Several energetic ion bursts were observed in the near-Earth magnetosheath
when the spacecraft was located at (-4.5, 18.6, -1.3) R-e on 14 January 199
6. The bursts appeared in the recovery phase of a moderate storm. One of th
em was singly ionized oxygen burst which lasted about 150 min and had a pea
k energy of about 250 keV. The oxygen event is characterised by strong impu
lsive increases in the oxygen flux with a nearly constant IMF orientation a
ngle (-45 degrees), whereas the energetic proton and helium ions essentiall
y disappeared. The oxygen burst exhibited strong field aligned streaming (a
ntiparallel to the magnetic field vector) whereas the hydrogen and helium b
ursts have a broad azimuthal angle distribution. These ion bursts exhibit l
ayer structures, the oxygen ions exist outside the layer of proton and heli
um ion. These observations suggest that energetic ions from the ring curren
t may leak out of the magnetosphere into the magnerosheath during storm rec
overy phase. (C) 1998 Elsevier Science Ltd. All rights reserved.