W. Miyake et al., SOFT ION PRECIPITATION AT VERY HIGH-LATITUDES DURING NORTHWARD INTERPLANETARY MAGNETIC-FIELD, J GEO R-S P, 99(A8), 1994, pp. 15025-15033
During extended periods of northward interplanetary magnetic field (IM
F), soft ion precipitation was frequently observed at very high latitu
des (>80-degrees ILAT) on EXOS D (Akebono). The precipitating protons
typically had temperatures of a few hundreds of eV, and were accompani
ed by precipitating electrons with temperatures of several tens of eV.
The densities of the precipitating protons were of the order of 10(-1
) cm-3, and were usually lower than those of the electrons. During the
se periods, the ion convection at the highest latitudes was chaotic or
weak, but often had an average antisunward component. During periods
of strongly northward IMF, ion precipitation was observed at all magne
tic local times (MLT). A flux minimum, sometimes below the level of de
tection of the Akebono suprathermal mass spectrometer instrument, was
often found just poleward of the dayside auroral oval. This region is
believed to coincide with the open magnetic field lines in the tail lo
be. The region of ion precipitation was observed at auroral latitudes
on the dawnside when the IMF B(y) changed polarity from negative to po
sitive; it was located at higher latitudes (>80-degrees ILAT) on the d
uskside when the IMF B(y) was positive. These observations suggest a c
onnection between the ion precipitation and the auroral oval.