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A statistical study of the likelihood of a super geomagnetic storm occurring in a mild solar cycle

Bin Zhuang YuMing Wang ChengLong Shen Rui Liu

地球与行星物理（英文）2018，Vol.2Issue(2)：112-119,8.

地球与行星物理（英文）2018，Vol.2Issue(2)：112-119,8.DOI:10.26464/epp2018012

A statistical study of the likelihood of a super geomagnetic storm occurring in a mild solar cycle

Bin Zhuang ¹YuMing Wang ¹ChengLong Shen ²Rui Liu¹

作者信息

1. CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei 230026, China
2. Synergetic Innovation Center of Quantum Information and Quantum Physics, University of Science and Technology of China, Hefei 230026, China
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摘要

关键词

solar cycle/super geomagnetic storm/repeat interval

Key words

solar cycle/super geomagnetic storm/repeat interval

引用本文复制引用

Bin Zhuang,YuMing Wang,ChengLong Shen,Rui Liu..A statistical study of the likelihood of a super geomagnetic storm occurring in a mild solar cycle[J].地球与行星物理（英文）,2018,2(2):112-119,8.

基金项目

We acknowledge and thank the World Data Center for Geomag-netism (Kyoto) for use of the geomagnetic stormDst database, and the Royal Observatory of Belgium (ROB) for use of sunspot number data. The CME catalog is generated and maintained at the CDAW Data Center by NASA and the Catholic University of America in cooperation with the Naval Research Laboratory. This work is supported by grants from NSFC (41774178, 41574165, 41421063, and 41274173), and the fundamental research funds for the central universities. （Kyoto）

地球与行星物理（英文）

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ISSN：2096-3955

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