Ionospheric effects preceding the October 2003 Halloween storm

被引:29
|
作者
Blagoveshchensky, DV
MacDougall, JW
Piatkova, AV
机构
[1] St Petersburg State Univ Aerosp Instrumentat, Dept Radio Engn, St Petersburg 190000, Russia
[2] Univ Western Ontario, Dept Elect & Comp Engn, London, ON N6A 5B9, Canada
关键词
magnetospheric storm; ionosphere; prediction; space weather;
D O I
10.1016/j.jastp.2005.10.017
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
The goal of this study is to reveal some ionospheric forerunners which occur prior to the expansion phase of any storm or substorm. Another task is to compare variations of two main ionospheric parameters, f(0)F2 and h(max)F2, on two chains of ionosondes located in Europe and North America during the interval 26-28 October 2003. This interval precedes the Halloween storm and includes its onset. Analysis is based on ionospheric data of the SPIDR system. The key findings are as follows. A positive peak of delta f(0)F2 occurs some hours before onset of a magnetic storm or substorm, where delta is a deviation from the quiet value. This peak can serve as a forerunner of disturbance development. Delta f(0)F2 peak amplitude reaches the sizes 20-100% of f(0)F2 values. Similarities of delta f(0)F2 variations on two chains are: (i) the delta f(0)F2 peak mentioned above occurs simultaneously as a rule before disturbances on both chains; (ii) similar delta f(0)F2 variations are observed on all of the mid-latitude (or high-latitude) ionosondes of each chain. Delta h(max)F2 variations are approximately the opposite of the f(0)F2 variations. Their amplitudes fall in the range 15-25% from the average h(max)2 value. This investigation is useful and important for the short-term prediction of Space Weather states. (c) 2005 Elsevier Ltd. All rights reserved.
引用
收藏
页码:821 / 831
页数:11
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