Response of the equatorial ionosphere in the South Atlantic region to the great magnetic storm of July 15, 2000

被引:192
作者
Basu, S [1 ]
Basu, S [1 ]
Groves, KM
Yeh, HC
Su, SY
Rich, FJ
Sultan, PJ
Keskinen, MJ
机构
[1] Air Force Res Lab, Space Vehicles Directorate, Hanscom AFB, MA USA
[2] Natl Sci Fdn, Div Atmospher Sci, Arlington, VA 22230 USA
[3] Natl Cent Univ, Inst Space Sci, Chungli 32054, Taiwan
[4] Naval Res Lab, Washington, DC USA
关键词
D O I
10.1029/2001GL013259
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The effects of the great magnetic storm of July 15, 2000 on the equatorial ionosphere have been studied by ground-based and satellite in-situ measurements. A large westward plasma drift in the evening equatorial ionosphere was observed as a result of the ionospheric disturbance dynamo. In that environment, the IMF Bz turned southward and presumably caused penetration of E-fields to low latitudes. This E-field initiated the onset of 250 MHz and L-band scintillations at Ascension Island (15 degreesW) and precipitous TEC decrease at Fortaleza, Brazil (38 degreesW), bounding the narrow longitude region in the South Atlantic. These impulsive ionospheric effects were extremely well correlated with abrupt decreases of SYM-H (1-min resolution Dst). The DMSP in-situ measurements showed the presence of severe ion density bite-outs extending over 30 degrees latitude in the South Atlantic Magnetic Anomaly region. The ROCSAT-1 satellite measured upward and large southward ion drifts in the same sector.
引用
收藏
页码:3577 / 3580
页数:4
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