The Relation Between Geomagnetic Storm (18 May 1910) and the Tail Structure of Halley's Comet (1910II)

Yan Lin-shan; Li Zhong-yuan; Gu Shun-yong

doi:10.11728/cjss1984.02.149

Volume 4 Issue 2

Apr. 1984

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Yan Lin-shan, Li Zhong-yuan, Gu Shun-yong. The Relation Between Geomagnetic Storm (18 May 1910) and the Tail Structure of Halley's Comet (1910II)[J]. Chinese Journal of Space Science, 1984, 4(2): 149-155. doi: 10.11728/cjss1984.02.149

Citation:

Yan Lin-shan, Li Zhong-yuan, Gu Shun-yong. The Relation Between Geomagnetic Storm (18 May 1910) and the Tail Structure of Halley's Comet (1910II)[J]. Chinese Journal of Space Science, 1984, 4(2): 149-155. doi: 10.11728/cjss1984.02.149

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The Relation Between Geomagnetic Storm (18 May 1910) and the Tail Structure of Halley's Comet (1910II)

doi: 10.11728/cjss1984.02.149 cstr: 32142.14.cjss1984.02.149

1.
Shanghai Observatory, Academia Sinical
2.
China University of Science and Technology

Received Date: 1983-04-11
Rev Recd Date: 1900-01-01
Publish Date: 1984-04-24

Abstract

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 H_γ 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.