Spectacular low- and mid-latitude electrical fields and neutral winds during a superstorm

被引:21
作者
Kelley, Michael C. [1 ]
Ilma, Ronald R. [1 ]
Nicolls, Michael [2 ]
Erickson, Philip [3 ]
Goncharenko, Larisa [3 ]
Chau, Jorge L. [4 ]
Aponte, Nestor [5 ]
Kozyra, Janet U. [6 ]
机构
[1] Cornell Univ, Sch Elect & Comp Engn, Ithaca, NY 14853 USA
[2] SRI Int, Menlo Pk, CA 94025 USA
[3] MIT, Haystack Observ, Westford, MA 01886 USA
[4] Geophys Inst Peru, Jicamarca Radio Observ, Lima, Peru
[5] Natl Astron & Ionosphere Ctr, Arecibo Observ, Arecibo, PR 00613 USA
[6] Univ Michigan, Dept Atmospher Ocean & Space Sci, Ann Arbor, MI 48109 USA
基金
美国国家科学基金会;
关键词
Magnetic storm; Solar wind; Thermospheric disturbances; Penetrating electric fields; EQUATORIAL PLASMA FOUNTAIN; GREAT MAGNETIC STORM; ADDITIONAL LAYER; F3; LAYER; IONOSPHERE; PENETRATION; REGION;
D O I
10.1016/j.jastp.2008.12.006
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
In November 2004, a major magnetic storm occurred, a lengthy portion of which was recorded by the Upper Atmospheric Radar Chain. On the 9th and 10th, the Jicamarca Radar detected the highest magnitude penetrating electric fields (+/- 3 mV/m) and vertical drifts (+/- 120 m/s) ever seen at this premiere facility. These large and variable drifts were highly correlated with the interplanetary magnetic and electric fields and created a double F layer on the dayside and unusual TEC behavior throughout the low-latitude zone. These solar wind-induced drifts both suppressed and generated irregularities at the magnetic equator at different times. Large-scale thermospheric disturbances were generated by high-latitude heating and tracked through the middle- to low-latitude zones where both parallel and perpendicular plasma drifts created major ionospheric changes. The auroral oval was located at a magnetic L shell of about three for many hours. (C) 2009 Elsevier Ltd. All rights reserved.
引用
收藏
页码:285 / 291
页数:7
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