse auroral zone characterized by hard electron p
recipitation with energies greater than 0.45 keV. This boundary, named
the hard auroral precipitation boundary (or the HAP boundary) in this
paper, is often regarded as the ionospheric footprint of the boundary
between the central plasma sheet (CPS) and the boundary plasma sheet
(BPS). By examining simultaneous ion drift and particle measurements f
rom about 500 satellite passes we find that the large-scale plasma flo
w in the morning and evening sectors changes its direction within the
auroral oval at the HAP boundary. However, exceptions are found in the
early morning sector between 0300 and 0600 MLT, where the convection
reversal is sometimes (in 30% of the DMSP crossings) displaced polewar
d relative to the HAP boundary. It is shown that the shape of the regi
on bordered by the HAP boundary can be roughly represented by a circle
, whose size is influenced by the IMF B-z component. There is roughly
a linear correlation between the diameter of this circle and the cross
-polar-cap potential drop, with the best correlation coefficient of 0.
65 for winter season. Our study suggests that the HAP boundary corresp
onds to the magnetospheric boundary between the quasi-dipolar region a
nd the region with more stretched field lines, and the source of the r
egion 1 field-aligned current is located near the HAP boundary. A B-y-
dependent shift of the HAP boundary with respect to the noon-midnight
meridian is also found. In the northern hemisphere, the shift is dawnw
ard for positive B-y and duskward for negative B-y; in the southern he
misphere, the shift is opposite to that in the northern hemisphere.