Relationship between plasma bubbles and density enhancements: Observations and interpretation

被引:35
|
作者
Huang, Chao-Song [1 ]
Le, G. [2 ]
de La Beaujardiere, O. [1 ]
Roddy, P. A. [1 ]
Hunton, D. E. [1 ]
Pfaff, R. F. [2 ]
Hairston, M. R. [3 ]
机构
[1] Air Force Res Lab, Kirtland AFB, NM 87117 USA
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Univ Texas Dallas, Hanson Ctr Space Sci, Dallas, TX 75230 USA
基金
美国国家航空航天局;
关键词
Equatorial ionosphere; Plasma bubbles; Plasma enhancements; Plasma blobs; EQUATORIAL-SPREAD-F; LOW LATITUDE IONOSPHERE; NONLINEAR EVOLUTION; HINOTORI SATELLITE; IMPEDANCE PROBE; IRREGULARITIES; BOARD;
D O I
10.1002/2013JA019579
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Plasma bubbles are regions of depleted plasma density in the nighttime equatorial ionosphere. Plasma enhancements, also referred as plasma blobs, are regions where the plasma density is increased. It has not been well understood whether and how plasma enhancements are related to plasma bubbles. In this paper, we present the observations of plasma bubbles and enhancements by the Communication/Navigation Outage Forecasting System (C/NOFS) satellite during 2008 and 2009. In some cases, C/NOFS first detected plasma bubbles near the magnetic equator and then plasma enhancements at the same longitudes but at higher latitudes during subsequent orbits. In other cases, C/NOFS first detected plasma enhancements at off-equatorial locations and then plasma bubbles near the magnetic equator at the same longitudes. It is also found that plasma enhancements existed just above plasma depletions. We propose a unified scenario to describe the evolution of plasma bubbles and the formation of plasma enhancements. In the proposed scenario, plasma enhancements can occur at different latitudes and altitudes during the early, intermediate, and late stages of the bubble evolution. This scenario provides a reasonable explanation of the observations.
引用
收藏
页码:1325 / 1336
页数:12
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