O. Saka et al., A POSSIBLE DRIVING SOURCE FOR TRANSIENT FIELD LINE OSCILLATIONS IN THE POSTMIDNIGHT SECTOR AT GEOSYNCHRONOUS ALTITUDES, J GEO R-S P, 101(A11), 1996, pp. 24719-24726
Geosynchronous orbit data from charged particle analyzer (30- to 500-k
eV electron flux) and magnetometer instruments on board the 1984-129,
GOES 6, GOES 5, and 1982-019 satellites distributed in the midnight-to
-dawn sector are examined during a particle injection event that occur
red at 0820 UT on May 21, 1986. The injection was detected by 1984-129
in the midnight sector as a dispersionless and short-lived (duration
was 9 min) event. The injected electron cloud drifted eastward and was
detected by 1982-019 in the dawn sector. Meanwhile, the GOES 6 and 5
satellites were in the postmidnight sector between the satellites whic
h measured the electron flux. They observed transient field line oscil
lations during the periods when the azimuthal plasma pressure arising
from the electron cloud was in the postmidnight sector. It is suggeste
d that field-aligned currents are likely to be built up preferentially
by a divergence of diamagnetic currents in the region where the azimu
thal plasma pressure gradient dominates. It is argued that these curre
nts excite an azimuthally polarized transient field line oscillation.