A statistical study of the likelihood of a super geomagnetic storm occurring in a mild solar cycleOACSCD
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
CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei 230026, ChinaCAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei 230026, ChinaSynergetic Innovation Center of Quantum Information and Quantum Physics, University of Science and Technology of China, Hefei 230026, ChinaCAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei 230026, China
solar cyclesuper geomagnetic stormrepeat interval
solar cyclesuper geomagnetic stormrepeat interval
《地球与行星物理（英文）》 2018 (2)
日冕物质抛射内部热力学和动力学过程的模型反演研究
112-119,8
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.
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