Equatorial and low latitude ionosphere during intense geomagnetic storms

被引:10
作者
Mansilla, G. A.
机构
[1] Univ Nacl Tucuman, Fac Ciencias Exactas & Tecnol, Dept Fis, Lab Ionosfera, RA-4000 San Miguel De Tucuman, Tucuman, Argentina
[2] Consejo Nacl Invest Cient & Tecn, Buenos Aires, DF, Argentina
关键词
geomagnetic storms; equatorial anomaly; ionospheric storms;
D O I
10.1016/j.jastp.2006.07.005
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
An investigation is made in order to analyse the role of neutral gas composition in the equatorial and low latitude ionosphere during intense geomagnetic storms. To this end data taken by the Dynamic Explorer 2 satellite at 280-300 km (molecular nitrogen N-2 and atomic oxygen O concentrations, electron density and vertical plasma drifts) are used. The sudden commencements of the events considered occurred at 11:38 UT on March 1, 1982, 18:41 UT on November 20, 1982 and 16:14 UT on February 4, 1983. Vertical plasma drifts are the most important contributor to the initial storm time response of the equatorial F region. Neutral composition changes (expressed as an increase in the molecular species, mainly N-2) possibly play a predominant role in the equatorial and low latitude (10-20 degrees) decreases of electron density at heights near F2-region maximum during the main and recovery phases of intense geomagnetic storms. Delayed increases of electron density observed at daytime during the recovery phase may be also attributed to increases in atomic oxygen. At low latitudes possibly a combined effect of O increase and upward plasma drift due to enhanced equatorward winds is the responsible mechanism for the maintenance of enhanced electron density values. (C) 2006 Elsevier Ltd. All rights reserved.
引用
收藏
页码:2091 / 2100
页数:10
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