日侧磁扰动中亚暴活动的前兆

O.A Troshichev , A.L Kotikov , E.M Shishkina , B.D Bolotinskaya , E Friis-Christensen , S Vennerstrom
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引用次数: 4

摘要

利用格陵兰岛经向站链的磁资料和磁活动的al指数,研究了昼侧裂谷区的磁扰动与夜间极光区亚暴活动之间的关系。对14个孤立的和持续时间较长的亚暴的分析表明,在夜间极光带的亚暴发展之前,中午后部分西进气流的增强是伴随亚暴发展的。即使在IMF正By分量的不利影响下,西流也作为亚风暴前兆出现在北裂中。这些趋势将在午盘延续。为了解释间隙电流与极光电喷之间的关系,提出了中性层电流与正午Birkeland电流之间的联系。这种联系可以通过源区恰好作用于白天磁层顶内部来实现,这是由于地磁场与IMF的静止重联,源区下游流向尾磁层顶。
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Substorm activity precursors in the dayside magnetic perturbations

Magnetic data from a meridional chain of stations in Greenland and AL-indices of magnetic activity have been used to study the relationship between magnetic perturbations in the dayside cleft region and substorm activity in the night-time auroral zone. The analysis of 14 substorms, isolated and prolonged, has shown that intensification of westward currents in the postnoon sector of the cleft precedes or accompanies substorm development in the night-time auroral zone. Westward currents appear in the northern cleft as substorm precursors even under the adverse influence of the IMF positive By component. These currents trend to extend in the prenoon sector. To explain the relationship between the cleft currents and auroral electrojet the connection between neutral layer currents and noon Birkeland currents is proposed. This connection can be realized by means of the source region acting just inside the daytime magnetopause owing to stationary reconnection of geomagnetic field and IMF, the source region flowing downstream to the tail magnetopause.

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