Auroral electrojets during severely disturbed geomagnetic condition on 24 August 2005

被引:4
|
作者
Singh, Anand K. [1 ]
Sinha, A. K. [2 ]
Saini, S. [1 ]
Rawat, Rahul [2 ]
机构
[1] ESSO Natl Ctr Antarctic & Ocean Res, Vasco Da Gama 403804, Goa, India
[2] Indian Inst Geomagnetism, New Panvel W, Navi Mumbai, India
关键词
Storm; Substorm; Auroral electrojets; SUBSTORMS; FIELD;
D O I
10.1016/j.asr.2014.11.034
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Very intense and highly dynamic eastward and westward currents flowing in the auroral ionosphere are traditionally monitored by the auroral electrojet indices -AU and AL, respectively. In this study we show that on occasions of intense magnetic activity, entire auroral oval could be dominated by the westward flowing currents, which lead to depression not only in AL index but also in supposedly positive AU index. During negative AU intervals, there could be up to similar to 20% underestimation of the total maximum intensity of the auroral electrojet represented by AE index(defined as AU - AL). A detailed investigation of a well-studied extremely intense event of 24 August 2005 has been carried out. Global prevalence of the westward auroral electrojet was clearly observed at the auroral latitudes during the unusually intense substorm (AL similar to -4000 nT) on the day. Moreover, along the noon meridian westward electrojet appeared in the auroral region whereas eastward electrojet shifted towards lower latitudes. This paper emphasizes that intense substorms are represented better by AL index than AE index. (C) 2014 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:1349 / 1355
页数:7
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