A POSSIBLE DRIVING SOURCE FOR TRANSIENT FIELD LINE OSCILLATIONS IN THE POSTMIDNIGHT SECTOR AT GEOSYNCHRONOUS ALTITUDES

Citation
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
Citations number
29
Categorie Soggetti
Geosciences, Interdisciplinary","Astronomy & Astrophysics","Metereology & Atmospheric Sciences
Journal title
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
ISSN journal
21699380 → ACNP
Volume
101
Issue
A11
Year of publication
1996
Pages
24719 - 24726
Database
ISI
SICI code
2169-9380(1996)101:A11<24719:APDSFT>2.0.ZU;2-9
Abstract
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.