The Relation Between Geomagnetic Storm (18 May 1910) and the Tail Structure of Halley's Comet (1910II)
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摘要: 本文探讨1910年5月18日菉葭浜天文台所记录的一次地球磁暴的暴源;解释哈雷彗星凌日与磁暴开始时刻之差;分析哈雷I型彗尾的某些特征并讨论磁暴机制.Abstract: In this paper, the geomagnetic storm on May 18, 1910 recorded by Lu-Kia-Pang Observatory near Shanghai that didn't corne from solar activity but came from the effects of plasma tail of Halley's comet (1910II) is explained. The difference between the time of Halley's comet ingress (transit) and storm-onset is interpreted. By means of the Hγ component figure of geomagnetic field, we try to analyse the structure of plasma tail of Halley's comet and also discuss the mechanism of geomagnetic storm.
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