Physics
Scientific paper
May 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agusmsa41a..07l&link_type=abstract
American Geophysical Union, Spring Meeting 2002, abstract #SA41A-07
Physics
2467 Plasma Temperature And Density, 2415 Equatorial Ionosphere, 2439 Ionospheric Irregularities, 2443 Midlatitude Ionosphere
Scientific paper
Large-scale plasma density depletions are typically associated with equatorial spread F (ESF) plasma irregularities in the nightside F region, especially in the post-sunset sector. Data from the Ionospheric Plasma and Electrodynamics Instrument (IPEI) onboard the ROCSAT-1 spacecraft reveal numerous cases of localized, discrete plasma density enhancements associated with regions of regular ESF plasma density depletion structures at 600 km altitude. Within these discrete regions, the plasma density may be enhanced by ~ 2-3 times above the background density. The density enhancement regions have sharp, distinct edges and appear to have similar scale sizes as plasma density depletions. They generally occur at edges of the regular plasma depletion region, poleward in latitudes and either earlier or later in local times. In all of the cases we examined so far, they occur in local times at least three-hours after the sunset. The ion velocity data within the density enhancement regions show upward plasma drifts perpendicular to the magnetic field, similar to those within adjacent plasma depletion regions. The magnetic field-aligned plasma flows are generally poleward within the density enhancement regions. We present observational characteristics of the density enhancements and discuss possible mechanisms in this paper.
Heelis Roderick A.
Huang Chan Chun
Le Guan
Pfaff Robert F.
Su Shangguo
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